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Genres: Variety
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Derren Brown: Mind Control (also known as Mind Control with Derren Brown) is a British variety series produced by Objective Productions in which illusionist Derren Brown attempts to predict and influence people's thoughts.The series originally aired in the UK on Channel 4. There are six half-hour episodes in the series.Derren Brown: Mind Control premiered in South Africa on DStv's BBC Entertainment channel on Sunday 5 October 2008, at 21h00.RepeatsMondays: 01h00SynopsisDerren Brown is a mentalist — someone who can seemingly read another's mind. Brown seems able to impose his will upon others with little more than a pep talk or a reassuring gesture.His show certainly is a demonstration of his power of persuasion. It's also a smart send-up of self-help conferences and a debunking of street tricks, frauds and mystical myths.Brown built his reputation as an amazing mentalist with such mind-blowing setups as:A random woman answers a ringing pay phone. She listens wordlessly for a couple moments before slumping to the concrete in a deep sleep.Another stranger is convinced by Brown that the sun has disappeared. Brown protects his cash-stuffed wallet from being pilfered on a busy sidewalk by putting it down and chalking a ring around it.Pushing psychological buttons most don't even realize exist, Brown opens windows into how our minds really work. And in Mind Control with Derren Brown, he reveals just enough of his secrets to further intrigue audiences.Derren Brown ShowsMind ControlRussian RouletteSéanceMessiahTrick of the MindThe HeistSomething Wicked This Way ComesThe EventsAn Evening of WondersEnigmaThe Experiments
New on TV today: Sunday 12 July
Ivor en die Verskilmakers starts on VIA and Two and a Half Men returns to eExtra.
Council of Dads (Season 1)
So what happens when a family man fights a grave illness, faces death, and is worried about how his wife and five kids are gonna carry on without him? He has a ...
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Somizi & Mohale: The Union comes to Wethu, the final season of Supernatural starts on M-Net City and Khabodacious returns to SABC2.
2020 SAMAs: Music Video and Record of the Year nominees
The SAMA public voting categories have been announced and the choice of Best Video cannot be taken lightly.
The Bold and the Beautiful on Eva Teasers - August 2020
Is there hope to find out who is threatening Hope?
Wild Skin Teasers - August 2020
Camila prevents a shooting. Also, a hit-man is hired.
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Finale alert! Agustin and Gracia go from being in cahoots to warnings being given.
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Join 1Magic for Dinner at Somizi's or Nat Geo to uncover Lost Treasures of the Maya.
Rhythm Cityzens take on Scandal! on Family Feud South Africa
They're wrapped between Steve Harvey this Sunday, 12 July. See who's competing.
Catch-up with Iron Rose star Aracely Arámbula
From Season 1 to Season 2. Telemundo's Iron Rose gives us her take on Altagracia's inner world across seasons.
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Kilkee by the sea, it's the beauty that sets your mind free.Register
Kilkee is a spellbinding seaside resort dating back more than 200 years and situated along the spectacular Loop Head Peninsula in Co Clare.Register
Kilkee by the sea, it's the beauty that sets your mind free.Register
Based on the most recent Government guidance relating to COVID-19 it very clearly is not possible to safely proceed with Run Kilkee as planned. Therefore, we have made the decision to postpone Run Kilkee for this year to Saturday 10th July 2021. We fully appreciate the disappointment that this will bring but we have to put the health and wellbeing of all our runners, walkers, crew, medical providers and all our collective extended families first.
All registrations have automatically been transferred to Saturday 10th July 2021 and you do not need to do anything further at this stage if you have already registered for the 2020 event.
We thank your sincerely for your cooperation and understanding and of course please email us at firstname.lastname@example.com if we can be of any assistance or if you have any queries.
Run Kilkee will take place along the spectacular Loop Head Peninsula in Co Clare on Saturday 10th July 2021. The course consists of a 13.1 mile Half Marathon and a 10km run/walk set along the stunning sea cliff panoramic views of the Loop Head Peninsula. This is a 'must do' event in one of Irelands must beautiful locations on the Wild Atlantic Way with the course designed for runners and walkers to enjoy its breathtaking scenery and beautiful rugged coastline. The routes will immerse runners and walkers in the natural beauty of the Loop Head Peninsula on the Wild Atlantic Way.
Register now to guarantee your place. Prices exclude an online booking fee of 7%.
Kilkee is a spellbinding seaside resort dating back more than 200 years and situated along the spectacular Loop Head Peninsula in Co Clare. Kilkee, Loop Head's main town, is built around a horseshoe bay with a kilometre of golden, blue-flag beach along Ireland's Wild Atlantic Way with breathtaking scenic walks and stunning sea cliff views.
It is a small coastal town located on the rugged West coast of County Clare, Ireland. The town is a particularly popular Irish seaside resort with family's travelling from all over the country to holiday here. Kilkee and the Loop Head Peninsula also attracts thousands of foreign tourists to the area annually with its breathtaking scenic walks and stunning sea cliff panoramic views as well as all the other wonderful amenities that are available in the area.
Hosting an event of this standard is a privilege & we are hugely indebted to a host of individuals & organisations who collectively strive to create the most enjoyable experience for all participants & visitors to Kilkee.

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John 20:19-20
When it was evening on that day, the first day of the week, and the doors of the house where the disciples had met were locked for fear of the Jews, Jesus came and stood among them and said, "Peace be with you." After he said this, he showed them his hands and his side. Then the disciples rejoiced when they saw the Lord.
The Church can now be opened for private prayer. Please contact the Vicar to make an appropriate time for visiting. Remember to keep social distancing, wash your hands and use the santiser provided in the Church. May God Bless you and keep you safe.
In keeping with Church of England Guidelines, please be advised that all public worship and Church services are suspended until further notice.
Keep us, good Lord,
under the shadow of your mercy.
Sustain and support the anxious,
be with those who care for the sick,
and lift up all who are brought low;
that we may find comfort
knowing that nothing can separate us from your love
in Christ Jesus our Lord.
Please click on this link for Daily Prayer Resources from the Church of England.
Remember to have a look on Facebook for services from Church of England.
We welcome you to our website and look forward to hearing from you
Parish Office Contact Details
The Office is situated at the rear of the Church Hall
Please contact the Vicar with equiries about Baptisms, Funerals and Marriages
By Prior Appointment, please contact via Email or Telephone Voicemail.
St. Andrew's Church Parish Office
118 Abbotts Walk
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Health conditions. Meaning of dream and numbers.
Find out what it means to dream health conditions. The interpretations and numbers of the Neapolitan cabala.
