PI: Sheila J Kannappan, U. of North Carolina, firstname.lastname@example.org
Address: Physics Department, 290 Phillips Hall, CB3255, Chapel Hill, NC 27599 USA
CoI: Kathleen Eckert, U. of North Carolina
CoI: Dara Norman, NOAO
CoI: Mark Norris, Max Planck Institut fur Astrophysik
CoI: Erik A Hoversten, U. of North Carolina
CoI: David V Stark, U. of North Carolina
CoI: Amanda Moffett, U. of North Carolina
CoI: Ashley D Baker, U. of North Carolina
CoI: Andreas Berlind, Vanderbilt U.
CoI: Steve Michael Crawford, SAAO
CoI: Ivana Damjanov, Harvard-Smithsonian Center for Astrophysics
CoI: Ian dell'Antonio, Brown U.
CoI: Roberto Gonzalez, U. of Chicago
CoI: Kirsten Hall, U. of North Carolina
CoI: Sadegh Khochfar, Max Planck Institut fuer extraterrestrische Physik
CoI: Adam Leroy, NRAO
CoI: Yu Lu, Stanford U.
CoI: Claudia Maraston, University of Portsmouth
CoI: Stacy McGaugh, Case Western Reserve U.
CoI: Liz Naluminsa, SAAO
CoI: John J Salzer, Indiana U.
CoI: Jerry A Sellwood, Rutgers U.
CoI: Petri Vaisanen, SAAO
CoI: Linda Watson, Harvard-Smithsonian Center for Astrophysics
Title: REsolved Spectroscopy Of a Local VolumE: The RESOLVE Survey in Stripe 82
Abstract: We request 14 nights of gray/dark time with the Goodman Spectrograph on SOAR and 88 hours of gray/dark time with the GMOS IFU on Gemini over two semesters to complete Phase~1 of the RESOLVE survey, providing a volume-limited gas, stellar, and dynamical mass census in the exceptionally complete Stripe 82 legacy equatorial strip. RESOLVE spans diverse large-scale cosmic structures and probes mass scales down to $\sim$^9$\msun\ in the gas-rich dwarf galaxy regime. With the proposed census, RESOLVE will (1) provide the first direct, complete, and environment-dependent measurement of the velocity function, potentially uncovering crucial clues to puzzling discrepancies in the dwarf galaxy inventory, and (2) put a unique constraint on the location of the ``missing baryons,'' via a comprehensive census of multiple mass components in relation to star formation and dynamical mass in a cosmological volume.
Program Type: Survey
Run 1 (2013B): SOAR/Goodman -- 6n on Sep 04 - Sep 05 2013, Oct 07 - Oct 08 2013, Oct 30 - Nov 01 2013
Run 1 (2014B): SOAR/Goodman -- 8n on Aug 30 - Sep 02 2014, Sep 17 2014, Sep 24 - Sep 25 2014, Oct 18 - Oct 19 2014, Nov 18 2014
Run 1 (2015B): SOAR/Goodman -- 3n on Nov 10 - Nov 12 2015
Run 3 (2013B): GEM-SQ/GMOSS -- 10hrs band 2 (GS-2013B-Q-51)
Run 3 (2014B): GEM-SQ/GMOSS -- 22hrs band 1 (GS-2014B-Q-13)
Run 4 (2014B): GEM-S/GMOSS -- 17hrs band 2 (GS-2014B-Q-52)
Run 5 (2015B): GEM-S/GMOSS -- 6n on Nov 06 - Nov 11 2015
National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360