text:
Observations on the ATCA normally consist of a sequence of scans: a scan is a period of observing where the telescope configuration stays the same. A complete observation is made up of a number of scans. Observations typically alternate between scans on the scientifically interesting sources and scans on one or more calibrators. The configuration of the scans and their order are kept in a schedule file.
The main observing task, caobs, reads the schedule file in order to determine what sources are to be observed, for how long, and in what order. The schedule file also defines the frequencies and correlator setup for each scan and can also be used to make the system automatically execute commands. The ATCA web scheduler is the tool to use to create ATCA schedule files in the CABB era. Schedules made with the old sched program are no longer understood by the CABB version of caobs and thus cannot be used. However, it is possible for the web scheduler to read in old schedules and save them for use with the new system. Please also note that an active ATNF username and password is required to gain access to the web scheduler page.
Generally, users will want to prepare at least two schedule files:
A schedule file for setting up (delay calibration etc.) and flux density calibration. It should include the appropriate flux density calibrator (SectionĀ2.2.4), and if the flux density calibrator cannot be used as a bandpass calibrator, another stronger calibrator that can be used for array setup and bandpass calibration.
A schedule file containing the science program source(s) and gain calibrator(s) (SectionĀ2.2.5).
You may also want to prepare contingency schedule files in case your preferred frequency is seriously affected by interference, or the selected calibrator proves to be resolved.
If your goal is to make a high-quality image of a source that has an angular extent much smaller than the size of the primary beam of the ATCA antennas, then you should observe your source in "snapshots". The same strategy can be applied if you want to image a small number of sources that are separated in the sky.
Snapshot observations will allow you to obtain a wide range of uv coverage without having to spend all your observing time on source. This is necessary because you will need to obtain calibration data within your time allocation. Generally, a snapshot consists of one or more calibration scans, followed by some integration time on the science target, followed by a gain calibration scan. These snapshots are repeated until your observations are complete.
Snapshot observing is best illustrated with examples.
This is essentially the simplest form of snapshot observing. All you need to do is integrate on the target, and occasionally visit a gain calibrator to ensure that you keep track of any phase changes. A single snapshot might therefore be:
2 minutes integration on a gain calibrator.
40 minutes integration on the target.
2 minutes integration on a gain calibrator.
This set of scans can be repeated as many times as possible within the allocated time.
These scans will give you enough data to properly calibrate the gains during your observing, and the polarisation as well, provided you get more than three snapshots in your allocated time. However you will need to spend some time observing the flux density calibrator (which also works as a bandpass calibrator) at some time during your allocated time.
Imaging several sources is basically the same as imaging a single source, except you have multiple snapshot sets to get through. For each source that you have, you will have an associated nearby gain calibrator. Then, you will have multiple sets that look like:
2 minutes integration on gain calibrator for source 1.
20 minutes integration on the target source 1.
2 minutes integration on gain calibrator for source 1.
During the allocated observing time, each set of scans will be observed multiple times, but it is best to interleave them to ensure you get the widest possible coverage of azimuths and elevations for each set. And once again, you must remember to get some time on the flux density calibrator.
Changing to the higher frequency 7mm band means that you must start doing online pointing correction scans. The basic set of scans is still the same, as in example 2, but now you have to occasionally add in a pointing scan. For example, if your normal scan set takes 20 minutes (e.g. 16 minutes on source, 4 minutes on the gain calibrator), then you could observe this set three times between pointing scans, as it is recommended that you don't use a pointing solution for more than an hour.
If your sources are all within 20░ of each other, you may be able to find a single source that can be used as the pointing correction calibrator, and you will only need to do this once per hour.
If your sources are spread around the sky you will need to do a pointing correction for each source. If you are only visiting your sources once per hour, then the pointing correction scan can simply be built into your snapshot set. However if you are looking at each source multiple times per hour, but you want to observe the sources interleaved with each other, you will need to be careful.
Usually, when you do a pointing correction scan, the corrections that are determined
are applied immediately and all subsequent scans (well, those that have
Pointing set to "Offset") will use those corrections.
This would be a problem if you are observing a source that is more than 20░
away from the location of the most recent pointing scan, even if it was within 20░ of the
location of a pointing scan that was done less than an hour ago; such a scan would
use the wrong pointing corrections!
The solution to this is to set
Pointing to "Offpnt"
for the scan. In this case, caobs will find the most recent
pointing corrections that are close to the location of the current scan, and use those
corrections for that scan.
In the 3mm band, not only do you need to do pointing corrections every hour, you need to do frequent observations of the paddle. The frequency of your paddle observations is determined by the conditions during your allocated time, and is related somewhat to the required frequency of your gain calibrator observations. That is, if the atmosphere is turbulent, then you may only be able to spend a few minutes away from a gain calibrator. And in such a case, the system temperature may be changing on a similar timescale. It is therefore usually a good idea to include a paddle scan in every snapshot set. Such a set might look like this:
Measurement of the paddle.
2 minutes integration on the gain calibrator.
8 minutes integration on the target source.
Measurement of the paddle.
2 minutes integration on the gain calibrator.
Since the apparent brightness of the sources you are observing will depend on the system temperature measured by the paddle scan, it is very important to ensure that you do the paddle measurement before you observe the sources. It is however not really necessary to ensure the measured amplitudes are accurate before doing a pointing scan.
If the source you will image is bigger than a small fraction of the ATCA primary beam, or the region you want an image for is considerably larger than the primary beam, you will need to use the ATCA's mosaicing functionality.
In interferometry adjacent pointings are not independent and so we can get fundamentally better images by processing the different pointings together. Necessary information about the pointing grid pattern to use for proper Nyquist sampling and the time to be spent on each position to optimise tangential uv coverage can be found in Chapter 21 of the Miriad Users Guide.
For close-packed mosaicing (pointing centres every half-beamwidth), drive times are determined by the acceleration limit of 800░/min▓. Half the drive time is spent accelerating and half decelerating. For drive times much further than 108′ in azimuth or 27′ in elevation, the drive times are dominated by the slew rate limits of 38░/min in elevation and 19░/min in azimuth. For example, a 16′ drive for a 16cm mosaic will take, depending on the elevation and azimuth of the source, approximately 2.2 seconds. Data taken during the off-source period is blanked in the correlator using a predicted drive time. As drive times can be a significant overhead, care should be taken to not move the array more than necessary.
Mosaicing is less useful if frequency switching is desired, as no frequency changes can occur during the mosaic scan. Since slew times are often much greater than the time it takes for the correlator to switch frequencies, the overheads involved in repeating a mosaic scan for each separate frequency might quickly negate the normal benefits of mosaicing.
Mosaicing mode can also be useful when a large number of nearby sources are to be observed, as observing overheads are reduced. Other applications include holography and source surveys using one dimensional cuts.
When scheduling a mosaic observation, the "snapshot" strategy should be used in order to get calibration data. That is, a point source calibrator should be observed periodically between observations of the mosaic pointings.
If you are mapping a very large, regularly-shaped region at low frequency, where the slew time between each pointing centre is dominated by the maximum speed of the antenna rather than the acceleration/deceleration rate, then you may get a significant reduction in overhead by using on-the-fly mosaicing.
On-the-fly (OTF) mosaicing has a couple of important differences to traditional mosaicing. Most importantly, although the mosaic pattern should be broadly the same – the hexagonal pattern is still the optimal sampling – the order of observations should be such that the telescope scans in a straight line for as long a distance as possible.
During an OTF mosaic, the phase center follows the mosaic points as specified, and the pointing center moves continuously across the pointings. In effect the primary beam of the antennas becomes elongated (to 1.5 beams) in the scanning direction.
To satisfy proper sampling of the sky, the antennas should not move by more than
half a beam per integration cycle, so the spacing of pointings in the mosaic file
should be the same as before. Because caobs assumes
you are scanning in rows or columns, the direction of scanning is inferred from
the next point. At the last point of a row or column the previous direction is
maintained to complete the scan. One extra point, marked with the name
TURN", needs
to be specified at the start of the next row/column, to allow for the antennas
to change direction and scan at the correct speed again.
The primary advantage of OTF mosaicing over regular mosaicing is its speed in covering a large area of sky, making it possible to get good uv coverage of a large field in a single observing run. It will not usually provide any better sensitivity than a carefully crafted regular mosaic.
Although OTF mosaicing is most useful at low frequencies where the slew time between mosaicing points are a significant fraction of the total integration time, this mode could also be used for mm observations by using bin mode and moving the antennas by e.g., 16 beams in a single integration with 32 time bins. The Miriad program atlod will need some work to properly record the phase center and pointing center in this case (ie. such a mode is not currently supported, but may be if demand for it is high).
Mosaic observations use a standard schedule file and an additional file,
called the mosaic file,
which lists the positions of the mosaic field centres.
Up to 2048 fields can be specified in a single file.
This mosaic file must consist of one line per pointing centre in the
mosaic pattern. Lines beginning with the "
#" character
are ignored and can be used for comments.
The general mosaic file format is:
# Comments .... ignored by the software # d(RA) d(DEC) INT $FIELD_1 d(RA) d(DEC) INT $FIELD_2 d(RA) d(DEC) INT $FIELD_3 d(RA) d(DEC) INT $FIELD_4
The items in each line are:
d(RA)" the offset Right Ascension of the pointing centre, in "degrees of polar rotation", from the reference position. For example,
d(RA) = +15.00will move +1 hr in RA at all declinations.
d(DEC)" the offset declination of the pointing centre, in degrees, from the reference position. e.g.
d(DEC) = +1.000will move the pointing centre one degree north.
INT" the integral number of integration cycles to spend on each pointing centre.
$FIELD_n" the name of the field. The "
$" symbol is a prefix to the field name, and indicates that scans will follow in the order as they are listed in the mosaic file. The field name must be different for each pointing centre and must have 9 or fewer characters (naturally, "
$" can not be used as the first character of the field name). Note: If you wish to use the "
mosaic" option in the Miriad task uvsplit (to keep the mosaic pointings together in one uv data file), the field name strings should differ by only the "
_n" part of the name, where "
n" is an integer. The field name given within the mosaic file does not need to match the source name given in the schedule file.
This file should be named "
mosnam.mos". The
.mos" suffix is required, or
caobs will not find the file. The
mosnam" part of the name
must match the source name given in the
schedule file.
To include a mosaic in a schedule file, insert a scan and set:
Source" to the name of the mosaic file, excluding the "
.mos" extension, i.e. "
ScanType" to "
RA" and "
Dec" to the reference position for the mosaic, i.e. the position that all the mosaic field centres are offset from. Check this carefully. Then check it again. Although the reference position is usually included as a comment in the mosaic file, caobs reads only the coordinate offsets from the mosaic file. Therefore, if the reference position is set incorrectly in the schedule file, caobs will not warn you, and your observations will fail.
All other scan settings have their usual effect, including the
Pointing" mode, and the observing
The mosaic file must be placed
in the
/atca/mosaic directory on xbones so
that caobs can locate it during the
observations. The mosaic file name must be completely in
lowercase letters, even if the corresponding source name in
the schedule has uppercase letters;
caobs will report that the mosaic file
could not be found unless it has an all-lowercase file name.
The "
.mos" suffix is required, or
caobs will not find the file.
The file can be copied into position manually, but there is also a web interface that will ensure your mosaic files are put in the correct location.
The time specified in the "
ScanLength" field
in the schedule file will determine how many times the mosaic
is looped through in a single scan. caobs
calculates this by dividing the "
time by the total length of the mosaic and rounding this to
the nearest integer; this will be the number of times the
mosaic is repeated during this scan. The mosaic is always observed at least
once, regardless of the "
It should be noted, in particular for mosaic files containing sources spread over a range of RAs, that if caobs encounters a source in that has set (or not risen), it will skip to the next scan in the schedule file, not to the next source in the mosaic file.
The following example shows a mosaic file specifying a four pointing centre pattern on a 0.25░ grid. Note that the RA offsets are coordinate increments not sky distances.
|Mosaic file:
# mymap.mos by P. Smith
# A four pointing centre mosaic
# Ref. Position = 05:21:33, -65:56:41
The scan in the corresponding schedule file might have the parameters:
|Scheduler fields:
With these settings, and with the default integration time of 10
seconds, the four pointing centres will be observed every 80 seconds.
Since the "
ScanLength" is 30 minutes, the mosaic will be repeated
23 times (22.5 is rounded up), but if the "
ScanLength" was 29.5
minutes, the mosaic would only be repeated 22 times (22.125 is rounded
Here is a 3x3 pointing grid around a source; we use 1934-638, but the same offsets could be used for any source.
0.0000 0.00 2 $@1934-on C -0.1812 -0.16 1 $TURN-10 -0.1812 -0.08 1 $1934-11 -0.1812 0.00 1 $1934-12 -0.1812 0.08 1 $1934-13 0.0000 0.16 1 $TURN-24 0.0000 0.08 1 $1934-23 0.0000 0.00 1 $1934-22 0.0000 -0.08 1 $1934-21 0.1812 -0.16 1 $TURN-30 0.1812 -0.08 1 $1934-31 0.1812 0.00 1 $1934-32 0.1812 0.08 1 $1934-33
Note that you can specify a non-scanning position in an OTF mosaic file by starting
the field name with a "@", like the 2 cycle calibration on
1934-on" above. Also
note the fields marked with "
TURN" - these are the extra
points required at the
start of each scanning row/column to give the antennas time to get to the correct position
and scanning speed. They should be discarded when processing the data.
Note also that all other pointing centres in the OTF mosaic file are only observed for 1 cycle. This cannot be changed, since the antenna will be moving while it observes each pointing.
To use
the OTF mosaic mode, specify a scantype of
OTFMos" in the web scheduler and
put a mosaic file like the one above in "
/atca/mosaic" on
The Miriad tasks mosgen and atmos may be useful when you are preparing your mosaic file.
If you need to map a region of known size around a known sky location, you will want to use mosgen. It will overlap each pointing correctly with hexagonal tiling, and will ensure that the pointings are observed with minimal overhead.
If you have a number of specific locations you want to observe, you will want to use atmos, as it will ensure that the offsets are correct and that the route between the pointings is optimised (the "travelling salesman" problem).
We do not recommend that you manually calculate the offset positions for your mosaic. An error in calculating the offsets will likely ruin your observations. Such an error is easily avoidable by using the Miriad tasks.
How large the mapping region is will determine whether you can image using standard snapshot observations, or if you will need to use mosaicing. In either case, the imaging strategy is no different to that of a continuum observation, but you may need more frequent calibration to ensure you get a sufficient signal to noise ratio for your lines; CABB's extra bandwidth doesn't help you observe a single line at known redshift!
If you're looking for your spectral line in one of the CABB continuum IFs, one of the most important things to consider is where the line to be observed will fall within the bandpass, ie. which channel(s) it will appear in. There are several channels in the CABB continuum IFs that are always flagged, and several more that are often contaminated with self-generated interference, and these should be avoided when observing spectral lines.
The CABB correlator always flags the centre continuum channel and each of the quarter-band channels. If you select a CABB mode that provides 1 MHz continuum channels, the flagged channels will be 513, 1025 and 1537. For CABB modes that provide 64 MHz continuum channels, the flagged channels will be 17, 33 and 49. You should avoid making the central CABB continuum frequency the same as the expected frequency of the line.
Self-generated interference will likely be present in the 1 MHz continuum channels 129, 157, 257, 641, 769, 1153, 1177, 1281, 1409, 1793 and 1921. All these channels can be easily flagged with the online correlator software (and they routinely are) and the interference does not leak into the adjacent channels.
If you are using the CABB zoom bands to detect your spectral line, you should again avoid using one of the continuum channels listed above, especially the quarter- and half-band channels. The zoom bands derived from those channels will usually have a very large spike at the centre of the zoom, and this spike may leak into adjacent channels since the zoom channels are not perfectly square.
It is important to note that ATCA is not able to Doppler track. You will need to ask for enough frequency coverage to ensure that your line will not drift out of the band due to observatory velocity changes.
Calibration of spectral-line observations is done with the same "snapshot" strategy that was described in SectionĀ2.3.2. It is important to note however that the calibration itself is slightly different. Because accurate measurements of a spectral line requires good bandpass characterisation, but in general you are dealing with much smaller bandwidths than for continuum observations, you will need to observe much brighter calibrators, observe the calibrators for longer, or observe the calibrators more often in order to get a sufficient signal-to-noise ratio.