establish conditions 35
Meaning of the dream: contempt of danger
demanding conditions 76
Description: relations to care
deteriorating health 57
Interpretation of the dream: inheritance
dictate conditions 85
Translation: unwillingness
health 13
Dream description: bad omen for the sick
restoring health 18
Meaning: physical discomfort
accept conditions 62
Translation of the dream: pretense and insincerity
decayed health 20
Interpretation: serenity conquered
ruining health 3
Sense of the dream: New Jobs
recover in health 81
What does it mean: malaise of short duration
home health 24
Meaning of the dream: secret ambitions
private health 26
Description: misgivings
Marshal health 19
Interpretation of the dream: speculation success
worry about someone's health 35
Translation: tension in the family
attention to their own health 4
Dream description: excellent recovery
health attestation 23
Meaning: you're too busy
health care bill 21
Translation of the dream: moments of despair
health care reform 25
Interpretation: Failure of a deal
terms 41
Sense of the dream: thou shalt well-being from your wisdom
women's health 35
What does it mean: coming dangers
changing condition 8
Meaning of the dream: gain that fades
acclamation 48
Description: adulation with sad consequences, subtleties
poor housing 1
Interpretation of the dream: keen observation
fight for the healthy 3
Translation: infirmity
angel for the healthy 67
Dream description: consolation, good news
confusion of vehicles 38
Meaning: inconstancy in love
confusion of objects 89
Translation of the dream: deal that goes through
confusion 12
Interpretation: great ideas
assisting convalescents 42
Sense of the dream: changing situations
predict a fortune 20
What does it mean: love of short duration
situation of distress 44
Meaning of the dream: encouraging results
confusion of people 8
Description: shyness and diffidence
aggravation of situation 19
Interpretation of the dream: dishonor
greater than condition 1
Translation: volatility harmful
convalescent visit a child 27
Dream description: important trip
convalescent visit a man 75
Meaning: prodigality exaggerated
convalescent visit a friend 67
Translation of the dream: Acute sensitivity
convalescent visit a woman 51
Interpretation: obstacles and hostilities
immutability 81
Sense of the dream: broken promises
fortune 7
What does it mean: enthusiasms and projects
state employment 18
Meaning of the dream: You are able to give some continuity to your business
salute the flag 54
Description: decisions well directed
state house 22
Interpretation of the dream: your friend will deceive
hygienist 39
Translation: unpleasant discussions
commanding fortune 30
Dream description: waiting
form a state 46
Meaning: realizations unrealized aspirations
healthy 47
Translation of the dream: concerns
inherit a fortune 42
Interpretation: sorrows and anxieties
adverse fortune 49
Sense of the dream: accumulated work to be done
squandering a fortune 30
What does it mean: defeats and disappointments
bandage fortune 90
Meaning of the dream: changes favorites
be on good terms 77
Description: lasting commitment
be on bad terms 7
Interpretation of the dream: slow progress
budget status 52
Translation: material difficulties


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2019 Top Brand DOM Luxury Men's Watch 30m Waterproof Date Clock Male Sports Watches Men Quartz Wrist Watch Relogio Masculino
Brand Name: DOM
Band Length: 19cm
Style: Sport
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The Murchison Widefield Array (MWA) is an open access telescope dedicated to studying the low-frequency (80–300 MHz) southern sky. Since beginning operations in mid-2013, the MWA has opened a new observational window in the southern hemisphere enabling many science areas. The driving science objectives of the original design were to observe 21 cm radiation from the Epoch of Reionisation (EoR), explore the radio time domain, perform Galactic and extragalactic surveys, and monitor solar, heliospheric, and ionospheric phenomena. All together
programs recorded 20 000 h producing 146 papers to date. In 2016, the telescope underwent a major upgrade resulting in alternating compact and extended configurations. Other upgrades, including digital back-ends and a rapid-response triggering system, have been developed since the original array was commissioned. In this paper, we review the major results from the prior operation of the MWA and then discuss the new science paths enabled by the improved capabilities. We group these science opportunities by the four original science themes but also include ideas for directions outside these categories.
We have detected 27 new supernova remnants (SNRs) using a new data release of the GLEAM survey from the Murchison Widefield Array telescope, including the lowest surface brightness SNR ever detected, G 0.1 – 9.7. Our method uses spectral fitting to the radio continuum to derive spectral indices for 26/27 candidates, and our low-frequency observations probe a steeper spectrum population than previously discovered. None of the candidates have coincident WISE mid-IR emission, further showing that the emission is non-thermal. Using pulsar associations we derive physical properties for six candidate SNRs, finding G 0.1 – 9.7 may be younger than 10 kyr. Sixty per cent of the candidates subtend areas larger than 0.2 deg2 on the sky, compared to < 25% of previously detected SNRs. We also make the first detection of two SNRs in the Galactic longitude range 220°–240°.
This work makes available a further
of the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey, covering half of the accessible galactic plane, across 20 frequency bands sampling 72–231 MHz, with resolution
. Unlike previous GLEAM data releases, we used multi-scale CLEAN to better deconvolve large-scale galactic structure. For the galactic longitude ranges
$345^\circ < l < 67^\circ$
$180^\circ < l < 240^\circ$
, we provide a compact source catalogue of 22 037 components selected from a 60-MHz bandwidth image centred at 200 MHz, with RMS noise
and position accuracy better than 2 arcsec. The catalogue has a completeness of 50% at
, and a reliability of 99.86%. It covers galactic latitudes
towards the galactic centre and
for other regions, and is available from Vizier; images covering
for all longitudes are made available on the GLEAM Virtual Observatory (VO).server and SkyView.
We examined the latest data release from the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey covering 345° < l < 60° and 180° < l < 240°, using these data and that of the Widefield Infrared Survey Explorer to follow up proposed candidate Supernova Remnant (SNR) from other sources. Of the 101 candidates proposed in the region, we are able to definitively confirm ten as SNRs, tentatively confirm two as SNRs, and reclassify five as H ii regions. A further two are detectable in our images but difficult to classify; the remaining 82 are undetectable in these data. We also investigated the 18 unclassified Multi-Array Galactic Plane Imaging Survey (MAGPIS) candidate SNRs, newly confirming three as SNRs, reclassifying two as H ii regions, and exploring the unusual spectra and morphology of two others.
The Murchison Widefield Array (MWA) is an electronically steered low-frequency (<300 MHz) radio interferometer, with a 'slew' time less than 8 s. Low-frequency (∼100 MHz) radio telescopes are ideally suited for rapid response follow-up of transients due to their large field of view, the inverted spectrum of coherent emission, and the fact that the dispersion delay between a 1 GHz and 100 MHz pulse is on the order of 1–10 min for dispersion measures of 100–2000 pc/cm3. The MWA has previously been used to provide fast follow-up for transient events including gamma-ray bursts (GRBs), fast radio bursts (FRBs), and gravitational waves, using systems that respond to gamma-ray coordinates network packet-based notifications. We describe a system for automatically triggering MWA observations of such events, based on Virtual Observatory Event standard triggers, which is more flexible, capable, and accurate than previous systems. The system can respond to external multi-messenger triggers, which makes it well-suited to searching for prompt coherent radio emission from GRBs, the study of FRBs and gravitational waves, single pulse studies of pulsars, and rapid follow-up of high-energy superflares from flare stars. The new triggering system has the capability to trigger observations in both the regular correlator mode (limited to ≥0.5 s integrations) and using the Voltage Capture System (VCS, 0.1 ms integration) of the MWA and represents a new mode of operation for the MWA. The upgraded standard correlator triggering capability has been in use since MWA observing semester 2018B (July–Dec 2018), and the VCS and buffered mode triggers will become available for observing in a future semester.
Neuropsychological tests are important instruments to determine a cognitive profile, giving insight into the etiology of dementia; however, these tests cannot readily be used in culturally diverse, low-educated populations, due to their dependence upon (Western) culture, education, and literacy. In this review we aim to give an overview of studies investigating domain-specific cognitive tests used to assess dementia in non-Western, low-educated populations. The second aim was to examine the quality of these studies and of the adaptations for culturally, linguistically, and educationally diverse populations.
A systematic review was performed using six databases, without restrictions on the year or language of publication.
Forty-four studies were included, stemming mainly from Brazil, Hong Kong, Korea, and considering Hispanics/Latinos residing in the USA. Most studies focused on Alzheimer's disease (n = 17) or unspecified dementia (n = 16). Memory (n = 18) was studied most often, using 14 different tests. The traditional Western tests in the domains of attention (n = 8) and construction (n = 15), were unsuitable for low-educated patients. There was little variety in instruments measuring executive functioning (two tests, n = 13), and language (n = 12, of which 10 were naming tests). Many studies did not report a thorough adaptation procedure (n = 39) or blinding procedures (n = 29).
