Rachel Somerville

9 ta ish

Flatiron Health (United States)

1. The Great Observatories Origins Deep Survey: Initial Results from Optical and Near-Infrared Imaging

   Mauro Giavalisco, Henry C. Ferguson, A. M. Koekemoer +54

   Maqola20047 iqtibos

   ABIABI:AkademIndex/2026.other.467813

2. 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

3. Profiles of dark haloes: evolution, scatter and environment

   James S. Bullock, Tsafrir Kolatt, Yair Sigad +5

   MaqolaOAOchiq kirish20013 iqtibos

   ABIABI:AkademIndex/2026.other.011277

4. On the Significance of Rare Objects at High Redshift: The Impact of Cosmic Variance

   C. K. Jespersen, Charles L. Steinhardt, Rachel Somerville +1

   MaqolaOAOchiq kirish20252 iqtibos

   ABIABI:AkademIndex/2026.other.141626

5. The Rise of Faint, Red Active Galactic Nuclei at <i>z</i> &gt; 4: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields

   Dale D. Kocevski, Steven L. Finkelstein, Guillermo Barro +53

   MaqolaOAOchiq kirish20252 iqtibos

   ABIABI:AkademIndex/2026.other.141631

6. Evolution of galaxy attenuation curves driven by evolving dust mass and grain size distributions

   Kosei Matsumoto, Laura Sommovigo, Andrea Gebek +8

   MaqolaOAOchiq kirishGalaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysics20251 iqtibos

   ABIABI:AkademIndex/2025.article.001474

7. The mass evolution of the first galaxies: stellar mass functions and star formation rates at 4 &lt; z &lt; 7 in the CANDELS GOODS-South field

   K. J. Duncan, Christopher J. Conselice, A. Mortlock +16

   Maqola20141 iqtibos

   ABIABI:AkademIndex/2026.other.467796

8. Mangrove: Learning Galaxy Properties from Merger Trees

   C. K. Jespersen, Miles Cranmer, P. Melchior +3

   Maqola20221 iqtibos

   ABIABI:AkademIndex/2026.other.467828

9. The evolving slope of the stellar mass function at 0.6 ≤ <i>z</i>&lt; 4.5 from deep WFC3 data

   P. Santini, A. Fontana, A. Grazian +12

   Maqola20111 iqtibos

   ABIABI:AkademIndex/2026.other.467863