There are many restrictions on the frequencies that can be observed with the CABB system. The most basic restriction is that only two 2048 MHz IFs can be observed simultaneously. All of the additional zoom bands must lie within these IFs, so they do not count as "extra" bandwidth. You can only specify the central continuum frequencies to the nearest MHz.
If you want to use the entire array at the same frequencies, then there are band-specific restrictions on the frequencies that can be observed.
In the 16cm band, the central frequency of each continuum IF must obey MHz.
In the 4cm band, the central frequency of each continuum IF must obey MHz.
In each of the mm bands, the centre frequencies of the two continuum IFs cannot be separated by more than 6000 MHz, ie. MHz.
In the 15mm band, the central frequency of each continuum IF must obey MHz.
In the 7mm band, the central frequency of each continuum IF must obey MHz.
In addition, the IF centre frequencies must both be below 40673 MHz, or both be above 41227 MHz.
In the 3mm band, the central frequency of each continuum IF must obey MHz.
If you don't need all the baselines at each frequency, it is possible to split the array up
so you can observe in two bands simultaneously. For each of the two CABB
continuum IFs you can select a set of antennas to use with the
caobs command "
set band1_antennas".
In this way you can specify a frequency in IF1 that is in a different band
to the frequency specified in IF2. The antennas specified in the
band1_antennas" would use the IF1
band, while the rest of the array would use the IF2 band.
The primary restriction in this mode is the central site oscillator. Since there is only one central site oscillator that feeds the entire array's L86 modules, if you want to observe in more than one mm band simultaneously, both the frequencies must be observable with the same central site frequency.
You cannot observe in both the 15mm and 3mm bands simultaneously.
Observing in the 15mm and 7mm bands simultaneously is possible if the 15mm central continuum frequency obeys MHz, and the 7mm central frequency obeys either MHz, or MHz.
Observing in the 7mm and 3mm bands simultaneously is possible if the 7mm central continuum frequency obeys either MHz, or MHz, and the 3mm central frequency obeys either MHz, or MHz.
Since neither the 16cm or 4cm bands need the central site synthesiser, there are no special frequency restrictions when one of the simultaneous bands is 16cm or 4cm.
It isn't possible with CABB to observe more than 4096 MHz of bandwidth simultaneously, but it is possible to quickly switch between frequencies within a single band, and also to swap between different bands with only a moderate loss of simultaneity.
If you want to change frequencies, you will need to start a new scan in the schedule. This restriction makes it impossible to change frequencies within a mosaic. Whenever you change scans you will experience two integration cycles of overhead, and if you are changing frequencies within a band, this is the only applicable overhead. For example, if you changed your central continuum frequencies from 5500 & 7500 MHz to 6500 & 8500 MHz, you will only need to incur two cycles of overhead as the scan is changed.
There is also no extra overhead when changing the zoom band configuration, which is simply viewed as a change of frequency within the same band.
If you are changing bands, you will likely incur more overhead. In this case, the turret on the antennas will need to rotate to put the new receiver at the right position, and if you are changing to or from the 7mm band the mm receiver package will need to be moved using the translator as well. Turret rotations will usually add only a few cycles of overhead at most, since the turret can be rotating during the normal two cycle overhead that occurs at every change of cycle. Translating the receiver to go to or from the 7mm band takes much longer: between 2 and 3 minutes.
When you change bands you may also have to refocus the antenna by moving the subreflector. When going to or from the 4cm band, antennas CA03 and CA05 need to be refocused, and this takes approximately 90 seconds. When going to or from the 3mm band, antenna CA01 needs to be refocused, and will take approximately 40 seconds.
WARNING: Movement of the turret does produce wear on the bearing, and it would be extremely difficult to replace it should it fail. We therefore ask that observers not change bands more than once every 15 minutes.
To schedule an observation of a major planetary object, simply put
its name in the "
Source" field of a scan. During the observations,
caobs will interpret this name and calculate where the planet, Sun
or Moon is and point the array towards it.
The scheduler will not automatically calculate where the planet will be during
the scheduling process, unless you enter the appropriate date and LST or UTC and then
click on the "
Listing" tab. At this point, the
scheduler will determine the planet's position and fill the "RA" and
Dec" fields. Alternatively, you could use
the Miriad task planets.
It is useful to note again that the "
RA" and
Dec" fields are ignored by caobs
when the source name is recognised as a planet, the Sun or the Moon, as
caobs will compute the appropriate position for the body in
real time. There is no reason therefore to prefer absolute time scheduling when
observing planets.
Solar system objects differ from most astronomical sources in that the proper motions are large enough that the object position changes in the course of an observation. When observing such objects, the schedule file should be created in absolute time mode to ensure that caobs correctly tracks the object. caobs has the ability to phase track an object with a non-sidereal rate. Note, however, the pointing centre used during a scan does not track the source (the pointing centre used is the mid-position of the object during the scan). Thus the scans must be short enough that there is not significant motion of the source within the primary beam during a scan (the scheduler does not check this).
For minor bodies, caobs cannot compute a position, so the correct
position must be provided by the user. In absolute time mode, the scheduler
treats source names beginning with the @ symbol (eg. a source name of
@hbopp) as pointing to an external ephemeris file (eg. a file
Ephemerides for minor solar system bodies can be computed before scheduling using JPL's Horizons on-line system. Only the telnet (terminal-based) access method is described here, but there is also a web-interface method available from the web page that is self-explanatory.
Horizons asks the user a series of questions. To generate an ephemeris file for ATCA observations:
telnet horizons.jpl.nasa.gov 6775
First select an object by giving the source name (followed by a semi-colon for minor bodies) or by source number.
In response to prompts, select "
Ephemeris", then "
Observe", then "
Geo" to select geocentric RA/Dec ephemerides.
Give the start time of interest, in UTC, in the format suggested by the prompt. At the next prompt give the end time, and then the time increment; typically 1 hour is more than adequate, and the scheduler uses simple linear interpolation of the ephemeris values. The ephemeris supplied to the scheduler must start at least two time increments before the scheduled start time, and must extend beyond its end time.
Accept "
default output", and at the "
Select table quantities" prompt, enter "
1,20" to get RA, Dec, distance and velocity of the object.
Horizons will then display the ephemeris in the terminal. To get it to email the ephemeris, press "
q" and the main menu will be displayed again. Then select "
[M]ail" and enter the email address to send the ephemeris to.
To log out of Horizons, press "
Ctrl-D" (the terminal hangup signal).
The ephemeris file produced by Horizons needs to be massaged into the format that the scheduler requires. This is best achieved with the ephformat command available on xbones.
First, copy the ephemeris from the email sent by Horizons into a plain text file on xbones.
Run the command ephformat with no arguments.
At the first prompt, give the name of the text file with the Horizons ephemeris (including file extension). At the second prompt, give a short descriptive name for the output ephemeris file (excluding any file extension). ephformat will then write out the appropriate ephemeris file to "
$ATCA_EPHEM:file.eph" where "
file" is the name entered at the second prompt.
To use the ephemeris you just created in the schedule, enter the name of the
ephemeris (the "
file" name described in the last
dot point above), preceded by the "
@" symbol, into
the "
Source" field of the web scheduler.
There is a limit to how far the antennas can slew in azimuth. The limit arises because of all the cabling inside the antenna which passes up the centre of the structure to the receiving and cryogenic equipment in the vertex room. There is a limit to how far these cables can wrap around in either direction, (similar to the head of an owl).
The wrap limits for the ATCA antennas are CCW=152.5░ and CW=327.5░ as shown in FigureĀ2.1.
It is a good idea to check what wrap the telescope is in at the start of your observations, as "unwrapping" can take up to 10 minutes. To determine the wrap you are in, consult MoniCA or atdrivemon. MoniCA shows the wrap explicitly, on the "ATCA Summary" page. atdrivemon shows the azimuth using the ATCA convention — while in the South wrap azimuths are expressed as positive angles, and negative angles in the North wrap.
The CABB web scheduler is used to prepare schedule files. The web scheduler checks the schedule for completeness and, where possible, checks choices such as observing frequency for hardware compatibility. Drive times, and source azimuths and elevations can also be computed to enable you to estimate overheads and observability.
Three steps are involved in using the web scheduler:
A new scan is added to the schedule.
The details of the scan are changed as desired.
When all the scans have been defined, the entire schedule is written to file.
When constructing a schedule, consider:
Is the sequence of sources sensible, and how much time is expended on slewing?
Does the schedule contain all the sources, and at the appropriate frequencies and bandwidths?
The web scheduler can produce a listing to help answer these questions.
It is a good idea to study these listings very
carefully before observing commences. The scheduler considers drive times:
all coordinate entries are automatically followed by a calculation of the
azimuth and elevation of the source, as well as the drive time from
the previous source, using the entered value for LST. When making
a schedule file, the integration times are specified
for each source (and calibrator source). Note that,
except in the case of mosaic schedules and
Dwell scan types,
these integration times
include drive times, so the specified time must be somewhat longer
than the amount of integration on source required. This is
particularly important for secondary calibrators, when the drive time
(up to a minute or so) may be comparable to the integration time
(one to three minutes). Alternatively, the
ScanType field can
be set to
Dwell to ensure a source or calibrator
is tracked for the specified scan duration.
The schedule file submitted to caobs (the online Compact Array control
task) need have no specific start time. Rather, the schedule file asks
caobs to start the first scan as soon as possible. The sequence of
scans will be exactly as specified in the schedule file. However, when
using the web scheduler, the calculation of azimuths, elevations and drive times
is possible only if the starting sidereal time is known (at least
approximately). The sidereal time for the first scan in the schedule
can be set in the web scheduler by giving the time in the
Time field,
and setting
TimeCode to
LST. Alternatively, the starting UT
may be specified by setting
TimeCode to
UT, and by setting
Date to the appropriate start date by clicking on it and using
the calendar that appears. Note that when viewing any scan other than the
first in the schedule, the fields
TimeCode and
Date all become read-only.
The environment flag can be used to instruct the online software to remember certain settings, such as attenuators, and to recall them whenever a scan with the same environment flag is encountered. However, this is generally not required, as the online software will remember user settings, and recall them when the same conditions are encountered again. There are at least 128 slots for user settings, so for a normal schedule, the environment flag will probably not need to be used.
See AppendixĀF for a complete guide to all the functionality available in the web scheduler.
Yes! In this section a simple continuum schedule file is constructed. It will contain three sources: a program source and two calibration sources. The following observing sequence will be specified:
Setup calibrator (0537-441, a catalogued source) for 5 minutes,
Program source (R.A. 05:21:35.5, Dec. -21:24:27.1 (J2000)) for 30 mins,
A gain calibrator for 5 minutes.
These sources will be observed at the standard 4cm band frequencies of 5500/9000 MHz. To create this schedule file, perform the following steps (instructions are given in bold, and the results of the instruction, or important caveats, and described below it):
- Navigate to the CABB web scheduler in a web browser.
The first screen is displayed.
Change the
Sourcefield to
test, the
RAfield to
05:21:35.5and the
Decfield to
The delimiter for coordinates must be a colon, and the default
J2000should only be changed if necessary.
ScanLengthto 00:30:00 and change the
This ensures that 30 minutes are spent on source, regardless of slewing times.
Pointingis set to
Offset pointing is not required for low-frequency observations.
Change the
Observerfield to
Wild, the
Projectcode to
These fields should be set in the first source - they will propagate to the other sources as they are added.
Change the
Timefield to
02:00:00, and the
TimeCodefield to
This indicates that the schedule will be started at an approximate LST of 2h.
Click the
Freq1 Setupbar.
This brings up the frequency selection fields.
5500in the
Continuumfrequency box, and keep the
Chn. BWselection box to
The velocity resolution should be calculated to be 55 km/s, and the velocity range will be 111632 km/s.
Click the
Freq2 Setupbar.
This brings up the frequency selection fields.
9000in the
Continuumfrequency box, and keep the
Chn. BWselection box to
The velocity resolution should be calculated to be 33 km/s, and the velocity range will be 68219 km/s.
Click the
Scan Parametersbar.
This brings up the scan details.
Click the
Search Calbutton.
This presents a list of nearby calibrators to the right of the scan details, sorted by distance to the source. The closest strong (> 1 Jy) source to the program source is shown to be 0454-234, at a distance of 6.02░.
Click on the
The details for this source are displayed from the calibrator database below the source list. This source is a suitable gain calibrator as it is strong, has a defect less than 0.1% and a closure phase less than 0.3%.
Click on the
0454-234button again.
Clicking on the button twice (without clicking another source button between clicks) inserts this source into the schedule above the currently selected source.
Select source 1, and change the
ScanLengthfield to 00:05:00. , To copy this source to the end of the schedule, click on the
Editmenu and select
Copy, then select the
testsource, click on
Editand select
The schedule should now have three sources (in order): 0454-234, test, 0454-234. The first source needs to be changed to 0537-441.
Select source 1
Change the
Sourcefield to 0537-441 and press
The scheduler will automatically put the source coordinates for this known calibrator in the
Click on the
Filemenu and select
Save As.
Schedule file selectorwindow will appear.
The schedule will be called c123_test.sch, so enter this into the
Filterbox to ensure that there is not already a schedule with this name.
If there is another schedule with the desired name, consider changing it.
c123_test.schinto the
Schedulebox and press the
The file selection window will disappear, and the name of the schedule should now appear at the top of the window.
To produce a listing of the schedule, in order to check that the
schedule proceeds as expected, click on the
Listing tab.
Yes! This example adds to the example from the previous section; ensure that the schedule created in the previous section is in the scheduler before continuing.
Now the aim is to observe 1 zoom band in each IF, each covering at least 70 km/s. The galaxy "test" is actually at an LSR recessional velocity of 25000 km/s, and these observations will look for CH3OH methanol and HC3N cyanoacetylene lines.
To create a schedule that can perform suitable observations for this situation, follow the steps:
- Select the first scan in the schedule.
This should be 0537-441.
Select the
Global changemenu item from the
Toolsmenu before changing the
Dateof this scan to 30/11/2014.
The date that the observation will be performed is required to ensure that the observatory velocity is computed correctly.
Hit the
Global Applybutton.
The date will now change for all the sources in the schedule.
Select the
Advanced viewmenu item from the
You should now see many more input fields.
Select the "
test" source in the schedule, then enter "
25000" into the
CatVelfield, and press TAB.
The entry in the
CatVelfield should now read "
25000 lsr radio" as the default frame is LSR, in the radio convention.
Click the
Freq1 5500MHzbar.
This brings up the IF1 frequency selection fields.
Click the topmost
This brings up the velocity calculator.
Select the
CH3OHline from the
Spectral Linedropdown box.
The rest frequency of this line (6668.518) appears in the
Rest Frequencybox below. The
Sky Frequencywill be updated to 6112.092 MHz, and the zoom band frequency will be calculated as the nearest half-MHz, in this case as
Click the
Applybutton in the velocity calculator.
The velocity calculator will disappear and information will be inserted into the first zoom band. In this case, the
6112MHz frequency translates into the channel
3273. The velocity resolution is given as 0.024 km/s, and the velocity range is listed as 49 km/s.
Select the zoom band width to be
2from the width drop box.
The velocity range now increases to 73.6 km/s.
Click the
Freq2 9000MHzbar.
This brings up the IF2 frequency selection fields.
Click the topmost
This brings up the velocity calculator as before.
Select the
HC3Nline from the
Spectral Linedropdown box.
The rest frequency of this line (9098.332) appears in the
Rest Frequencybox below, and the
Sky Frequencywill be updated to 8339.161 MHz. The zoom band frequency will be calculated to be
Click the
Applybutton in the velocity calculator.
The velocity calculator will disappear and information will be inserted into the first zoom band. In this case, the
8339MHz frequency translates into the channel
727. The velocity resolution is given as 0.018 km/s, and the velocity range is listed as 36 km/s.
Select the zoom band width to be
3from the width drop box.
The velocity range now increases to 71.9 km/s, comparable to the width provided for the IF1 zoom band.
Click the
Scan Parametersbar.
This brings up the scan details.
Select the
Master1option from the
FreqConfigdropdown box.
This signifies that the frequency configuration, including the zoom modes, from this scan, should be defined as the master configuration.
Select the
0537-441source from the schedule, then elect the
Slave-1option from the
FreqConfigdropdown box.
Now this scan will exactly mirror the frequency and zoom mode configuration from the
testscan, even if the configuration of the
testscan is changed. When a scan is set as a slave scan, the
Freqpanels will display a message describing which frequency and scan it is slaved to.
Select the
0454-234source from the schedule, then select the
Slave-1option from the
FreqConfigdropdown box.
Now this scan will exactly mirror the frequency and zoom mode configuration from the
At this point, the schedule would correctly describe a zoom mode observation.