Various formats of memory tests seem suitable for low-educated, non-Western populations. Promising tasks in other cognitive domains are the Stick Design Test, Five Digit Test, and verbal fluency test. Further research is needed regarding cross-cultural instruments measuring executive functioning and language in low-educated people.
We apply two methods to estimate the 21-cm bispectrum from data taken within the Epoch of Reionisation (EoR) project of the Murchison Widefield Array (MWA). Using data acquired with the Phase II compact array allows a direct bispectrum estimate to be undertaken on the multiple redundantly spaced triangles of antenna tiles, as well as an estimate based on data gridded to the uv-plane. The direct and gridded bispectrum estimators are applied to 21 h of high-band (167–197 MHz; z = 6.2–7.5) data from the 2016 and 2017 observing seasons. Analytic predictions for the bispectrum bias and variance for point-source foregrounds are derived. We compare the output of these approaches, the foreground contribution to the signal, and future prospects for measuring the bispectra with redundant and non-redundant arrays. We find that some triangle configurations yield bispectrum estimates that are consistent with the expected noise level after 10 h, while equilateral configurations are strongly foreground-dominated. Careful choice of triangle configurations may be made to reduce foreground bias that hinders power spectrum estimators, and the 21-cm bispectrum may be accessible in less time than the 21-cm power spectrum for some wave modes, with detections in hundreds of hours.
The Commensal Real-time Australian Square Kilometre Array Pathfinder Fast Transients survey is the first extensive astronomical survey using phased array feeds. Since January 2017, it has been searching for fast radio bursts in fly's eye mode. Here, we present a calculation of the sensitivity and total exposure of the survey that detected the first 20 of these bursts, using the pulsars B1641-45 and B0833-45 as calibrators. The beamshape, antenna-dependent system noise, and the effects of radio-frequency interference and fluctuations during commissioning are quantified. Effective survey exposures and sensitivities are calculated as a function of the source counts distribution. Statistical 'stat' and systematics 'sys' effects are treated separately. The implied fast radio burst rate is significantly lower than the 37 sky−1 day−1 calculated using nominal exposures and sensitivities for this same sample by Shannon et al. (2018). At the Euclidean (best-fit) power-law index of −1.5 (−2.2), the rate is
(sys) ± 3.6 (stat) sky−1 day−1 (
(sys) ± 2.8 (stat) sky−1 day−1) above a threshold of 56.6 ± 6.6(sys) Jy ms (40.4 ± 1.2(sys) Jy ms). This strongly suggests that these calculations be performed for other FRB-hunting experiments, allowing meaningful comparisons to be made between them.
The GaLactic and Extragalactic All-sky Murchison Widefield Array survey is a radio continuum survey at 72–231 MHz of the whole sky south of declination +30º, carried out with the Murchison Widefield Array. In this paper, we derive source counts from the GaLactic and Extragalactic All-sky Murchison data at 200, 154, 118, and 88 MHz, to a flux density limit of 50, 80, 120, and 290 mJy respectively, correcting for ionospheric smearing, incompleteness and source blending. These counts are more accurate than other counts in the literature at similar frequencies as a result of the large area of sky covered and this survey's sensitivity to extended emission missed by other surveys. At S154 MHz > 0.5 Jy, there is no evidence of flattening in the average spectral index (α ≈ −0.8 where S ∝ vα) towards the lower frequencies. We demonstrate that the Square Kilometre Array Design Study model by Wilman et al. significantly underpredicts the observed 154-MHz GaLactic and Extragalactic All-sky Murchison counts, particularly at the bright end. Using deeper Low-Frequency Array counts and the Square Kilometre Array Design Study model, we find that sidelobe confusion dominates the thermal noise and classical confusion at v ≳ 100 MHz due to both the limited CLEANing depth and the undeconvolved sources outside the field-of-view. We show that we can approach the theoretical noise limit using a more efficient and automated CLEAN algorithm.
We provide the first in situ measurements of antenna element beam shapes of the Murchison Widefield Array. Most current processing pipelines use an assumed beam shape, which can cause absolute and relative flux density errors and polarisation 'leakage'. Understanding the primary beam is then of paramount importance, especially for sensitive experiments such as a measurement of the 21-cm line from the epoch of reionisation, where the calibration requirements are so extreme that tile to tile beam variations may affect our ability to make a detection. Measuring the primary beam shape from visibilities is challenging, as multiple instrumental, atmospheric, and astrophysical factors contribute to uncertainties in the data. Building on the methods of Neben et al. [Radio Sci., 50, 614], we tap directly into the receiving elements of the telescope before any digitisation or correlation of the signal. Using ORBCOMM satellite passes we are able to produce all-sky maps for four separate tiles in the XX polarisation. We find good agreement with the beam model of Sokolowski et al. [2017, PASA, 34, e062], and clearly observe the effects of a missing dipole from a tile in one of our beam maps. We end by motivating and outlining additional on-site experiments.
We describe the motivation and design details of the 'Phase II' upgrade of the Murchison Widefield Array radio telescope. The expansion doubles to 256 the number of antenna tiles deployed in the array. The new antenna tiles enhance the capabilities of the Murchison Widefield Array in several key science areas. Seventy-two of the new tiles are deployed in a regular configuration near the existing array core. These new tiles enhance the surface brightness sensitivity of the array and will improve the ability of the Murchison Widefield Array to estimate the slope of the Epoch of Reionisation power spectrum by a factor of ∼3.5. The remaining 56 tiles are deployed on long baselines, doubling the maximum baseline of the array and improving the array u, v coverage. The improved imaging capabilities will provide an order of magnitude improvement in the noise floor of Murchison Widefield Array continuum images. The upgrade retains all of the features that have underpinned the Murchison Widefield Array's success (large field of view, snapshot image quality, and pointing agility) and boosts the scientific potential with enhanced imaging capabilities and by enabling new calibration strategies.
The discovery of the first electromagnetic counterpart to a gravitational wave signal has generated follow-up observations by over 50 facilities world-wide, ushering in the new era of multi-messenger astronomy. In this paper, we present follow-up observations of the gravitational wave event GW170817 and its electromagnetic counterpart SSS17a/DLT17ck (IAU label AT2017gfo) by 14 Australian telescopes and partner observatories as part of Australian-based and Australian-led research programs. We report early- to late-time multi-wavelength observations, including optical imaging and spectroscopy, mid-infrared imaging, radio imaging, and searches for fast radio bursts. Our optical spectra reveal that the transient source emission cooled from approximately 6 400 K to 2 100 K over a 7-d period and produced no significant optical emission lines. The spectral profiles, cooling rate, and photometric light curves are consistent with the expected outburst and subsequent processes of a binary neutron star merger. Star formation in the host galaxy probably ceased at least a Gyr ago, although there is evidence for a galaxy merger. Binary pulsars with short (100 Myr) decay times are therefore unlikely progenitors, but pulsars like PSR B1534+12 with its 2.7 Gyr coalescence time could produce such a merger. The displacement (~2.2 kpc) of the binary star system from the centre of the main galaxy is not unusual for stars in the host galaxy or stars originating in the merging galaxy, and therefore any constraints on the kick velocity imparted to the progenitor are poor.
