A Deep, Large-Angular-Scale Redshift Survey of Galaxies
{'Code': '03020400', 'Directorate': {'Abbreviation': 'MPS', 'LongName': 'Direct For Mathematical & Physical Scien'}, 'Division': {'Abbreviation': 'AST', 'LongName': 'Division Of Astronomical Sciences'}}
{'SignBlockName': 'Pol C. Delosreyes', 'PO_EMAI': None, 'PO_PHON': None}
A deep survey of galaxy redshifts in a 1 degree x 100 degree                    strip on the sky will be carried out using dedicated time on the                new McGraw-Hill Observatory 2.4-meter telescope.  The galaxy                    catalogue will be provided by M. Geller, J. Huchra, and M. Kurtz                of the Center for Astrophysics who are conducting a                             complementary photometric survey and collaborating on this                      project.  The catalogue will be derived from photodensitometer                  scans of the Palomar Sky Survey.  Some of the most difficult                    galaxies will be measured with the Multi-Mirror Telescope (MMT)                 at Mount Hopkins. Measurements of redshifts for about 2000                      galaxies will be carried out.  The typical redshifts will be                    about 24,000 km per second.                                                                                                                                     The survey strip is chosen for observational convenience alone,                 and should constitute a "fair" sample of the Universe.  It runs                 down the middle of the strip surveyed by deLapperant, Geller, and               Huchra in 1986, but extends to over twice the depth of their                    survey.  Among the issues which this survey will clarify are:                   (1) the upper limit on void volumes; (2) the relationship between               rich clusters and the structures that surround them; (3) the                    galaxy luminosity function; and (4) whether low luminosity                      galaxies are distributed in structures similar to the more                      luminous ones.  Finally, a few dozen galaxies with peculiar                     spectra, especially active galactic nuclei, should be discovered.
[{'FirstName': 'Gary', 'LastName': 'Wegner', 'PI_MID_INIT': 'A', 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'Gary A Wegner', 'EmailAddress': 'gaw@bellz.dartmouth.edu', 'PI_PHON': '6036463329', 'NSF_ID': '000431687', 'StartDate': '08/01/1987', 'EndDate': None, 'RoleCode': 'Co-Principal Investigator'}, {'FirstName': 'John', 'LastName': 'Thorstensen', 'PI_MID_INIT': 'R', 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'John R Thorstensen', 'EmailAddress': 'john.thorstensen@dartmouth.edu', 'PI_PHON': '6036462869', 'NSF_ID': '000142767', 'StartDate': '08/01/1987', 'EndDate': None, 'RoleCode': 'Principal Investigator'}]
{'Name': 'Dartmouth College', 'CityName': 'HANOVER', 'ZipCode': '037552170', 'PhoneNumber': '6036463007', 'StreetAddress': '7 LEBANON ST', 'StreetAddress2': None, 'CountryName': 'United States', 'StateName': 'New Hampshire', 'StateCode': 'NH', 'CONGRESSDISTRICT': '02', 'CONGRESS_DISTRICT_ORG': 'NH02', 'ORG_UEI_NUM': 'EB8ASJBCFER9', 'ORG_LGL_BUS_NAME': 'TRUSTEES OF DARTMOUTH COLLEGE', 'ORG_PRNT_UEI_NUM': 'EB8ASJBCFER9'}
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{'Code': '1217', 'Text': 'EXTRAGALACTIC ASTRON & COSMOLO'}
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