text:
You will never want to leave this brand new, spacious, beautiful vacation home located in Solterra Community.
This home provides you with comfort, luxury and fun! The list of 'extra touches' is endless - themed decorations, leather chairs, unique decor pieces and ceiling fans are just the beginning.
Decorated in many appealing themes, such as Sea Side, Movies and Animated Characters, everyone in your party will enjoy coming back to this home after a day at the parks and shopping.
Tiled throughout the main area, you are welcomed into the open floor plan Kitchen, Living Area and Dining Area, with a view of the over sized lanai and screened in pool area.
The Gourmet Kitchen would be the envy of any chef with the following features:
Upgraded Black Appliances
Upgraded Stainless Steel Small Appliances
Marble Counter Tops
Beautiful Wood Cabinets
Cooking Utensils, Dishware and Crockery
Formal Dining Area with Seating for 8
Breakfast Bar with Seating for 4
The Main Living Area offers:
Comfortable Overstuffed Couches
Unique Decorations
Flat Screen Television w/Cable
DVD Player
The Garage Game Room has a Foosball Table, Billiard Table and High Top Bar Table w/2 Stools for relaxing!
Just up the stairs you will find the Entertainment Area which includes:
Large Sectional Couches
Flat Screen TV w/Cable
Gaming Table with Seating for 6
You will have to flip a coin over who sleeps where! The bedding layout of the home is unique and each room holds its own charm! There are three bedrooms downstairs and four bedrooms upstairs.
King Master Bedroom
(No TV in room at posting time)
2nd King Master Bedroom - Themed
Flat Screen TV w/Cable
3rd Downstairs Bedroom with Two (2) Queen Beds
Flat Screen TV w/Cable
1 Full Bath with Walk-in Shower
King Master Bedroom
En-Suite Bathroom
Flat Screen w/Cable
En-suite bath features Double Sinks & an Over Sized Walk In Shower
2nd King Master Bedroom - Themed
Flat Screen TV w/Cable
Access To Large Hall Full Bath
Bunk Room w/ Two (2) Double Sized Bunk Beds
(Total of 4 Double Beds)
En-Suite Bathroom
3rd King Master Bedroom
En-Suite Bathroom w/Tub & Shower
Additional extras in the home for your convenience include:
Free Wi-Fi
Local Telephone Calling
Cable Throughout the Home
Large Laundry Room w/Laundry Chute from Upstairs
Washer & Dryer (Full Size)
Iron & Ironing Board
Folding Table in Laundry Room
Vacuum/Broom & Mop
Last but certainly not least, you have the enjoyment of the pool area for those lazy afternoons. The extended lanai offers a great place for the family to gather and enjoy the pool.
You will want to call this vacation home, your home away from home, year after year!
PLEASE NOTE: During your stay, please be aware of on-going construction in the community and near your vacation home. Thank you.
Guest Reviews:
I reserved the property through FlipKey, and I must say the house exceeded my expectations. Gorgeous home! Everything you could imagine was in the home, plenty of space, quiet neighborhood, this was truly a great experience. I have started to plan next years vacation and this resort is definitely being considered again. I couldn't rate the house from the mobile site, however I would like to rate it a 5. Joe M.
Everything has been nice and clean so far! My family and I are having a great time, we look forward to doing this again. Bilal D.
We had our company team stay at Solterra, it was so convenient, clean and a lot of space. We will be staying here next year as well. Patricia G.
The house was absolutely beautiful. It accommodated my family wonderfully. I would definitely stay again and would definitely recommend it to my friends. Janelle E. (edited for space)
Thank you for your review, we have shared with our team and look forward to your next stay with us. Thank you
Thank you for your review, we have shared with our team and look forward to your next stay with us. Thank you again.
We have corresponded with the guest regarding their review and the 2 Star rating. The 2 Star rating was an accident and the guest said this was one of the best vacations they have ever had!