We describe the design and performance of the Engineering Development Array, which is a low-frequency radio telescope comprising 256 dual-polarisation dipole antennas working as a phased array. The Engineering Development Array was conceived of, developed, and deployed in just 18 months via re-use of Square Kilometre Array precursor technology and expertise, specifically from the Murchison Widefield Array radio telescope. Using drift scans and a model for the sky brightness temperature at low frequencies, we have derived the Engineering Development Array's receiver temperature as a function of frequency. The Engineering Development Array is shown to be sky-noise limited over most of the frequency range measured between 60 and 240 MHz. By using the Engineering Development Array in interferometric mode with the Murchison Widefield Array, we used calibrated visibilities to measure the absolute sensitivity of the array. The measured array sensitivity matches very well with a model based on the array layout and measured receiver temperature. The results demonstrate the practicality and feasibility of using Murchison Widefield Array-style precursor technology for Square Kilometre Array-scale stations. The modular architecture of the Engineering Development Array allows upgrades to the array to be rolled out in a staged approach. Future improvements to the Engineering Development Array include replacing the second stage beamformer with a fully digital system, and to transition to using RF-over-fibre for the signal output from first stage beamformers.
The S-band Polarisation All-Sky Survey has observed the entire southern sky using the 64-m Parkes radio telescope at 2.3 GHz with an effective bandwidth of 184 MHz. The surveyed sky area covers all declinations δ ⩽ 0°. To analyse compact sources, the survey data have been re-processed to produce a set of 107 Stokes I maps with 10.75 arcmin resolution and the large scale emission contribution filtered out. In this paper, we use these Stokes I images to create a total intensity southern-sky extragalactic source catalogue at 2.3 GHz. The source catalogue contains 23 389 sources and covers a sky area of 16 600 deg2, excluding the Galactic plane for latitudes |b| < 10°. Approximately, 8% of catalogued sources are resolved. S-band Polarisation All-Sky Survey source positions are typically accurate to within 35 arcsec. At a flux density of 225 mJy, the S-band Polarisation All-Sky Survey source catalogue is more than 95% complete, and ~ 94% of S-band Polarisation All-Sky Survey sources brighter than 500 mJy beam−1 have a counterpart at lower frequencies.
The Evolutionary Map of the Universe (EMU) is a proposed radio continuum survey
of the Southern Hemisphere up to declination + 30°, with the Australian
Square Kilometre Array Pathfinder (ASKAP). EMU will use an automated source
identification and measurement approach that is demonstrably optimal, to
maximise the reliability and robustness of the resulting radio source
catalogues. As a step toward this goal we conducted a "Data
Challenge" to test a variety of source finders on simulated images. The
aim is to quantify the accuracy and limitations of existing automated source
finding and measurement approaches. The Challenge initiators also tested the
current ASKAPsoft source-finding tool to establish how it could benefit from
incorporating successful features of the other tools. As expected, most finders
show completeness around 100% at ≈ 10σ dropping to about 10% by
≈ 5σ. Reliability is typically close to 100% at ≈
10σ, with performance to lower sensitivities varying between finders. All
finders show the expected trade-off, where a high completeness at low
signal-to-noise gives a corresponding reduction in reliability, and vice versa.
We conclude with a series of recommendations for improving the performance of
the ASKAPsoft source-finding tool.
GLEAM, the GaLactic and Extragalactic All-sky MWA survey, is a survey of the entire radio sky south of declination + 25° at frequencies between 72 and 231 MHz, made with the MWA using a drift scan method that makes efficient use of the MWA's very large field-of-view. We present the observation details, imaging strategies, and theoretical sensitivity for GLEAM. The survey ran for two years, the first year using 40-kHz frequency resolution and 0.5-s time resolution; the second year using 10-kHz frequency resolution and 2 s time resolution. The resulting image resolution and sensitivity depends on observing frequency, sky pointing, and image weighting scheme. At 154 MHz, the image resolution is approximately 2.5 × 2.2/cos (δ + 26.7°) arcmin with sensitivity to structures up to ~ 10° in angular size. We provide tables to calculate the expected thermal noise for GLEAM mosaics depending on pointing and frequency and discuss limitations to achieving theoretical noise in Stokes I images. We discuss challenges, and their solutions, that arise for GLEAM including ionospheric effects on source positions and linearly polarised emission, and the instrumental polarisation effects inherent to the MWA's primary beam.
Aluminum oxide films have been deposited by electron-beam evaporation on heated substrates under oxygen ion bombardment. Substrates were crystalline silicon, grafoil and glass. Both substrat temperature and ion current density were changed for each deposition The films deposited on silicon were examined by spectroscopie ellipsometry which showed that for substrate temperatures between 70°C and 250°C the index of refraction, and therefore the film density, first rose and then decreased with increasing ion current density. Ai 400°C the index reached a plateau under these conditions. Study by Rutherford backscattering of films deposited on grafoil showed no significant correlation between oxygen-aluminum stoichiometry and fi; density, suggesting that the decrease in density for large ion currei is not due to oxygen-ion incorporation, as has been suggested in the past. The films deposited on glass at 400°C showed some evidence of crystallization.
We suggest a new application for elastic scattering of a metastable spin-polarized atomic helium beam at thermal energy. We demonstrate how angle-resolved measurements of the Bragg peaks of scattered surviving metastable atoms can give information about the spin-ordering of an antiferromagnetic (AF) transition metal oxide surface. In this paper, we discuss the feasibility of such measurements for NiO(100) and MnO(100), based on available information about their electronic structure and the properties of spin-polarized metastable helium. On impact with a surface, the survival probability of metastables is generally very low (<10-2). There are two possible decay mechanisms for metastables, a resonance ionization followed by auger neutralization, or an auger de-excitation process. For AF surfaces which fulfill certain requirements on their electronic structure, spin-selection rules will inhibit the decay of the metastable atoms from a favourably aligned magnetic sublattice. The survival probability will then be dramatically enhanced from the chosen sublattice, and the coherently scattered surviving metastables will reflect the periodicity of that magnetic sublattice. In contrast to other methods currently applied to magnetic systems, this method does not rely on difference spectra. Consequently, reversal of spinorientation is not necessary for the observation of magnetic ordering.
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The Batman was filming in the UK and the production remains on pause. Meanwhile, Tenet adorns the cover of the new Total Film magazine (order here), which includes extended interviews with Nolan, Pattinson, John David Washington, Elizabeth Debicki, and Kenneth Branagh. Total Film readers who have already subscribed will get an exclusive cover featuring John David Washington's protagonist, and the newsstand cover features Washington and Robert Pattinson. Check them out below. … [Read more...] about Robert Pattinson on The Batman delay: "Having some time off is not the worst thing in the world"
Chad stahelski keanu reeves matrix
Respawn on storytelling, lore, and Season 11 of Apex Legends
The quests are pretty simple overall. It's mostly a case of running to a location, doing a bit of PvE while you pick up an artifact, then running to a landing zone to escape. The more interesting part is the story you get as you're playing, as well as the character conversations you unlock after completing one. I've always found that when big multiplayer games tell stories, you tend to feel like a bystander – you're just on the sidelines watching everything unfold. But, for as basic as the new missions are, I think they do a pretty good job of making you feel more involved and, as a result, more invested, which McCord says is pretty much what they were going for. … [Read more...] about Respawn on storytelling, lore, and Season 11 of Apex Legends
Goofy strategy sim Spacebase Startopia announced for late next year
Spacebase Startopia, a colorful and goofy-looking space station strategy simulation, is the descendant of a much older and less colorful game from 2001, Startopia. The cinematic trailer that introduces us to the new Spacebase Startopia doesn't give up much on gameplay (though it does squeeze in a Keanu at E3 joke) but based on the brief details from the game's Steam page, it will share some things in common with the original. … [Read more...] about Goofy strategy sim Spacebase Startopia announced for late next year
Watch the wholesome moment this Super Mario 64 speedrunner broke the world record after eight years of trying
Ryan "Simply" Reeves is a well-known Super Mario 64 speedrunner from Minnesota, USA who yesterday completed Nintendo's N64 classic with all 120 stars obtained in an incredible time of 1:38:28. Simply's time beat the previous world record of 1:38:43, which was obtained by a player called Liam Kings on 31st March 2020, by 15 seconds. … [Read more...] about Watch the wholesome moment this Super Mario 64 speedrunner broke the world record after eight years of trying


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Gjestene er enige: Disse oppholdene er høyt rangert for beliggenhet, renhold med mer.
