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The Ultraviolet Luminosity Function at 0.6 < Z < 1 from UVCANDELS

Lei Sun,Xin Wang,Harry I. Teplitz,Vihang Mehta,Anahita Alavi,Marc Rafelski,Rogier A. Windhorst,Claudia Scarlata,Jonathan P. Gardner,Brent M. Smith,Ben Sunnquist,Laura Prichard,Yingjie Cheng,Norman Grogin,Nimish P. Hathi,Matthew Hayes,Anton M. Koekemoer,Bahram Mobasher,Kalina V. Nedkova,Robert O'Connell,Brant Robertson,Sina Taamoli,L. Y. Aaron Yung,Gabriel Brammer,James Colbert,Christopher Conselice,Eric Gawiser,Yicheng Guo,Rolf A. Jansen,Zhiyuan Ji,Ray A. Lucas,Michael Rutkowski,Brian Siana,Eros Vanzella,Teresa Ashcraft,Micaela Bagley,Ivano Baronchelli,Guillermo Barro, Alex Blanche,Adam Broussard,Timothy Carleton,Nima Chartab,Alex Codoreanu,Seth Cohen,Y. Sophia Dai,Behnam Darvish,Romeel Dave,Laura DeGroot,Duilia De Mello,Mark Dickinson,Najmeh Emami,Henry Ferguson,Leonardo Ferreira,Keely Finkelstein,Steven Finkelstein,Timothy Gburek,Mauro Giavalisco,Andrea Grazian,Caryl Gronwall,Shoubaneh Hemmati,Justin Howell,Kartheik Iyer,Sugata Kaviraj,Peter Kurczynski,Ilin Lazar,John Mackenty,Kameswara Bharadwaj Mantha,Alec Martin,Garreth Martin,Tyler Mccabe,Charlotte Olsen,Lillian Otteson,Swara Ravindranath,Caleb Redshaw,Zahra Sattari,Emmaris Soto, Bonnabelle Zabelle

The Astrophysical Journal（2024）

Cited 7|Views101
Key words
Galaxies,Galaxy evolution,Luminosity function,High-redshift galaxies
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