subset: commoncrawl


text:
Staples memberships could save you more | Learn More
Dress up your floor with this colorful and textured "Surya Oasis OAS1102 Hand Tufted Rug". The rich texture of this wool rug exudes sheer elegance, while the impressive transitional style reflects your unique taste. Its multiple shades give it an interesting, rich look that further adds to the overall beauty of this rug. Great for modern style set up and classic style decor, this color scheme complements both. This rug comes in rectangle shape and measures 3'3" x 5'3" to fit most spaces.
|Rug Primary Color
|Rug Material
|Rug Shape
|Rug Style


text:
In URS Corporation v. Atkinson/Walsh Joint Venture (No. G055271 filed September 26, 2017), Division Three of the Fourth Appellate District dealt with, for the first time, the question of whether an appeal of an attorney disqualification order results in an automatic stay of the trial proceedings and, if so, how far the automatic stay extends.
The underlying action involved a construction dispute between a contractor and subcontractor. During the pendency of that action, one party's counsel filed a motion to disqualify another party's counsel based on an alleged misuse of mediation-privilege protected documents. The trial court granted the disqualification motion and the disqualified counsel promptly filed a notice of appeal. The trial court then denied an application to stay proceedings pending the appeal, rejecting the assertion that the appeal automatically stayed the underlying proceedings.
Reprinted courtesy of Howard M. Garfield, Haight Brown & Bonesteel LLP and Renata L. Hoddinott, Haight Brown & Bonesteel LLP
Mr. Garfield may be contacted at email@example.com
Ms. Hoddinott may be contacted at email@example.com


text:
Donna Schlarb
2nd Grade Teacher
- Donna graduated from Bob Jones University with a B.S. in Elementary Education. Her 29 years of teaching has included 4th grade, 5th grade, and 2nd grade.
- Donna is married to Keith. They have three children and three grandchildren.
- In high school Donna was a cheerleader and a baton twirler. Another fun fact about our 2nd grade teacher is that she has visited Guam and one grandson is Canadian.
- In her spare time, Donna enjoys reading, hiking, driving through the country, symphonies in the park, watching the sun set at South Haven, and watching Notre Dame football.
"I pray that the second grade students will grow academically, spiritually, and socially and be prepared for third grade at the end of the year. My desire is to be used by God to meet the needs of my students. Also, I want to make learning fun."
Contact information: firstname.lastname@example.com
Upcoming Events
Feb22No School - IACS Bball TourneyAll Day
Mar1Spring Sports Fellowship6:30pm – 8:00pm
Mar8Storybook Day - K5-3rdAll Day


text:
Here's some #TuesdayMotivation to get out of your comfort zone–it's time for Stretching! This exciting Sketchbook Skool kourse is back by popular demand, and it's a great way to take your creativity to a whole new level. Watch the video, then go to http://sketchbookskool.com/kourses/stretching to enroll!
Want the Latest?
Subscribe to our zine for ideas, interviews, tips, news & inspiration emailed to you every couple of weeks:


text:
Spinnaker's Returns Management Consulting services help clients drive financial performance and enhance brand loyalty by providing an improved customer experience. We tailor our solutions to support your organization's unique strategic goals and objectives. Spinnaker strives to increase an organization's overall net recovery, streamline and align the forward and reverse supply chain, and enhance inventory management and control.
Spinnaker has proven methodologies and expertise to understand the specific business issues and opportunities, to identify gaps, and define the desired future state performance. Spinnaker consultants can help your organization strategically optimize returns to lower costs, reduce headcount, maximize recovery, mitigate risks, increase brand value, and ultimately drive product efficiency and innovation.
Spinnaker's Returns Management Consulting Services
- Returns Management Strategy & Roadmaps
- Reverse Supply Chain Design
- Returns Management Planning
- Technology Planning & Enablement
- Operational Performance Improvement
- Sustainability & Green Supply Chain
Spinnaker's consultative services range from highly strategic roadmaps to technology driven improvements and operational optimization. We take a holistic view of returns management to make sure the strategy, plans, and execution are aligned to drive optimal business results.
Contact us to learn more about how we can help improve the returns management process