A paradise for people who like peace and quiet, birdsong, marvellous countryside, clean air and lakewater, bonfires and barbecues, not to mention swimming and boating.
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A freshly renovated attic suite for up to 6 with a heavenly double bed and a sofa bed, lounge with TV, 2nd bedroom with single beds. Private wc and shower, kitchenette with a mini oven/stove, kettle and fridge, WiFi, private entrance and terrace. Endla lake and Nature Reserve on doorstep, offering 10 km of hiking trails, boardwalks, wachtowers, unique landscapes, wildlife, fresh air, peace and quiet. Order laundry service or breakfast for extra or rent a relaxing sauna 200 m away at our BnB.
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I was finally able to check this off my bucket list and had some friends along for the ride. After traveling by overnight sleeper train from Bangkok to Chiang Mai, we absolutely loved the the park and freedom we had to interact with the elephants. I learned a lot from the sanctuary about what happens to elephants that are exploited in Thailand and I felt strongly to spread these messages as far as I can. I hope you enjoy watching the incredible experience I had and also learn the sad truth of what is happening to so many elephants who are not as lucky.


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Ultra Joint 360 Review
Ultra Joint 360 Review Advice When coping with joint pain, it is almost always a fantastic idea to make certain that your weight is spread evenly if standing. Don't place on one leg than another. Obviously, you can't prevent this while walking but while standing, keep decent posture and even weight reduction to aid with… Read More »


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Lattice study of the Schwinger model at fixed topology
At small lattice spacing QCD simulations are expected to become stuck in a single topological sector. Observables evaluated in a fixed topological sector differ from their counterparts in full QCD, i.e. at unfixed topology, by volume dependent corrections. We investigate these corrections in the two-flavor Schwinger model, which is in several aspects similar to QCD, using Wilson fermions. We also try to remove these corrections by suitable extrapolations to infinite volume.
1 Introduction
Lattice QCD simulations are expected to suffer from frozen topology at small values of the lattice spacing independent of the quark discretization. The reason is that gauge link configurations belong to different topological sectors, which are separated by barriers of rather large Euclidean action. Choosing a smaller value for the lattice spacing increases these barriers, until standard HMC simulation algorithms are not anymore able to frequently traverse these barriers. Then the simulation gets stuck in a certain topological sector for a rather long time and computed observables contain corresponding systematic errors (cf. e.g. [1] and references therein). When using overlap fermions, topology freezing is even observed at rather coarse lattice spacings [2].
A possible solution to these problems is to restrict computations to a single topological sector, either by sorting the generated gauge link configurations with respect to their topological charge or by directly employing so-called topology fixing actions (cf. e.g. [3, 4, 5]). In a second step systematic effects due to topology fixing need to be removed by suitable extrapolations. Corresponding expressions have been derived [6, 7] and tested in simple models, i.e. in the Schwinger model [8] and in quantum mechanics [9].
In this work we explore computations at fixed topology in the Schwinger model. In contrast to [8], we use a computationally much cheaper lattice discretization of fermions (Wilson fermions instead of overlap fermions), which allows, to generate lattice results for many different topological sectors and spacetime volumes. In addition to the pseudoscalar meson mass (the "pion mass") we also study the static potential.
2 The Schwinger model with flavors of fermions
2.1 The Schwinger model in the continuum
The Schwinger model describes 2-dimensional Euclidean quantum electrodynamics:
It is a well known toy model for QCD, since it shares several interesting features with QCD. For example the gauge theory in two spacetime dimensions allows for topologically non-trivial field configurations, which are similar to instantons in -dimensional Yang-Mills theory. The corresponding topological charge is given by
Moreover, for its low lying energy eigenstates contain a rather light iso-triplet, which are quasi Nambu-Goldstone bosons and, therefore, can be seen as the pions of this model. Finally, the model provides fermion confinement.
2.2 The Schwinger model on the lattice
We study the Schwinger model (1) on a periodic spacetime lattice with lattice sites corresponding to a spacetime extension of ( is the lattice spacing) and a spacetime volume . We use flavors of Wilson fermions and the Wilson plaquette gauge action. As usual all dimensionful quantities are expressed in units of and denoted by , e.g. and .
One can approach the continuum limit by increasing , while keeping the dimensionless ratios and fixed ( denotes the mass of the aforementioned quasi Nambu-Goldstone bosons, i.e. the pion mass). This requires to decrease both and proportional to (for the latter has to be adjusted appropriately). It is also common to use the dimensionless inverse squared coupling constant .
We use the geometric definition of topological charge on the lattice,
[12, 13], where denotes the sum over all plaquettes with . With this definition for any given gauge link configuration.
We performed simulations at various values of , and using a Hybrid Monte Carlo (HMC) algorithm with multiple timescale integration and mass preconditioning [14]. In Figure 1 the probability for a transition to another topological sector per HMC trajectory is plotted versus and , while is kept constant. is proportional to the lattice spacing . is proportional to and, therefore, proportional to , the bare quark mass in physical units. As expected there are frequent changes of the topological sector at large values of the lattice spacing (large values of ), while at small values of (small values of ) topology freezing is observed. The dependence of the probability for a transition on the bare quark mass is rather weak.
3 Physical hadron masses from computations at fixed topology
3.1 Basic principle
The temporal correlation function of a hadron creation operator at fixed topological charge and finite spacetime volume is
For sufficiently large one can use a saddle point approximation and expand the correlation function according to
[6, 7], where the expansion is in the three parameters , and . is the mass of the hadron excited by at fixed topological charge and finite spacetime volume , is the hadron mass in a -vacuum at infinite (cf. e.g. [15]), is the physical hadron mass (i.e. the hadron mass at unfixed topology), and denotes the topological susceptibility.
To determine physical hadron masses (i.e. hadron masses at unfixed topology) from fixed topology computations we use a method, which has been proposed in [6] and tested in [8, 9]:
Determine the physical hadron mass (the hadron mass at unfixed topology and infinite spacetime volume), and by fitting (6) to the masses obtained in step 1.
3.2 Numerical results
The hadron masses we investigate in the following are the pion mass and the static potential (the ground state energy of a static quark antiquark pair at separation ). Suitable hadron creation operators are
( denotes a sum over space and and label the two degenerate fermion flavors) and
( and represent scalar static color charges and is the product of spatial links connecting and ).
We obtain hadron masses and at fixed topology by first determining the topological charge on each gauge link configuration according to (3). Then we perform independent computations of the pion mass and the static potential using only gauge link configuration with the same absolute value of .
In Figure 2 lattice results for for , and are plotted against . These results have been used as input for a single minimizing fit with (6). As discussed above (6) is an expansion in , and . Therefore, only fixed topology pion masses with sufficiently small values of and should be included in the fit. In Figure 2 we require (as indicated by the black boxes)111The topological susceptibility can be obtained numerically according to .. The fit is of acceptable quality and yields consistent results, , , which indicates that is a reasonable constraint. Since is determined by the fit, one can only check a posteriori, whether also is small, which is the case ().
For there are sufficiently many transitions between different topological sectors, to safely determine in the conventional way, i.e. by computing the corresponding temporal correlation function on all available gauge link configurations (i.e. as an average over all topological sectors) at a single sufficiently large . The result, (at ), agrees with the above results obtained by fixing topology within statistical errors.
