VizieR Online Data Catalog: The UNCOVER phot. catalog of A2744 wiht HST+JWST (Weaver+, 2024)

The photometric catalogs presented herein include all public JWST/NIRCam imaging of A2744 available to date: the Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization (UNCOVER) Treasury survey (PIs: Labbe & Bezanson, JWST-GO-2561; Bezanson+ 2022arXiv221204026B), the Early Release Science (ERS) GLASS-JWST program (PI: Treu, JWST-DD-ERS-1324; Treu+ 2022ApJ...935..110T), and a Directors Discretionary Time (DDT) program (JWST-DD-2756, PI: Chen). Our data set combines the deep NIRCam imaging with 4-6hr exposures in seven filters (F115W, F150W, F200W, F277W, F356W, F410M, and F444W) from UNCOVER, with the ultradeep imaging with 9-14hr exposures from GLASS-ERS in seven filters (F090W, F115W, F150W, F200W, F277W, F356W, and F444W). Additionally, the DDT program includes two epochs of NIRCam imaging in six filters (F115W, F150W, F200W, F277W, F356W, and F444W), totaling ~1hr per filter. See Section 2.1.

A wide range of imaging of the A2744 cluster and surrounding area exists within the public HST archive. Briefly, we summarize the programs relevant herein. Program HST-GO-11689 (PI: Dupke) and HST-GO-13386 (PI: Rodney) include deep HST/Advanced Camera for Surveys (ACS) imaging in the cluster center in three filters (F435W, F606W, and F814W), with program HST-DD-13495 (PI: Lotz; Lotz+ 2017ApJ...837...97L) acquiring complementary deep HST/Wide Field Camera 3 (WFC3) observations in four filters (F105W, F125W, F140W, and F160W). While each of the above programs are (deep) individual pointings limited by the ACS and WFC3 fields of view (FOVs), respectively, the data were later expanded by a factor of 4 with shallower imaging in two ACS filters (F606W and F814W) and three WFC3 filters (F105W, F125W, and F160W) by the BUFFALO survey (Program HST-GO-15117, PIs: Steinhardt & Jauzac; Steinhardt+ 2020ApJS..247...64S). Most recently, the deep optical coverage was further expanded by Program JWST-DD-17231 (PI: Treu). See Section 2.2.

All magnitudes in this paper are expressed in the AB system, for which a flux f_ν of 10nJy (10^-28erg/cm²/s/Hz) corresponds to AB_v=28.9-2.5log₁₀(f_v/uJy). When computing physical properties such as rest-frame fluxes, we adopt a standard ΛCDM cosmology with H₀=70km/s/Mpc, Ω_M=0.3, and Ω_Λ=0.7.

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