text:
Are there any natural treatments that can help prevent hearing loss nerve damage or is this condition the same as presbycusis, which is a gradual loss of hearing as you age.
The answer to this question is a yes and a no.
Yes to the first part as there are several natural treatments that when they are combined may prevent this form of hearing loss, and no to the second part, as it is not the same as presbycusis.
The reason for this is really quite simple; you cannot reverse presbycusis once it has occurred, but you can prevent hearing loss nerve damage if you understand how it occurs.
To fully understand how natural treatments can prevent hearing loss nerve damage, it is extremely helpful to understand how your hearing process actually works.
Once you understand the full process, the natural treatments that can help begin to emerge as their benefits have been substantiated by a recent study that tackles this damage head on.
n humans and most all animals, hearing will occur when sound waves that are made actually reach the structures located inside of the ears.
Here these waves or vibrations are converted into signals.
Once they are converted into what is referred to as nerve signals, the brain will then convert them into recognizable sounds.
Your ear is made up of three major components; the outer, middle, and inner ear, and these sound waves pass through the outer ear which causes vibrations in your eardrum.
From here, the eardrum and the three small bones that make up your middle ear, referred to as the hammer, anvil, and stirrup, will amplify these vibrations as they travel to your inner ear.
Once they are there, they will then pass through a fluid located in your cochlea, which is a small snail-shaped structure that is found in your inner ear.
It is in this step that natural treatments for hearing loss nerve damage begin to emerge.
The reason is simple; there are thousands of tiny hairs attached to the nerve cells in your cochlea that will help to translate sound vibrations.
This is a huge step as the vibrations of various sounds can very easily affect these finite hairs in several different ways.
This can then cause these nerve cells to send several different signals to your brain.
It is this step that helps you identify and distinguish different sounds, but it also this step where hearing loss nerve damage can begin to develop.
There are several potential causes of hearing loss nerve damage.
However by far and away the most common are damages to your inner ear as the result of prolonged exposure to loud noises.
This will target and cause severe wear and tear in the cochlea and these finite hairs.
If these hairs or their nerve cells do become damaged, or worse yet go missing all together because of this noise, the electrical signals will not be transmitted properly.
This is the beginning step in the loss of your hearing.
The next potential cause is a ruptured eardrum, which is also the result of loud and sudden blasts of noise, as well as sudden drops in the pressure in your ears.
It can also be the result of poking or rupturing your eardrum with a sharp object, although this is very uncommon.
Other potential causes may include ear infections, bone growths of some type, and some medications, although these are also much less common.
The next steps in selecting which natural treatments can help you with hearing loss nerve damage are to understand typical decibel levels that may affect you.
Decibel levels are the intensity of these sound waves and the range begins at 30 which are the lowest, and this would be the sound range of some whispering to you.
A normal conversation would be 60 decibels, and 85 to 90 would be very loud traffic or a power mower. 95 to 100 would be a motorcycle or snowmobile.
110 would be a chain saw or a very loud rock concert.
Sirens measure in at 120 decibels, a shotgun blast at 165, and a rocket launch is even more dangerous than a rock concert, as it measures at 180 decibels.
From here, there are standards that have been set by the National Institute of Deafness as well as the National Institute for Occupational Safety and Health.
They have designed duration's of time spans depending on the decibel levels.
A 90 decibel range is set at 8 hours, 92 at 6, 95 at 4, and 97 at 3 hours. 100 decibels are maxed out after 2 hours, 105 after 1 hour, and 115 at 15 minutes.
From this chart is it very easy to see how very dangerous loud noises can be and how easily they can trigger hearing loss nerve damage.
The natural treatments for hearing loss nerve damage will all center around some key nutrients; vitamins A, C, and E, as well as several in the B-complex, and one mineral; magnesium.
There have recently been monumental studies conducted by the University of Michigan Health Services.
This has demonstrated that a combination of these nutrients taken on a daily basis prior to any excessive noise exposure can have dramatic effects on the damages to these nerves.
Vitamin A is considered to be one of the most potent, as it actually helps to nourish and feed your ears tissues.
In fact, as a baby forms in the womb, it is this vitamin that has the major responsibility in forming the ears.
A deficiency of vitamin A is also one of the leading causes of most all ear problems as well as a hearing loss.
Vitamins E and C are perhaps the most powerful anti-oxidants of any nutrient, and when they are combined, make a very powerful one-two punch in fighting free radical damages.
However, vitamin E goes even one step further in fighting hearing loss nerve damage as it is the major catalyst in delivering oxygen to the cells of your ears which can help in keeping your nerves healthy.
Vitamin B6 also plays a major role in this process, as it is critical in normal brain functions by creating neurotransmitters.
This allows your brain cells to communicate to each other when they are receiving messages of what sounds to send to your ears.
Vitamin B-9 also plays a major role as it is associated with age related hearing loss but it is also a key player in controlling high-pitched hearing loss.
It also with high frequency loss which is exactly what is occurring with this condition.
However, of all the B vitamins perhaps the real power player in hearing loss nerve damage is B-12, which is vital in the production of myelin.
Myelin is a fatty sheath like substance that is responsible for insulating your nerve fibers which in turn keeps your electrical impulses moving throughout your body.
If these impulses are not moving properly, your nerves in your ear are even more at risk.
The mineral magnesium, however, may be the most important of all these nutrients as it is has the major responsibility of transmitting electrical impulses across both your nerves and muscles.
When you combine all of these vitamins as well as magnesium into one form of attack against hearing loss nerve damage, you stand a much better chance of protecting the nerves in your ears.
Protecting your ears in the workplace with earmuffs in the form of earpieces can also control the decibel levels.
However the real protection comes internally with this combination taken once a day in the form of liquid vitamins and minerals.
Sources of Help for Hearing Loss Nerve Damage


text:
Customer Exclusive! Own a piece of this rare collection brought to you from Catherine Malandrino's original vault! Many of these beautiful items are one of a kind, exclusive and showcased by celebrities like Taylor Swift, Beyoncé and Kati Perry.
All items come with the Catherine Malandrino label sewn inside the garment as well as the original hang tag. Since some of these beautiful pieces are exclusive and were never put into production, many may not include the fabric content or care instructions. We have done our best on identifying the main fabric content for you. As with most luxury and high quality fabrics, we recommend dry cleaning as your method of care.
*Free Standard Shipping is valid on domestic orders placed on BHFO.com and must be selected during checkout. If you choose another shipping option, additional charges will apply. Our 20% off Catherine Malandrino Sale on BHFO.com is valid through November 30, 2015. Eligible customers must enter the promotion code CATHERINE20A during checkout to receive the discount. Discount will be deducted after code is applied. Shipping and handling and taxes will not be discounted. This promotion is not valid for orders placed on eBay or other marketplaces or on prior purchases. Offer is subject to change without notice.
Join our email list and be the first to hear about deals, trends, new brands and more. Plus, you'll get exclusive offers and discounts on your favorite brands.
The BHFO Story BHFO has come a long way since we began in 2003. Our vision was...
© 2019 BHFO, Inc. - Privacy Notice - Terms of Service
This store is PCI Compliant


text:
Microinnovative offers high quality data entry services and back office support for clients from all over the world. Finding the right and reliable company for data entry jobs is a tiresome task for business firms. Microinnovative, with our 4 years experience in the field, offers reliable data entry and data mining services which help you to saves time and money and focus on more profitable tasks.
1: Article Writing Services - 1$ / 100 words
2: Content Writing Services - 2$ / 100 words
3: Data Entry Services - 200$ per / month


text: Now that we're in the midst of the post-housing bubble foreclosure mess, it's easy to lose sight of part of how we got here: "liar's loans."Liar's loans were mortgages that didn't require the wannabe borrower to prove she could repay the loan. They came in various flavors, allowing the borrower to state without proving her income, or assets, or both. These loans violated all the basic principles of underwriting, the process banks abandoned during the housing bubble. And it's no wonder most are ending in foreclosure.And as a fax-email exchange first posted by the blog Foreclosure Fraud shows, the fraudulent nature of these loans was not only no secret at the banks, but bank staff steered applicants into filling out mortgage applications with false information. While I realize what follows is a single exchange, keep in mind when reading it that:• It involves a "Senior Loan Officer" -- how rogue can the behavior be?• The tone and details indicate this was a normal activity for at least this employee.• While it involves a JPMorgan Chase (JPM) loan, it cannot be true that Chase was the only mortgage lender behaving this way. Nothing that's come out to date about housing-bubble loans suggests Chase was unusually irresponsible. To the extent a big mortgage lender has gotten that rep, it's been Countrywide, which Bank of America (BAC) swallowed.• The borrower was sent documents and apparently was asked to sign them. Rather than sign them, the borrower asked questions. When reading the questions, think about the idea that the borrower was asked to sign these papers.• Finally, the borrower seems pretty sophisticated. Imagine how the process would work with a less sophisticated one. would they ask any of the questions?So, here are the key bits:On Sept. 25, 2006, aspiring borrower faxes Marc Bristol, senior loan officer of JPMorgan Chase Home Mortgage, regarding a mortgage application:"I have the following concerns with the documents you sent me:(1) I do not make $34,000 a month or anything close to this figure. I am not comfortable signing a document with a number I can not document in some form.(2) There are repeated mentions that this is an adjustable rate mortgage. I could find no mention of the frequency and amount of the adjustment. I need this.(3) I do not wish to escrow insurance or taxes. I will pay these.(4) Apparently this is a $417,000 first and a $70,000 second. Where are the documents for the second? What is the rate, how adjustable, what are the costs, what is the term? Why are we doing it this way?I will need the information and answers I have requested before I can execute and return the documents."And the borrower cc'd someone else, presumably a co-applicant, given Bristol's same-day emailed response, which is as follows:"Gentlemen, I hope all is going well you. [sic] This e-mail is in response to the fax you had sent me. I'll address each numbered concern:1. This is a stated-income deal. We had to state an amount that will be consistent through each deal. There are certain ratios that have to be met for income to debt. With [property 1] AND [property 2] AND taxes and insurance on your current, this is the figure that made the ratios fit. Since you have ample equity and assets, along with great credit, this where the luxury of a stated program comes in. It will not need to be documented. If there is a form 4506 (request for tax transcript) in the package that needs to be signed, it is only to verify that you FILE your taxes.2. This is a loan that is listed for 5 years. The initial fixed, locked-in rate will be good for 5 years. After that it turns into a 1 year adjustable, meaning that, on it's [sic] 1 year anniversary, it will adjust, adding an index (1 year LIBOR) and a margin (2.25%) together. The maximum cap is 5 years over the life of the loan.3. Escrows will be waived. The only reason they show up is for qualifying purposes. If they were on the Good Faith Estimate, I apologize. Please remove ANY "reserves deposited with lender" and initial.4. The route we took to get the absolute best rate, was keeping the first mortgage at a "conforming" or "conventional" amount. 417,000 is that maximum amount. Once it went to a "JUMBO" or "Non-Conforming" loan amount, the rate jumps .25%The second mortgage of 70,125 is to avoid mortgage insurance and allow you to put less down. The ideal goal would be to pay that one down and use it for future purchases.I appreciate all your business and want you to be as comfortable with me as possible. I know we've had some delays that seem a bit silly, but I guarantee that I'm laying the foundations for these deals and several more. Once we get these initial few closed, it's smooth sailing from there on out. If you'd prefer a sit-down sometime this week, please let me know. I know you gentlemen are busy, but I want you to be confident AND comfortable with me.Respectfully, -MarcMarc S. BristolSenior Loan OfficerJP Morgan Chase Home MortgageWhen I reached out to Chase for comment on this 2006 exchange, spokeswoman Daisy Cabrera said: "Our disciplined underwriting requires that we verify income on all mortgage applications." I'm sure that's true these days, and it was probably true pre-bubble, but as to those heady bubble days? The fax/email exchange speaks for itself.By ABIGAIL FIELD, DailyFinance