We performed similar determinations of at fixed topology also at other values of and , e.g. at (which corresponds to a lattice spacing smaller by the factor compared to ) and (a pion masses larger by the factor compared to and ). As before we obtain accurate results, which are in agreement with conventional computations at unfixed topology.
In exactly the same way we successfully determined the static potential at fixed topology. An exemplary plot (analogous to Figure 2) corresponding to , and is shown in Figure 3.
Further numerical results are collected in Table 1. Note that hadron masses (i.e. the pion mass and the static potential) can be determined rather precisely (uncertainty ), while there is a rather large error associated with the topological susceptibility (uncertainty up to ). This is in agreement with similar existing investigations in the Schwinger model [8] and in quantum mechanics [9].
|(fixed top.)
|(fixed top.)
4 Conclusions
We successfully determined the pion mass and the static potential in the Schwinger model from computations at fixed topology using a method proposed and equations derived in [6]. The generalization of the method to QCD seems to be straightforward. There it might be used to circumvent problems associated with topology freezing expected at small values of the lattice spacing or when using e.g. overlap fermions.
Acknowledgments.We thank Carsten Urbach for providing program code for simulating the Schwinger model. We thank Wolfgang Bietenholz, Arthur Dromard, Gregorio Herdoiza, Karl Jansen and Carsten Urbach for discussions. M.W. acknowledges support by the Emmy Noether Programme of the DFG (German Research Foundation), grant WA 3000/1-1. This work was supported in part by the Helmholtz International Center for FAIR within the framework of the LOEWE program launched by the State of Hesse.
- [1] M. Lüscher and S. Schaefer, JHEP 1107, 036 (2011) [arXiv:1105.4749 [hep-lat]].
- [2] S. Aoki et al. [JLQCD Collaboration], Phys. Rev. D 78, 014508 (2008) [arXiv:0803.3197 [hep-lat]].
- [3] H. Fukaya et al., Phys. Rev. D 73, 014503 (2006) [hep-lat/0510116].
- [4] W. Bietenholz et al., JHEP 0603, 017 (2006) [hep-lat/0511016].
- [5] F. Bruckmann et al., Eur. Phys. J. A 43, 303 (2010) [arXiv:0905.2849 [hep-lat]].
- [6] R. Brower et al., Phys. Lett. B 560, 64 (2003) [hep-lat/0302005].
- [7] S. Aoki et al., Phys. Rev. D 76, 054508 (2007) [arXiv:0707.0396 [hep-lat]].
- [8] W. Bietenholz and I. Hip, J. Phys. Conf. Ser. 378, 012041 (2012) [arXiv:1201.6335 [hep-lat]].
- [9] A. Dromard and M. Wagner, arXiv:1309.2483 [hep-lat].
- [10] A. V. Smilga, Phys. Rev. D 55 (1997) 443 [hep-th/9607154].
- [11] C. Gattringer, I. Hip and C. B. Lang, Phys. Lett. B 466 (1999) 287 [hep-lat/9909025].
- [12] M. Lüscher, Commun. Math. Phys. 85, 39 (1982).
- [13] C. R. Gattringer, I. Hip and C. B. Lang, Nucl. Phys. B 508, 329 (1997) [hep-lat/9707011].
- [14] https://github.com/urbach/schwinger.
- [15] S. R. Coleman, Subnucl. Ser. 15, 805 (1979).


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Real Estate Broker of Kadriorg Bureau
Bureau: Tallinn,Kadriorg
+372 56 220 777
About Me
I joined Uus Maa Kadriorg real estate agency team in November 2018. Although I had 9 years of previous marketing and entrepreneurial experience, I had to quickly acquire additional real estate specific knowledge. I was briefly involved in real estate sales back in 2007-2009 selling housing developments in the outskirts of Tallinn and in Tartu.
I am an active and results oriented broker. I love my job which makes it especially enjoyable. It is always a pleasure to see happy customers who have just found their dream home or business premises.
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My Achievements
Best Novice Broker - december 2018
Biggest annual turnover amongst novice brokers in 2019
Largest number of transactions in Uus Maa Kadriorg office in 2019


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Learn the rules of this common graphical language and apply them confidently to your process workflows with this BPMN 2.0 course!
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The course takes a step-by-step approach to train professionals to model business processes. They will learn to use the BPMN 2.0 standard across all business domains with precision. Professionals who complete this course will have a clear understanding of BPMN diagram specifications, as well as the rules that keep them consistent across a business.
During the course, learners will master the art of creating BPMN diagrams with clear process logic and solid adherence to the world-class modeling method.
Benefits for Individuals
This BPMN 2.0 course provides introductory and advanced level training in BPMN's process-oriented modeling system. Students will learn to understand and create BPMN process diagrams, enabling them to break business processes down and represent them coherently.
The course is ideal for professionals who want to learn how to optimize business processes. BPMN 2.0 Foundation and Practitioner is an excellent option for professionals eager to thrive in a career in business analysis or process design.
Benefits for Organizations
The primary purpose of this training suite is to provide learners with a solid understanding of the BPMN notation. The modeling language is easily accessible for business users, making it easy to bridge the gap between the business analysts who draft processes and the technical teams who develop and implement them.
Training your teams in BPMN 2.0 will standardize the business modeling process in your company. You will benefit from the clear communication of requirements between all business users involved in design and implementation processes.
Course Outline
BPMN Level 1
Module 1: Course Overview
An overview of the course objectives and the BPMN modeling tool.
Module 2: What is BPMN?
An explanation of the purpose of BPMN and its important role in clear and effective business process modeling.
Module 3: Getting Started with BPMN
A chance to familiarise yourself with the Orbus BPMN 2 template to model straightforward process diagrams.
Module 4: Pools, Sub-Processes and Hierarchical Modeling
A detailed view of the interactions between entities in a process model. An explanation of the BPMN symbols and shapes that make up the modeling language.
Module 5: Collaboration and a 'Complete' Top-Level Diagram
An exploration of collaboration in a complete process model diagram.
Module 6: BPMN Concepts and High-Level Map
An explanation of the essential concepts supporting well-designed process models.
A practical guide to the first two steps of the model: Scoping the Process and High-Level Map.
Module 7: Creating BPMN with the Method
An explanation of translating a High-Level Map into a BPMN Diagram. An overview of child-level diagrams and how to effectively add message flows to diagrams.
Module 8: BPMN Style
An overview of the basic elements of the BPMN style at Level 1.
BPMN Level 2
Module 1: Events Overview and Using Timer Events
An overview of the use of events in BPMN models. A detailed look at Timer events.
Module 2: Sending, Receiving and Using Message Events
An explanation of Message events in BPMN models.
Module 3: Using Error, Event Sub-Processes and Other Level 2 Elements
An explanation of the 'Error' event in the model and the other important Level 2 event types.
Module 4: Branching and Merging
A detailed look at branching and merging with gateways and conditional sequence flows.
Module 5: Iteration
An explanation of using loop and multi-instance activities in BPMN to describe iterative process behavior.
Module 6: Following the Rules and Next Steps
An overview of the BPMN metamodel, XML, rules, and model validation.
Each module is designed to train learners in creating BPMN business process models with precision and aligning them with wider business goals. There are also regular knowledge checks and scenario-based BPMN example exercises to complete.
The course is designed with retention and application in mind. Answers will be provided for each exercise to help learners work through tough topics. Learners who complete the course will earn a completion certificate.
For more information, please contact us at firstname.lastname@example.com.
