Gillian Wilson

6 ta ish

University of California, Merced

1. Star Formation in AEGIS Field Galaxies since <i>z</i>  = 1.1: The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-forming Galaxies

   K. G. Noeske, Benjamin J. Weiner, S. M. Faber +26

   Maqola20075 iqtibos

   ABIABI:AkademIndex/2026.other.467852

2. The All-Wavelength Extended Groth Strip International Survey (AEGIS) Data Sets

   M. Davis, Puragra Guhathakurta, Nicholas P. Konidaris +53

   Maqola20073 iqtibos

   ABIABI:AkademIndex/2026.other.467794

3. The stellar mass function of quiescent galaxies in 2 &amp;lt; <i>z</i> &amp;lt; 2.5 protoclusters

   Adit H Edward, Michael L. Balogh, Yannick M Bahé +21

   Maqola20233 iqtibos

   ABIABI:AkademIndex/2026.other.467801

4. Evidence for strong evolution in galaxy environmental quenching efficiency between z = 1.6 and z = 0.9

   Julie Nantais, Adam Muzzin, R. F. J. van der Burg +7

   Maqola20162 iqtibos

   ABIABI:AkademIndex/2026.other.526178

5. MAGAZ3NE: Massive, Extremely Dusty Galaxies at z ∼ 2 Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at 3 &lt; z &lt; 4*

   Ben Forrest, Michael C. Cooper, Adam Muzzin +17

   Maqola20241 iqtibos

   ABIABI:AkademIndex/2026.other.467807

6. Environmental Effects on the Stellar Mass Function in a z ∼ 3.3 Overdensity of Galaxies in the COSMOS Field*

   Ben Forrest, B. C. Lemaux, Ekta A. Shah +17

   Maqola20241 iqtibos

   ABIABI:AkademIndex/2026.other.467808