text:
New Jersey
Ocean County
Harvey Cedars Marina
Harvey Cedars Marina, New Jersey
Custom Search
Boating in New Jersey is such a fun thing to do. Harvey Cedars Marina is a very well liked marina by the folks from Barnegat Light. Famous New Jersey kindness and the very perfectly managed facilities makes the visit here worthwhile.
We should all go boating from time to time, and Harvey Cedars Marina is a good local marina if you happen to be in New Jersey. A visit to Dipper Point next to Harvey Cedars Marina is always a fine idea; people from Barnegat Light
love to come here. Beaches are good; and Little Beach near Harvey Cedars Marina is no exception, and a day of fishing at Barnegat Bay Fishing Charters is always a great idea. Spend the day on the beach at Island Beach since you're
here at Harvey Cedars Marina, and Manahawkin Lake is a delightful lake nearby. During your stay at Harvey Cedars Marina do go to close by Shore Beach, and an attention-grabbing thing to stop at in close proximity to Harvey Cedars Marina is Kinseys Pond. If you adore the outdoors, you'll adore Harvey Cedars Marina. A day at Long Beach close to Harvey Cedars Marina is time well spent, and in case you wish for fishing you can always pop by Miss Beach Haven Fishing
Charter. A pleasant beach in the neighborhood of Harvey Cedars Marina is Long Beach. A great deal of rain falls at Harvey Cedars Marina. July is the month that gets the most rain, and the driest of the months is February. During the
days of summer highs here at Harvey Cedars Marina reach the 80's. All through the moonlight hours it's usually in the 60's. The cold days of the winter come with highs in the 40's while the cold winter nights at Harvey Cedars Marina are in the 10's.
Detailed Map
Contact Info
Phone, Email, Address, GPS coordinates
Local weather forecast
These outdoors activities are available near Harvey Cedars Marina.
Marinas Near Harvey Cedars Marina:
Robbie's Loveladies Marina
, Beach Haven , 3 miles away
Surf City Marina
, Beach Haven , 3 miles away
Marina at Barnegat Light
, Barnegat Light , 4 miles away
Lighthouse Marina
, Barnegat Light , 4 miles away
High Bar Harbor Yacht Club
, Barnegat Light , 4 miles away
Causeway Boat Rentals
, Manahawkin , 4 miles away
Arnold's Escape Harbor Marina
, Beach Haven , 5 miles away
Campgrounds Near Harvey Cedars Marina:
Cedar Creek Campground
, Bayville , 10 miles away
Brookville Campgrounds
, Barnegat , 12 miles away
Sea Pirate Campground
, West Creek , 12 miles away
Bakers Acres Campground
, Tuckerton , 13 miles away
Baker's Acres Campgrounds
, Little Egg Hbr , 13 miles away
Hotels Near Harvey Cedars Marina:
Drifting Sands Hotel
, Ship Bottom , 3 miles away
Holiday Inn MANAHAWKIN/LONG BEACH ISLAND
, Manahawkin , 8 miles away
Sea Spray Motel
, Beach Haven , 11 miles away
Windjammer Motor Inn
, Seaside Park , 13 miles away
Comfort Inn Toms River
, Toms River , 14 miles away
Atlantic Inn
, Seaside Heights , 14 miles away
Cloud 9
, Seaside Heights , 14 miles away
Beaches Near Harvey Cedars Marina:
Long Beach
, Ocean County , 3 miles away
Little Beach
, Ocean County , 3 miles away
Long Beach
, Ocean County , 4 miles away
Shore Beach
, Ocean County , 5 miles away
Island Beach
, Ocean County , 8 miles away
Ski Areas Near Harvey Cedars Marina:
Hidden Valley
, New Jersey , 83 miles away, 620 foot drop, 4 lifts, 12 runs
Tuxedo Ridge
, New York , 83 miles away, 400 foot drop, 4 lifts, 7 runs
Mt. Peter
, New York , 83 miles away, 400 foot drop, 3 lifts, 11 runs
Mountain Creek
, New Jersey , 83 miles away, 1040 foot drop, 12 lifts, 46 runs
Spring Mountain
, Pennsylvania , 96 miles away, 420 foot drop, 6 lifts, 9 runs
Shawnee Mountain
, Pennsylvania , 97 miles away, 700 foot drop, 9 lifts, 23 runs
Whitewater Near Harvey Cedars Marina:
Whitewater Outfitter - Wild Cat Thrill Boat Ride
, Atlantic County , 26 miles away, Whitewater outfitter
Public Lands Near Harvey Cedars Marina:
New Jersey Pinelands National Reserve
, New Lisbon - NJ , 37 miles away
Gateway National Recreation Area
, Brooklyn - NY , 48 miles away
Golf Courses Near Harvey Cedars Marina:
Ocean Acres Country Club
, Manahawkin , 9 miles away
Cedar Creek-Berkeley Golf
, Bayville , 12 miles away
B L England Golf Course
, Ocean City , 12 miles away
Sea Oaks Country Club LLP
, Tuckerton , 14 miles away
Toms River Country Club
, Toms River , 15 miles away
Lakes Near Harvey Cedars Marina
Manahawkin Lake
, Ocean County , 8 miles away
Copyright © Stratus-Pikpuk, Inc.


