MMT Observing Programs
May - August 2012

PA-12A-0238 Fine, Shanks, Green, Croom, Webster Reverberation Mapping of ~1000 QSOsHectospec
PA-12A-0332 Brown, Walkowicz, Hawley, Kowalski, Saar, Furesz MMT Hectochelle Spectral Variability of Active Late-type Stars in the Kepler Field (2012A)Hectochelle
PA-12A-0353 Dey, Prescott, Hong Mapping the Cosmic Web at z~2.7Hectospec
SAO-1 Brown, Kilic Merging White Dwarf BinariesBlue Channel
SAO-2 Strader, Caldwell, Romanowsky, Brodie M87 and the Virgo ClusterHectospec
SAO-3 Geller, Fabricant, Kurtz, Hwang, Diaferio, Rines HectoMAP: Clusters and Large-Scale Structure at 0.25<z<0.5Hectospec
SAO-4 Brown, Kilic Remnant Planetary Systems Around White DwarfsSWIRC
SAO-5 Foley, Kirshner, Simon Circumstellar Material in Type Ia Supernova Progenitor SystemsHectochelle
SAO-6 Walker, Olszewski, Belokurov Galactic Sub-Substructure and the Nature of Ultrafaint Galaxies: Segue 1 and the Orphan StreamHectochelle
SAO-7 Strader, Caldwell, Seth, Szentgyorgyi, Ivans The Hectochelle Northern Galactic Globular Cluster SurveyHectochelle
SAO-8 Benbow, Furniss, Williams, Fumagalli, Hogan Determining Blazar Redshifts for Studies of the EBLHectospec
SAO-9 Wright, Drake, Guarcello, Hora, van der Veen, Steeghs, Drew The Stellar Content and Dynamics of Cygnus OB2Hectospec
SAO-10 Berger,Chomiuk,Chornock,Czekala,Dittmann,Drout,Foley,Kirshner,Lunnan,Margutti,Marion,Milisavljevic,Narayan,Sanders,Soderberg,Stubbs,Zauderer The MMT Spectroscopic Survey of Pan-STARRS TransientsHectospec/Blue Channel
SAO-11 Adams, Dupree, McCarthy, Kulesa High-Resolution Images of Kepler/Spitzer TargetsNGS/ARIES
SAO-12 Meibom, Barnes, Furesz, Latham, Szentgyorgyi Toward Better Ages for Stars and Their PlanetsHectochelle
SAO-13 Hora, Koenig, Cygnus-X Team Characterization of Cygnus-X Young Stellar Objects with HectospecHectospec
SAO-14 Dupree, Adams, Gilliland Double Dipping and More in the Kepler Field IIHectochelle
SAO-15 Benbow, Furniss, Williams, Fumagalli, Hogan Parallel Observations to Determine Blazar Redshifts for Studies of the EBLHectospec
UAO-E15 Bendek, Hart, McCarthy, Kulesa, Newman Commissioning ARIES Spectroscopy and Detailed Performance Characterization with the MMT GLAO SystemLGS/ARIES
UAO-G44 Jones, Packham, Shenoy Imaging Polarimetry with MMTPolMMTPol
UAO-G45 Humphreys, Grammer Luminous and Unstable Stars in N4214 and M101Hectospec
UAO-G49 Evans, Borish, Privon, Kim, McCarthy, Kulesa, Armus, Petric, Surace Nuclear Star Formation and AGN Activity in Luminous Infrared Galaxy MergersNGS/ARIES
UAO-G50 Zheng, Yan, Shi, Mao, Huang, Gu, Chen, Xia, Hao WISE+UKIDSS: Unveiling Rapid Black Hole Growth in ObscurationRed Channel UAO-G51 Fang, H. Wang, M. Wang Spectroscopic Survey of Young Stars in North American and Pelican NebulaeHectospec
UAO-S1 Cai, Fan, Frye, McGreer MApping the Most Massive Overdensity Through Hydrogen (MAMMOTH)Blue Channel
UAO-S2 Patience, King, De Rosa, Bell, Scowen Confirmation and Characterization of Substellar and Degenerate CompanionsNGS/ARIES
UAO-S3 McGreer, Fan, Jiang The Faint QSO Luminosity Function at z ~ 5 from CFHTLS-W3Red Channel
UAO-S4 Windhorst, Morrison, Arnouts, Yun, Owen, Dickinson, Miller, Keel, Sengupta, Miller Abell 1882-SuperGroup: Galaxy Cluster Assembly at z = 0.14Hectospec
UAO-S6 Dey, Lee, Jannuzi A Search for the Most Actively Star-Forming Galaxies at z ~ 3.7Hectospec
UAO-S9 Stark, Belokurov, Robertson, Auger, Sand Physical Properties of Gravitationally-Lensed Galaxies in SDSSRed Channel
UAO-S11 Clément, Egami, Jiang Spectroscopic Identification of z ~ 6 7 Candidates in Massive Lensing Cluster Fields and the Subaru Deep FieldRed Channel
UAO-S12 Olszewski, Walker, Mateo, Belokurov Galactic Sub-Substructure and the Nature of Ultrafaint Galaxies: Segue 1 and the Orphan StreamHectochelle
UAO-S17 Smith, Bilinski, Mauerhan Constraining Pre-Supernova Mass Loss: Spectroscopy of Circumstellar Gas Overtaken by the Blast WaveBlue Channel
UAO-S20 Smith, Mauerhan Spectroscopic Followup of Explosive Massive-Star TransientsBlue Channel
UAO-S30 Zheng, Rhoads, Malhotra, McLinden, Smith Lyman Alpha Emitters at z = 2.1: Evolution on both the Ly- Luminosity Function and the Spectral Energy Distribution?Hectospec