output
20072025
most citedGrackle: a Chemistry and Cooling Library for Astrophysics

343 citations

Showing astro-ph.GAShow all

18 papers · 1 filter

astro-ph.GA2025

The DESI Single Fiber Lens Search. I. Four Thousand Spectroscopically Selected Galaxy-Galaxy Gravitational Lens Candidates

Juliana S. M. Karp, David J. Schlegel, Xiaosheng Huang +47

We present 4,110 strong gravitational lens candidates, 3,887 of which are new discoveries, selected from a sample of 5,837,154 luminous red galaxies (LRGs) observed with the Dark E…

astro-ph.GA2025★ 2 cited

DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity

T. Hagen, K. S. Dawson, Z. Zheng +49

We measure the projected two-point correlation functions of emission-line galaxies (ELGs) from the Dark Energy Spectroscopic Instrument (DESI) One-Percent Survey and model their de…

astro-ph.GA2025★ 8 cited

PAC in DESI. I. Galaxy Stellar Mass Function into the Frontier

Kun Xu, Y. P. Jing, Shaun Cole +34

The Photometric Objects Around Cosmic Webs (PAC) method integrates cosmological photometric and spectroscopic surveys, offering valuable insights into galaxy formation. PAC measure…

astro-ph.GA2023★ 26 cited

No Tension: JWST Galaxies at Consistent with Cosmological Simulations

Joe McCaffrey, Samantha Hardin, John Wise +1

Recent observations by JWST have uncovered galaxies in the very early universe via the JADES and CEERS surveys. These galaxies have been measured to have very high stellar masses w…

astro-ph.GA2022★ 25 cited

How long do high-redshift massive black hole seeds remain outliers in black hole vs. host galaxy relations?

Matthew T. Scoggins, Zoltán Haiman, John H. Wise

The existence of supermassive black holes (SMBHs) within the first billion years of the universe remains a puzzle in our conventional understanding of black h…

astro-ph.GA2022★ 11 cited

Signature of Supersonic Turbulence in Galaxy Clusters Revealed by AGN-driven H Filaments

Haojie Hu, Yu Qiu, Marie-Lou Gendron-Marsolais +5

The hot intracluster medium (ICM) is thought to be quiescent with low observed velocity dispersions. Surface brightness fluctuations of the ICM also suggest that its turbulence is…