text:
Thursday, November 26, 2015
The Nail Challenge Collaborative Presents: Monochrome - Non-Traditional Thanksgiving
34 comments:
Very non traditional but it looks great.ReplyDelete
Nice! Just wish that the stamping was a little less subtle, but if you wanted it that way then I'll shut up.ReplyDelete
Nice mani! I like the subtle-ness of the stamping. Looks great! :)ReplyDelete
Pretty combo! I really like it!ReplyDelete
This comment has been removed by the author.ReplyDelete
love this monochrome lookReplyDelete
Cute Love QuotesReplyDelete
Love Quotes for Her
Love Quotes for Him
Short Love Quotes
True Love Quotes
Romantic Love Quotes
SHAREit Apk
SHAREit Download App
SHAREit for PC
SHAREit App
SHAREit Download
SHAREit App Download
Happy Easter DayReplyDelete
Happy Easter Day
Happy Easter Day
Happy Easter Quotes
Happy Easter Images
Happy Easter Wishes
Easter Quotes
Easter Images
Easter Wishes
Happy Memorial Day
Happy Memorial Day
Happy Memorial Day Images
Happy Memorial Day Quotes
Memorial Day Images
Memorial Day Quotes
Happy Mothers Day
Happy Mothers Day
Happy Mothers Day
Happy Mothers Day Quotes
Happy Mothers Day Images
Happy Mothers Day Messages
Mothers Day Quotes
Mothers Day Images
Mothers Day Messages
Happy Holi Images
Happy Holi Messages
Happy Holi SMS
Holi Images
Holi Messages
Holi SMS
Hello! I would like to open cosmetology salon. Do you have an experience in this business? There are too many options in beauty salon equipment. Could you give me an advise? What companies are more reliable to buy galvanic facial for acne and cavitation ultrasonic machine?ReplyDelete
Happy mothers day 2017ReplyDelete
Mothers Day 2017 is celebrated on the second Sunday of May every year, so the 2017 edition of it will take place on May 14.
Happy Mothers Day 2017 Quotes
Best Happy Mothers Day 2017 Quotes in english for the celebration of this year Mothers day. Just select any of the Quotes from our collection.A mother is a person who, seeing there are only four pieces of pie for five people, promptly announces she never did care for pie. – Tenneva Jordan
mother's day gifts 2017
Great mother's day gifts 2017 Ideas For all that Mom does for her family, she deserves to be celebrated every day of the year but especially on Mother's Day.
Happy Mother's Day 2017 Gift Ideas
Happy Mothers Day 2017 Quotes
Happy Mother's Day 2017 cards
Happy Mothers Day 2017 Images Wallpapers Pictures
Mother's day SMS 2017 From Daughter
Cheap Mother's Day Flowers 2017
Mothers Day 2017 Quotes
Mother's Day Brunch 2017 Recipes Ideas
Mother's day 2017 SMS,status text messages
mother's day
Happy mothers day 2017
Mother's day 2017
Mothers day gifts
Mothers day gifts 2017
Mothers day quotes 2017
Happy mothers day quotes 2017
Mothers day images
Happy mothers day images 2017
mothers day poems 2017
mothers day cards2017
happy mothers day images 2017
Memorial Day 2017
Mothers Day 2017 Quotes In HindiReplyDelete
Happy Mothers Day 2017 Wishes In Hindi
Mothers Day Advance Wishes
Mothers Day Bollywood Songs List
Mothers Day FB Status For Mom
Mothers Day Surprise Ideas for Mom
Mothers Day 2017 Images In HD
This is really showing that Audi is trying to penetrate the market and trying to work around the ridiculous customs duties so the car becomes somewhat affordable.ReplyDelete
There is absolutely no doubt that these mid sized saloon are way ahead the build quality of the local Civics.
I've worked on and performance tuned many Audi's from the 1.2 TFSI's to RS6's. They are build to good standards and last.
In the UK you will still see many Audi's from 1997-2005 still running strong with huge miles. The interiors are robust and wear well. Bigg Boss 11 The paint is good. Very little goes wrong with them. They are built to last and the styling is timeless.
Anything to bring the prices down, be it make the car a little less on features is a welcome move from Audi. Great marketing strategy.
I really hope Audi pushes for lower custom duties. Happy new year 2018 It's a huge group (VAG) and should have the ability to use it's financial muscle to do something.
Bored of the numb driving experience of the Japanese cars.
The LEGO Ninjago Movie 2017ReplyDelete
Watch The LEGO Ninjago 2017 Full Movie Watch or Download Online for free on Ipad, Iphone, Mac Pro, Tablet, PC or any Devices From Any Where.
The LEGO Ninjago Movie Watch Online
The LEGO Ninjago Movie is a 2017 American animation-action, adventure film directed by Charlie Bean, Paul Fisher and written by Hilary Winston, with a story by Bob Logan.We start the week with news of that genre that likes big boys. Yes, the animation! It is that Warner Bros. Pictures revealed NINE posters of the LEGO® NINJAGO® Movie characters, a film by the same team that built "The LEGO Movie" and " LEGO Batman: The Movie "(The LEGO Batman Movie). Do not miss out!
The LEGO Ninjago Movie 2017
The LEGO Ninjago Movie Watch Online
The LEGO Ninjago Movie
The LEGO Ninjago Movie 2017
Watch The LEGO Ninjago Movie Online
The LEGO Ninjago Movie full Online
The LEGO Ninjago full Movie 2017 Online
The LEGO Ninjago full Movie 2017 Online
Watch The LEGO Ninjago full Movie 2017
LEGO Ninjago 2017 Full Movie
The film The LEGO Ninjago Movie: Warner Bros. Interactive and TT Games have announced the launch of LEGO Ninjago Movie – The Video Game for PlayStation 4, Xbox One, Nintendo Switch and PC on September 26. In it, players will be able to immerse themselves in the world of the new animated adventure for the big screen: The LEGO Ninjago Movie.
Developed by TT Games, in this new title players will break through waves of enemies in the skin of their favorite ninjas: Lloyd, Nya, Jay, Kai, Cole, Zane and Wu Sensei to defend Ninjago, their home island , By Lord Garmadon and his shark army. To achieve this, they must master the art of ninjagilidad, with which they can run through walls, jumping and fighting against enemies, to improve their classification and combat skills.
"The LEGO Ninjago Movie – The Videogame takes the incessant action and exciting combats of the feature film home so the children can embark on their own adventures. Enhanced moves will help players navigate Ninjago with the flow of a secret ninja warrior And refine their combat skills, "said Tom Stone, executive director of TT Games.
This is a topic which is close to my heart... Thank you! Will Like To Read More Like This.ReplyDelete
Watch Indian Dramas
Stream Sports Channels
Download Indian Tv Shows
Pinoy Tv Shows
Checkout My Websites Please And Tell Me How To Make Them Like Your's .
Use this article to increase your knowledge . cara menggugurkan kandunganReplyDelete
hi this topic is very good and clearReplyDelete
Pinoy tv
Pinoy Channel
Pinoy Tambayan
Kasam tere pyar ki
The topic "The Nail Challenge Collaborative Presents" is ver informative and cover its subject.ReplyDelete
ika-6 na utos
La Luna Sangre
Ang Probinsyano
Republic Day Advance Images 2018ReplyDelete
Republic Day Images 2018
Republic Day Songs
Republic Day Animated Images
Republic Day Speech
Admin Good Job. Nice workReplyDelete
thank u admin you share review with us wonderfullReplyDelete
Neha Babe is an Independent escorts in Noida with high profile here for your entertainment and fulfill your desires in noida call girls best service.ReplyDelete
noida escorts
call girls noida gallary
noida call girls profiles
escorts service rates in noida
neha babe contac for girl
mumbai escorts
nehbabe delhi escorts
bangaloe escorts
hyderabade escorts
ahmedabad escorts
Enjoyed reading the article above , really explains everything inReplyDelete
detail,the article is very interesting and effective.Thank you and good
luck for the upcoming articles
clipping path
clipping path service
background removal
raster to vector
The article you have shared here very good.ssc full from This is really interesting information for me. Thanks for sharing!ReplyDelete
Norton Customer ServiceReplyDelete
Avast Customer Service
McAfee Customer Service
Avast Contact NumberReplyDelete
McAfee Contact Number
Apple Support Number
iTunes Contact Number
Thanks for posting.ReplyDelete
Avast message keeps popping up
hp error 0xc18a0206
Avast error code 7005
Solve Installation Issue Due to Corrupted Setup Files via Avast Support Number
Norton Error 8504
prevent malwarebytes popups
print spooler service not running
microsoft edge virus
How to Solve HP Envy 5055 Error
Thank you so much for sharing this blog with us, it is really amazing valuable and informative.ReplyDelete
sound engineering course
Microsoft edge supportReplyDelete
Mozilla Firefox Support Phone Number
Quickbooks Support Phone Number
iTunes Contact Number
Apple Support Phone Number
Contact Quickboks online Support to help them advance business technology. To help them accounting in small and mid business.if customer any problem you can contact us on 18445519757. Quickbooks are always ready to assist you for any problem you face while using Quickbooks. There is always support option available on Quickbooks Support.
Quickbooks Online is a financial software it is designed to to slash the time to spend managing your finance by helping Quickbooks online. The first version of quickbooks online accounting software was a product released way back in the year 2004 by its parent company Intuit.Quickbooks online working in the cloud it is also a mobile technology data collection is a key to Quickbooks online Support. If you have any technical support you can contact us 18888857555.ReplyDelete
Thanks for posting this informative content here, it helped me a lot and will surely a lot of other people as well.ReplyDelete
Apple Helpline Number UK
Apple Support Number UK
If you are looking for instant full support for issues related to any Antivirus. You may contact Mcafee Antivirus support number for resolving all issues related to Mcafee Antivirus. Our experts are always present for any kind of Mcafee Antivirus help which you require instantly. The well-experienced and certified experts are available 24*7, to give the best support for your computer.ReplyDelete
mcafee internet security,
mcafee helpline phone number
This blog post will prove informative for a lot of readers; the writer deserves all the appreciation for the efforts made on this post.ReplyDelete
Avg Support Number UK
Avg Contact Number UK
McAfee Support Number UK


text:
CompTIA – Linux+ Certification
Test Drive our training programs
Exam Information
This instructor-led course will prepare students for the CompTIA Linux+ 2009 certification exam. It provides a comprehensive look at common tasks performed by system administrators. This includes installation, management of Linux systems from the command line and the GUI, user administration, file permissions, customization, software configuration, management of Linux-based clients, troubleshooting, and much more. Expanded coverage of networking and security are covered, which is in step with the 2009 CompTIA exam objectives
There are no prerequisites for this course. It is intended for IT professionals who are specializing in the Linux+ platform. Oracle and Novell recognize CompTIA's Linux+ certification in certain tracks.
Each online video class comes with the following features to prepare you for the exams listed below:
- Instructor lectures in a video classroom environment
- Printable Courseware
- 24×7 Learning Zone Live Mentor Support
Course Outline
|The Linux+ exam (XK1-003) is a substantive revision with updates on applications, networking, and security.
Our Expert Instructor
Kenneth Mayer – Certified CEH Trainer (CCSI, MCT, CCNP, CCDA)
Ken Mayer is a Microsoft Certified Trainer as well as a Certified Ethical Hacker Trainer and Security consultant. He started his career in computer technology in 1980s. He has offered a wide variety of IT training and high level consulting projects for Fortune 500 companies across the United States and Western Europe. He has achieved the Certified Cisco Systems Instructor certification. The CCSI certification involved a two-day lab and observation event held on Cisco in Paris, France Facility. This gave Ken the accreditation to be able to deliver Cisco Authorized Courses as a CCSI. He has taught the full line of Cisco CCNA, CCDA, CCNP, CCDP and CCIP course curriculums, including Cisco's security appliances such as PIX and IDS.


