THE PAN-STARRS1 MEDIUM-DEEP SURVEY: THE ROLE OF GALAXY GROUP ENVIRONMENT IN THE STAR FORMATION RATE VERSUS STELLAR MASS RELATION AND QUIESCENT FRACTION OUT TO<i>z</i>∼ 0.8
Lihwai Lin(National Taiwan University), C. Waters(Princeton University), Bau-Ching Hsieh(National Astronomical Observatory of Japan), Chin-Wei Chen(Institute of Astronomy and Astrophysics, Academia Sinica), P. A. Price(Monterey Institute for Research in Astronomy), R. G. Bower(Cardiff University), Chien‐Hsiu Lee(National Astronomical Observatory of Japan), P. Norberg(Durham University), M. E. Huber(Technical University of Munich), Shaun Cole(Durham University), Hung-Yu Jian(Tohoku University), W. S. Burgett, N. Metcalfe(Durham University), J. Tonry(University of Hawaii System), S. Foucaud(Shanghai Jiao Tong University), N. Kaiser(University of Hawaii System), H. Flewelling(University of Hawaiʻi at Mānoa), Wenping Chen(National Central University), K. C. Chambers(University of Hawaii System), P. Arnalte-Mur(Durham University), S. Heinis(University of Maryland, College Park), S. Phleps(Max Planck Institute for Extraterrestrial Physics), R. J. Wainscoat(University of Hawaii System), R. P. Kudritzki(University of Hawaii System), L. Denneau, K. W. Hodapp(University of Hawaii at Hilo), E. A. Magnier(University of Hawaii System), Jean Coupon(Subaru (Japan)), P. W. Draper
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