- 6 months' access from the date of purchase to complete your training
- 7 hours of online training content
- An interactive and engaging training experience
- Exam simulator with mock exams
- Additional practice assignments
- Searchable microlearning units and modules
- On/off tracker
- Access through multiple devices
- Offline player for studying on the move
- Access to Orbus' Learning Ecosystem, including:
- Detailed personal performance report
- Enrolment in a community for business and IT professionals
- Free resource center (articles, case studies, white papers, etc.)
- Support suite
- Tutor support
- Study schedule
What is BPMN?
BPMN, or 'Business Process Model and Notation', is the de-facto standard for business process modeling. It is maintained by the Object Management Group and offers a common language for modeling process workflows in all areas of a business.
Why is the BPMN standard important?
Business processes have changed dramatically over the last decade or so. They have become more complex, with more factors and participants involved. BPMN provides a standardized modeling technique, giving users a royalty-free notation similar to the popular UML standard used in software engineering.
What are the prerequisites for this course?
There are no formal prerequisites for this course.
What is the duration of this course?
This course provides 7 hours' worth of training materials. This includes all the learning modules and quizzes.
How long can users access this course?
Learners receive 6 months of access from the purchase date of the course.
Is there an exam with this course?
There is no formal assessment as part of this course, but there are regular checks and exercises to help students retain their new knowledge. Learners who complete the course will earn a completion certificate.
For more information, please contact us at firstname.lastname@example.com.
Does the course include a manual?
The course does not require a manual.
How does the on/off tracker work?
Based on our research on learner experiences and effective knowledge retention, we have designed an online tracker that provides learners with ideal time durations for completing our courses. It even gives them email reminders when they go off-track. This takes into account the ideal amount of time professionals can put aside for training amidst their busy schedules.
Please note that the tracker is an optional feature that works on a recommended timeframe. It does not have any impact on the duration of user access.
Which Learning Management System (LMS) does the course use?
The Docebo LMS is integrated into the Orbus Learning Ecosystem.
What are the minimum system and browser requirements?
Click here to view the latest system and browser requirements to run this course efficiently.
How can I get help?
For tutor, technical and administrative support, please mail us on email@example.com.
This course is delivered by Good e-Learning who are the accredited training provider.
{{course.Price | currencySymbol:course.Currency}}
Key Features
Duration of access:
6 months
Training hours:
7 hours
Accredited by:
Good e-Learning
Certification of completion
Why train with Orbus Software
Training a team?
Read more about our Corporate training services.Read more
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Why Choose Orbus Online Training
Trusted, approved and accredited courses
High quality self-paced training designed by industry experts
20,000 Active Users
Innovative ecosystem for formal, social and experiental learning
Extensive Report Suite
Business driven CMTI reporting for the entire organization
24/7 access through multiple devices
Offline mode to study on the move
Browser & System Requirements
This page carries the minimum browser and system requirements for Orbus eLearning and a few technical limitations we should keep you aware of. For any further questions, contact our support team on email@example.com.
Supported desktop and browsers
Internet Explorer 11
Microsoft Edge*
Mozilla Firefox*
Google Chrome*
Mozilla Firefox*
Google Chrome*
iOS: Default browsers in version 10 and above
Android: Default browser in version 6.0 and above
Last two major releases of the recommended browsers.
Supported mobile operating systems
iOS 10
Android 6.0
Last two major releases of the
recommended operating systems.
PC Users
Windows Vista
MS Windows 8 (or higher)**
Mac Users
OS X 10.5 or higher
OSX (Last two major releases)
Internet Download Speed
0.768 Mbps
1.5 Mbps
Internet Upload Speed
0.384 Mbps
1 Mbps
Other Browser Settings
Cookies must be enabled
Local Storage must be enabled
Please Note:
* Browser
- If the learning management system (LMS) does not open, please check that your browser is not blocking the pop-up.
- Microsoft Edge, Firefox, Chrome and Safari follow a continuous release policy that makes difficult to fix a minimum version. For this reason, following the market recommendation our LMS provider, Docebo, will support only the last 2 major versions of each of these browsers.
** Operating System
Windows XP is no longer supported by its original vendor, Microsoft, but if your organization has internal policies that have extended the use of Windows XP, our LMS provider, Docebo, recommends that your PCs be migrated to MS Windows 8 or above at your earliest convenience. Docebo strongly recommends that clients maintain updated operating systems (both desktop and mobile) aligned to the latest release made available by the respective vendors.
Convince Your Boss Email
Dear [your boss's name]:
I'd like to expand and prove my technical skills by earning a BPMN 2.0 Foundation and Practitioner (level 1 and 2) Certification. The registration fee is {{course.Price | currencySymbol:course.Currency}}.
When I pass this certification, you'll have proof of my ability to work with BPMN 2.0 Foundation and Practitioner (level 1 and 2). Orbus Software has training and online resources to help me prepare for the exam. I believe I'll be more effective and productive after achieving this valuable technical certification.
Let me know if you have any questions. In the meantime, you can find out more about this at https://www.orbussoftware.com/online-training/business-process-analysis/bpmn-20-foundation-and-practitioner-level-1-and-2/. As you can see, the exam validates skills that are crucial to our team's success.
Thank you for your support,
[your name]


text:
- 0
- 0
KennySegal – a history of black informations
0:00 / 3:18Purchase
about music
so this wraps up the #SegalSummerBootlegSeries...this time I dedicated it to one of my favorite rappers, @open-mike-eagle. you can download all the tracks in the series for free here: https://kennysegal.bandcamp.com/album/segalsummerbootlegseries-2 thank you for all the <3 also shout outs to @ruff-draft for the initial spark of inspiration that led to this track, and @mr_carmack for letting me record his stony jabroney bass playing at 3am before I chopped the shit out of it. mastered by @nalepa


text:
3322 Chanate Road , Santa Rosa, California 95404
Currently Has Openings
- OverviewClinic & Center Description:
Sonoma County Behavioral HealthLanguages:
- Spanish
- DetailsServices Offered:
Approaches to Therapy:
- Case Management
- Crisis Intervention Team
- Family Therapy
- Group Therapy
- Individual Therapy
- Intensive Case Management
- Psychiatric Emergency Walk-Ins
- Psychosocial Rehabilitation Services
- Supportive Employment
- Supportive Housing
- Suicide Prevention Services
- Integrated Primary Care Services
Tags: adolescents, adults, Anxiety, Case Management, children, Children with Emotional Disturbance (ED), Co-occurring Disorders, Court Referred, Crisis Intervention Team, Crisis Intervention, Day Treatment, Depression, Dual Diagnosis, Eating Disorders, Emotional Disturbance, Family Therapy, Group Therapy, Individual Therapy, Integrated Primary Care Services, Intensive Case Management, Older Adults, outpatient, Partial Hospitalization / Day Treatment, Partial Hospitalization, Peer Support, Psychiatric Emergency Walk-Ins, Psychiatric Emergency, Psychosocial Rehabilitation Services, Referred by Court / Judicial System, schizoaffective, schizophrenia, Seniors and Older Adults, Seniors, Serious Mental Illness, SMI (Serious Mental Illness), SMI, Suicide Prevention Services, Supportive Employment, Supportive Housing, Teens, Transition-Aged Youth, Walk In, and Young AdultsAges Accepted:
- BMT (Behavior Modification Therapy)
- CBT (Cognitive Behavioral Therapy)
Clinic Setting:
- Children
- Adolescents
- Adults
- Outpatient
- AvailabilityCurrently Accepting Clients: YesNear Public Transportation?: NoTeletherapy:
- No
- PaymentCurrently Accepting Health Insurance?:
- Medicare
- Medicaid
- TriCare
Phone: 707-565-4850
Primary Intake number: 707-565-6900
No Records Found
Sorry, no records were found. Please adjust your search criteria and try again.
