Now showing items 1-2 of 2

    • Galaxy Zoo: Quantitative Visual Morphological Classifications for 48,000 galaxies from CANDELS 

      Simmons, B. D.; Lintott, Chris; Willett, Kyle W.; Masters, Karen L.; Kartaltepe, Jeyhan S.; Häußler, Boris; Kaviraj, Sugata; Krawczyk, Coleman; Kruk, S. J.; McIntosh, Daniel H.; Smethurst, R. J.; Nichol, Robert C.; Scarlata, Claudia; Schawinski, Kevin; Conselice, Christopher J.; Almaini, Omar; Ferguson, Henry C.; Fortson, Lucy; Hartley, William; Kocevski, Dale; Koekemoer, Anton M.; Mortlock, Alice; Newman, Jeffrey A.; Bamford, Steven P.; Grogin, N. A.; Lucas, Ray A.; Hathi, Nimish P.; McGrath, Elizabeth; Peth, Michael; Pforr, Janine; Rizer, Zachary; Wuyts, Stijn; Barro, Guillermo; Bell, Eric F.; Castellano, Marco; Dahlen, Tomas; Ownsworth, Avishai Dekel Jamie; Faber, Sandra M.; Finkelstein, Steven L.; Fontana, Adriano; Galametz, Audrey; Grützbauch, Ruth; Koo, David; Lotz, Jennifer; Mobasher, Bahram; Mozena, Mark; Salvato, Mara; Wiklind, Tommy (2017-02-01)
      We present quantified visual morphologies of approximately 48,000 galaxies observed in three Hubble Space Telescope legacy fields by the Cosmic And Near-infrared Deep Extragalactic Legacy Survey (CANDELS) and classified ...
    • Investigating the Dominant Environmental Quenching Process in UVCANDELS/COSMOS Groups 

      Kuschel, Maxwell; Scarlata, Claudia; Mehta, Vihang; Teplitz, Harry I.; Rafelski, Marc; Wang, Xin; Sunnquist, Ben; Prichard, Laura; Grogin, Norman; Koekemoer, Anton; Windhorst, Rogier; Rutkowski, Michael; Alavi, Anahita; Chartab, Nima; Conselice, Christopher J.; Dai, Y. Sophia; Gawiser, Eric; Giavalisco, Mauro; Haro, Pablo Arrabal; Hathi, Nimish; Jansen, Rolf A.; Ji, Zhiyuan; Lucas, Ray A.; Mantha, Kameswara; Mobasher, Bahram; O’Connell, Robert W.; Robertson, Brant; Sattari, Zahra; Yung, L. Y. Aaron; Davé, Romeel; DeMello, Duilia; Dickinson, Mark; Ferguson, Henry; Finkelstein, Steven L.; Hayes, Matt; Howell, Justin; Kaviraj, Sugata; Mackenty, John W.; Siana, Brian (2023-04-12)
      We explore how the fraction of quenched galaxies changes in groups of galaxies with respect to the distance to the center of the group, redshift, and stellar mass to determine the dominant process of environmental quenching ...