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The Lyman Continuum Escape Fraction of Star-forming Galaxies at $2.4\lesssim z\lesssim3.7$ from UVCANDELS

Authors :
Wang, Xin
Teplitz, Harry I.
Smith, Brent M.
Windhorst, Rogier A.
Rafelski, Marc
Mehta, Vihang
Alavi, Anahita
Brammer, Gabriel
Colbert, James
Grogin, Norman
Hathi, Nimish P.
Koekemoer, Anton M.
Prichard, Laura
Scarlata, Claudia
Sunnquist, Ben
Haro, Pablo Arrabal
Conselice, Christopher
Gawiser, Eric
Guo, Yicheng
Hayes, Matthew
Jansen, Rolf A.
Ji, Zhiyuan
Lucas, Ray A.
O'Connell, Robert
Robertson, Brant
Rutkowski, Michael
Siana, Brian
Vanzella, Eros
Ashcraft, Teresa
Bagley, Micaela
Baronchelli, Ivano
Barro, Guillermo
Blanche, Alex
Broussard, Adam
Carleton, Timothy
Chartab, Nima
Cheng, Yingjie
Codoreanu, Alex
Cohen, Seth
Dai, Y. Sophia
Darvish, Behnam
Dave, Romeel
DeGroot, Laura
De Mello, Duilia
Dickinson, Mark
Emami, Najmeh
Ferguson, Henry
Ferreira, Leonardo
Finkelstein, Keely
Finkelstein, Steven
Gardner, Jonathan P.
Gburek, Timothy
Giavalisco, Mauro
Grazian, Andrea
Gronwall, Caryl
Hemmati, Shoubaneh
Howell, Justin
Iyer, Kartheik
Kaviraj, Sugata
Kurczynski, Peter
Lazar, Ilin
MacKenty, John
Mantha, Kameswara Bharadwaj
Martin, Alec
Martin, Garreth
McCabe, Tyler
Mobasher, Bahram
Nedkova, Kalina
Olsen, Charlotte
Otteson, Lillian
Ravindranath, Swara
Redshaw, Caleb
Sattari, Zahra
Soto, Emmaris
Yung, L. Y. Aaron
Zabelle, Bonnabelle
team, the UVCANDELS
Publication Year :
2023

Abstract

The UltraViolet Imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) survey is a Hubble Space Telescope (HST) Cycle-26 Treasury Program, allocated in total 164 orbits of primary Wide-Field Camera 3 Ultraviolet and Visible light F275W imaging with coordinated parallel Advanced Camera for Surveys F435W imaging, on four of the five premier extragalactic survey fields: GOODS-N, GOODS-S, EGS, and COSMOS. We introduce this survey by presenting a thorough search for galaxies at $z\gtrsim2.4$ that leak significant Lyman continuum (LyC) radiation, as well as a stringent constraint on the LyC escape fraction ($f_{\rm esc}$) from stacking the UV images of a population of star-forming galaxies with secure redshifts. Our extensive search for LyC emission and stacking analysis benefit from the catalogs of high-quality spectroscopic redshifts compiled from archival ground-based data and HST slitless spectroscopy, carefully vetted by dedicated visual inspection efforts. We report a sample of five galaxies as individual LyC leaker candidates, showing $f_{\rm esc}^{\rm rel}\gtrsim60\%$ estimated using detailed Monte Carlo analysis of intergalactic medium attenuation. We develop a robust stacking method to apply to five samples of in total 85 non-detection galaxies in the redshift range of $z\in[2.4,3.7]$. Most stacks give tight 2-$\sigma$ upper limits below $f_{\rm esc}^{\rm rel}<6\%$. A stack for a subset of 32 emission-line galaxies shows tentative LyC leakage detected at 2.9-$\sigma$, indicating $f_{\rm esc}^{\rm rel}=5.7\%$ at $z\sim2.65$, supporting the key role of such galaxies in contributing to the cosmic reionization and maintaining the UV ionization background. These new F275W and F435W imaging mosaics from UVCANDELS have been made publicly available on the Barbara A. Mikulski Archive for Space Telescopes.<br />Comment: 33 pages, 21 figures, and 5 tables. Resubmitted after addressing the referee report

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2308.09064
Document Type :
Working Paper