Google Map Not Loaded
Sorry, unable to load Google Maps API.


text:
11 Granny Square Crochet Patterns for Square Crochet Projects
Bonus: Get our newsletter & special offers for free. We will not share or sell your email address. View our Privacy Policy
Latest Comments
"Easy Raspberry Ripple Baby Blanket is what you sent me via email. Yet, this is what comes up. Searching, I can't find it. Can you help? Donna Lee"
"Can't print not centered half of the instructions are cut off!!!"
"Very pretty, but unfortunately Im unable to read the pattern as theres an advert plastered across it! So frustrating!"
"I know we are supposed to encourage others in their endeavours but sometimes it must be more humane to put them out of their misery, I can't believe someone would admit to creating the smiley lion Afghan.let alone publish it on their website lol."
"The link is no good for the pattern for the blanket."
Springtime Crochet Granny Square
We are adding the pattern to your Afghan Patterns.
This project has been added to your afghan patterns.
Click here to view your crochet patterns.
Bright and colorful as can be, the Springtime Crochet Granny Square is a cheerful design that will look amazing in a larger project. The easy crochet granny square uses yarn in an assortment of vivid colors, resulting in a square that is eye-catching and mesmerizing. You'll especially enjoy the floral designs around the squares! As this crochet pattern uses a wide range of colors, you might be able to make the square using materials found in your yarn stash. This beautiful crochet pattern is just the right design for anyone looking for a quick project that won't take long to make.
Crochet HookI/9 or 5.5 mm hook
Yarn Weight(4) Medium Weight/Worsted Weight and Aran (16-20 stitches to 4 inches)
Crochet Gauge4 stitches and 2 rounds = 1 inch
Finished SizeApproximately 12″ x 12″
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Little Gracie Baby Blanket
"Combine this simple stitch pattern with a solid yarn for an heirloom-quality baby blanket. Or, create something whimsical using… Continue reading: "Little Gracie Baby Blanket"
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- How To Crochet: 14 Flower Crochet Granny Squares
- How to Crochet: 16 Quick and Easy Granny Square Patterns
- The Crocheter's Gift Guide: Free Crochet Afghan Patterns, Baby Blankets and More for All Occasions


text:
Property Details
Basic Information
- Property Type: Attached
- MLS Number: 72640836
- Square Feet: 2,020
- Year Built: 1984
- Zoning: Res
- Rooms: 7
- Foundation: Poured Concrete
- Town: Cohasset
- County: Norfolk
- State: MA
- Zip: 02025
Interior Features
- Description: Located in desirable Cedar Ledge Village, convenient to Town, the Common and the Train Station as well as a sidewalk to Black Rock Beach and Wheelwright Park, this large move-in-ready 7- Room, 3- Bedroom, 2.5- Bath home features a spacious open floor plan for today's living with kitchen-dining-living and family spaces all leading out to a beautiful sunny deck and a flat yard bordered by a stone wall and evergreen trees for four season enjoyment. The updated kitchen with its new transom window is filled with light and overlooks all the living areas and the outdoors. A welcoming front yard entry invites you in to a two-story staircase, excellent closet space, laundry and half bath plus a "great room view to the night-lighted deck and woodlands beyond". A door leads to the attached, oversized garage with additional storage. Upstairs is a large master suite with full bath and walk-in closet. Two additional generous size bedrooms are served by a full bath. An impeccable home and village !!!
- Waterfront: No
- Bedrooms: 3
- Basement: No
- Family Room Description: Flooring - Hardwood, Deck - Exterior, Exterior Access, Open Floor Plan, Slider
- Family Room Level: First Floor
Dining Room
- Dining Room Description: Flooring - Hardwood, Open Floor Plan
- Dining Room Level: First Floor
- Kitchen Description: Flooring - Stone/Ceramic Tile, Dining Area, Countertops - Stone/Granite/Solid, Open Floor Plan, Recessed Lighting, Peninsula
- Kitchen Level: First Floor
Exterior Features
- Parking Description: Off-Street, Paved Driveway
Utilities and Appliances
Utilities and Appliances
- Cooling: None
- Water: City/Town Water
- Elementary School: Osgood/DeerHill
- Junior High: Cohasset Middle
- High School: Cohasset High
- Adult Community: No
- Miles to Beach: 1 to 2 Mile
Other Details
- Taxes: $4,494
- Tax Year: 2020


text:
|MK809 IV Android 7 1 TV Dongle RK3229 Quad Core 2G 16G UHD 4K Smart TV Stick HD 3D Mini PC H 265 WiFi DLNA Smart MediaPlayer
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Medium: Local Media Playback, supports HDD, U disk, TF card, etc. Specifications: Model Number: MK809 IV Power: DC input 5V/2A I / O: 1 HD Up to 4K ; 1 USB 2.0 port; 1 TF Card Slot; 1 Micro USB with OTG Connect PC ; 1 Power Input Micro USB port 5V/2A . Color: Black with Red Main Item Size: 9.5 3.8 1.2cm / 3.7 1.49 0.47in Main Item Weight: 28g / 1.0oz Package Size: 13.5 9.5 5.2cm / 5.3 3.74 2.0in Package Weight: 192g / 6.8oz. Package List: 1 MK809 IV Android 7.1 TV Dongle 1 Power Adapter 1 USB Female to Micro USB Male 1 HD Male to HD Female cable 1 English User Manual 1 We accept Alipay, West Union, TT. All major credit cards are accepted through secure payment processor ESCROW. 2 Payment must be made within 3 days of order. 3 If you can t checkout immediately after auction close, please wait for a few minutes and retry Payments must be completed within 3 days. 1. WORLDWIDE SHIPPING. Except some countries and APO/FPO 2. Orders processed timely after the payment verification. 3. We only ship to confirmed order addresses. Your order address MUST MATCH your Shipping address. 4. The images shown are not the actual item and are for your reference only. 5. SERVICE TRANSIT TIME is provided by the carrier and excludes weekends and holidays. Transit times may vary, particularly during the holiday season. 6. If you have not received your shipment within 45 days from payment, please contact us. We will track the shipment and get back to you as soon as possible with a reply. Our goal is customer satisfaction 7. Due to stock status and time differences, we will choose to ship your item from our first available warehouse for fast delivery. 8. Delivery Time: 1. You have 7 days to contact us and 30 days to return it from the date it was received. If this item is in your possession more than 7 days, it is considered used and WE WILL NOT ISSUE YOU A REFUND OR REPLACEMENT. There are NO EXCEPTIONS Shipping cost is bear by both seller and buyer in half. 2. All returned items MUST BE in the original packaging and you MUST PROVIDE us with the shipping tracking number, specific reason for the return, and your po . 3. We will refund YOUR FULL WINNING BID AMOUNT, upon receipt of the item in its original condition and packaging with all components and accessories included, AFTER BOTH Buyer and Seller cancel the transaction from aliexpress. OR, you may choose to have a replacement. 4. We will bear all the shipping cost if the product s is are not as advertised. 1. 12 months Manufacturer s limited Warranty for defective items excluding items damaged and/or misused after receipt . Accessories come with a 3-month warranty. 2. Defective items MUST BE reported and returned within the warranty period and in the original packaging, if possible . You must tell us what the defect is and give us your order number. WE DO NOT REPAIR OR REPLACE ITEMS WITH AN EXPIRED WARRANTY. You agree to all of the above-listed policies upon ordering on aliexpress We maintain high standards of excellence and strive for 100 customer satisfaction Feedback is very important We request that you contact us immediately BEFORE you give us neutral or negative feedback, so that we can satisfactorily address your concerns. 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