text:
If you are interested in the low-carb, moderate protein, high-fat, ketogenic diet, then this is the podcast for you. We zero in exclusively on all the questions people have about how being in a state of nutritional ketosis and the effects it has on your health. There are a lot of myths about keto floating around out there and our two amazing cohosts are shooting them down one at a time. Keto Talk is cohosted by 10-year veteran health podcaster and international bestselling author Jimmy Moore from "Livin' La Vida Low-Carb" and Arizona osteopath and certified bariatric physician Dr. Adam Nally from "Doc Muscles" who thoroughly share from their wealth of experience on the ketogenic lifestyle each and every Thursday. We love hearing from our fabulous Ketonian listeners with new questions--send an email to Jimmy at firstname.lastname@example.com. And if you're not already subscribed to the podcast on iTunes and listened to the past episodes, then you can do that and leave a review HERE. Listen in today as Jimmy and Adam have another educational and entertaining show for you in Episode 43.
**Special THANK YOU to Louann, Laura, Richard, Chris, Pedro, and Diane**
Here's what Jimmy and Adam talked about in Episode 43:
- Should I be concerned about the fat related digestion results of my stool analysis?
Hi guys,
I recently had a CDSA stool analysis to look for more information about my health. Under the absorption category, my fat related digestion is all quite high. I am wondering if this is common with keto since the test is norm referenced vs non-keto or is this something that needs to be addressed? Also of note is that the pH is quite high. Again, is this a keto thing? And what suggestions would you have?
Thank you,
- Glycemic Control for Patients With Type 2 Diabetes Mellitus: Our Evolving Faith in the Face of Evidence
1. Can a ketogenic diet be beneficial for morning sickness during pregnancy?
Hey Jimmy and The Doc,
Love your show and never miss it.
My wife is 6 weeks pregnant and she suffers a LOT with morning sickness. She just can't stand it. I've been keto for about 10 months now (and loving it), but she is not. In fact, she does not have any desire or hunger at all because of all the morning sickness. And I'm afraid eating the fat on a ketogenic diet would make it worse since she is not fat adapted.
My question is: what role could a ketogenic diet play in relieving these morning sickness episodes? Is it safe to start a ketogenic diet at this point in the pregnancy? Would the keto adaptation phase of 2-4 weeks make it even worse given the possibility of keto flu and electrolyte imbalance?
I really want this topic to be addressed. Thanks a lot and keep up the good work,
Fernando from Rio de Janeiro, Brazil
2. Is eating ketogenic detrimental to someone with a binge eating disorder?
I've been living keto most of the time for the last year and a half, and I've lost 130 pounds so far. I'm still overweight, but I spent most of my adult life well over 300 pounds for a 5'4" woman. Needless to say, this is a huge change. Aside from the weight loss, eating keto has also helped to lessen the depression I've been struggling with since puberty. The problem I'm having is that I periodically get sucked into days of binge eating non-keto foods, which leaves me dealing with not only re-acclimating to ketosis but also a significant biochemical mood dive. When I'm on track (which is most of the time) my macros are 80/15/5, and I weigh/measure/plan/track my food so that's quite accurate. My total carbs are around 20g/day. I very rarely test my ketones due to the cost of strips, but when I do my numbers are between 1.5 and 4. I test my fasting blood glucose regularly and it's usually in the 70s.
When I'm looking at books and online programs for dealing with binge eating or food addiction, they all seem to be against even standard low-carb diets, much less keto. Their reasoning is that the restrictions lead to binge eating. Have you found that people with binge eating or food addiction problems need to eat a more "balanced" whole foods diet in order to mentally recover? I really don't want to walk away from keto because it's been so amazing for me, but I'm also scared that I'll get sucked fully back into binge eating junk and end up back to where I started. Eating keto does decrease my cravings and appetite but for me they never quite go away. I've tried intermittent fasting and it's consistently tipped me over into binging.
Thank you for what you do! I really like listening to your podcast.
3. Are my carb cravings late in the day while eating keto physiological or habitual?
I'm insulin resistant and know that I do better and feel better on a keto diet. I've been low carb for 5 years. Everyday, I vow that it will be the day that I stick to a strict keto diet. I do great in the mornings eating bacon, greens, and eggs for breakfast, maybe some dinner leftovers for lunch such as a protein with cooked veggies or leftover salad. But the late afternoon and evening after dinner is when my best-laid plans fall apart. I grab a few handfuls of popcorn that my teenage daughter brought home and stashed in the pantry. Or I eat a bowl of sugar-free (but obviously not junk free or very low carb) ice cream I bought during my last trip to the store. Or I'll go in the cupboard and grab a small piece of dark chocolate, but I'll go back for one or two more pieces before I'm satisfied.
Are these cravings for something sweet and creamy, or salty and crunchy physiological or habitual? I know they keep me from being totally keto. One of the things I tell myself when I reach for that handful of popcorn or that bowl of sugar-free ice cream is, "I've been on track most of the day/week/month, I can treat myself to some of this." Sometimes I don't tell myself anything, I just have this deep craving, this obsessive thought, that something sweet and creamy will quench my craving. It's like cigarettes or something!
Do you guys have any clue what can I do about it?
- What impact do steam rooms and saunas have on ketone levels?
Hi Jimmy and Doc Nally,
Love the podcast. Very informative and loads of useful info. I have a question regarding the use of steam rooms and saunas. Will the use of these have any effect good or bad on ketone production? I typically use a steam room with temperature over 40 degrees Celsius once a week. Obviously it speeds up heart rate and is supposed to help the liver detox.
Thanks for any info you might have!
Jason from England
iTunes review:
- SUPPORT OUR SPONSOR: Try quality low-carb meats from ButcherBox (use coupon code LLVLC at checkout for $10 your first box)
- Make plans to attend the 2nd Annual Conference on Nutritional Ketosis and Metabolic Therapeutics coming to Tampa, Florida on February 1-4, 2017
- SUPPORT OUR SPONSOR: Go to RealGoodPizzaCo.com for delicious low-carb frozen pizza (Get free shipping and 10% off your order with coupon code "LLVLC")
- SUPPORT OUR SPONSOR: Try Cronometer to track your keto progress (get 50% off a 3-month gold subscription)
- Jimmy Moore from "Livin' La Vida Low-Carb"
- Dr. Adam Nally, DO from DocMuscles.com
- Glycemic Control for Patients With Type 2 Diabetes Mellitus: Our Evolving Faith in the Face of Evidence


text:
I've noticed that I have tried and tried in my social life. I tried to make friends with people who didn't value me. I tried to meet girls who just didn't like me. I tried and tried and tried. But, the relationships that I have that last were ones that I did not try for. Those relationships just came to me. Long ago a friend told me that I put too much effort in meeting new people. He said I should wait and see who comes to me. I sounded like a very deep suggestion. Unfortunately, not so many people are interested in me. And those that are are not usually my type. I decided to devote my life to work and spirituality as the frequency of people being interested in me is not great enough.
I just wonder if my friend was right. When I am working hard at meeting people I'm sending the universe a message that I want to meet people. Since I have stopped trying, the universe has not sent me too many people. Perhaps it is because I live in Los Angeles or because I'm in my 40's. I can't say.
In any case — don't die trying at relationships. Perhaps a balanced amount of effort is the right amount.


text:
Ames Police
June 19: Jonathan Dixon Williby, 34, of Ames, operating while intoxicated; Steven Chales Robinson, 62, of Boone, theft; Joshua Richard Scott, of Ames, theft and criminal trespass.
June 20: Timothy Alan Howdesell, 23, of Ames, operating while intoxicated; Steven James Catus, of Ames, public intoxication.
Story County Sheriff
June 19: Todd Adrian Stevens, 18, probation violation; Cynthia Starr Ross, 41, contempt of court; Jerad Michael Ruble, 20, contempt of court.
ISU Police
June 17: Stephen Morton, 21, of Ames, theft; Xin Cui, 22, of Ames, driving under suspension.
June 19: Brittney Oxley, 19, of Marion, public intoxication; Matthew Quicksell, 20, of Woodbury, Minn., public intoxication, disorderly conduct, criminal mischief and unlawful use of a license.
Boone County Sheriff
June 19: Steven Robinson of Boone, theft.
ISU Police
June 17: Qingyu Kong, 21, of Ames, animal cruelty.
ISU Police
June 19: An officer doused wood pallets that were on fire on Mortensen Road at 4:59 a.m.
June 20: 4:25 a.m. public assist in the 2200 block of Clark Avenue.
June 19: 6:12 p.m. vehicle fire in the 400 block of Freel Drive.
June 19: 11:47 a.m. fire alarm in the 200 block of Richardson Court.


text:
|Message view
|« Date » · « Thread »
|« Date » · « Thread »
|sebb <seb...@gmail.com>
|Re: svn commit: r1370208 - in /commons/proper/jexl/branches/2.0: RELEASE-NOTES.txt pom.xml src/site/xdoc/changes.xml
|Tue, 07 Aug 2012 14:48:47 GMT
On 7 August 2012 15:16, henrib <email@example.com> wrote: > Just trying to ensure that I will not generate a public jexl2 release > compiled against a jdk6. Did not prevent me using Java 1.6 to compile. Try updating a source file to add a call to "".isEmpty() - a Java 1.6+ method - and see what happens if you compile with the default Java set to 1.6 That compiles fine for me on WinXP Compiling with 1.6 will still generate 1.5-compatible code provided that the source/target properties are set correctly. Note that the Continuum build should pick up any usage of Java 1.6+ methods which is the only other issue here. > Since most (if not all) JEXL users can't even use published snapshots, the > likelihood of anyone attempting to compile jexl2 and not being able to > comment the toolchain plugin in the pom seems very low... It's a pain having to update the pom just to check with different JVMs. That's partly why CP now includes the java-1.x profiles. Also, the way that is implemented actually works! > Anyhow, you can revert the modification and you are more than welcome to > release jexl-2.1.2 if you want to. :- I don't mind it being present if it adds utility without causing problems. > > > -- > View this message in context: http://apache-commons.680414.n4.nabble.com/Re-svn-commit-r1370208-in-commons-proper-jexl-branches-2-0-RELEASE-NOTES-txt-pom-xml-src-site-xdoc-cl-tp4637751p4637754.html > Sent from the Commons - Dev mailing list archive at Nabble.com. --------------------------------------------------------------------- To unsubscribe, e-mail: firstname.lastname@example.com For additional commands, e-mail: email@example.com
|View raw message


text:
Strona domowa ▸ Sklepy ▸ Sklep #79 ▸ Oceny i komentarze
Oceny i komentarze • Hobby Frontier
- Good Alternative if JP ran out of stock!This shop is a good alternative here in SG if stocks in JP ran out. price is also competitive. favorable for buyers in SG due to JP + Shipping is equivalent to hobby-frontier's price. (so just imagine you paid for item + shipping)
- would love to shop with this shop again and againLike to shopping with, price are reasonable for Pre-Order items, Website design is top notch with search and "out of stock" filter with just one click. My first choice provided they have items I want before I look further for other source.
- Pretty decent prices (in SG) and responsible owner.I purchased items from this shop (once in june and another in aug). Plus preordered 3..
Pricing is generally decent compared to other shops in SG..
Owner gave me a discount once when the delivery was late for almost 30mins due to an earlier customer failing to show up for appointment which is a nice gesture! Also went out of his way to order replacement item from amiami without change in pricing for me when his supplier failed to supply one of my preordered toys after release day.. pretty cool tho i find him abit talkative lol..
Will def support again!
- Good Prices, quick response.Bought some of my Miku Nendoroids and Attack on Titan Levi from them. Price is pretty good compared to other stores in SG, also seems like they do not adjust pricing upward even if item is rare and selling at high prices on resale market/ebay. My email was replied quickly even though i sent them late at night. (night owl!? lol)
Only issue i see is they do not source out of stock items but the delivery guy explained that it is because they only buy from wholesaler/distribution and not from 2nd hand or other stores to sell back to me so i guess it can't be helped.
- Sometimes good for domestic buyersSome figures are priced relatively cheaper and delivery was prompt.
- 11 opinie