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Barro, Guillermo; Perez-Gonzalez, Pablo G; Cava, Antonio; Brammer, Gabriel; Pandya, Viraj; Moral, Carmen Eliche; Esquej, Pilar; Dominguez-Sanchez, Helena; Pampliega, Belen Alcalde; Guo, Yicheng; Koekemoer, Anton M; Trump, Jonathan R; Ashby, Matthew L N; Cardiel, Nicolas; Castellano, Marco; Conselice, Christopher J; Dickinson, Mark E; Dolch, Timothy; Donley, Jennifer L; Briones, Nestor Espino; Faber, Sandra M; Fazio, Giovanni G; Ferguson, Henry; Finkelstein, Steve; Fontana, Adriano; Galametz, Audrey; Gardner, Jonathan P; Gawiser, Eric; Giavalisco, Mauro; Grazian, Andrea; Grogin, Norman A; Hathi, Nimish P; Hemmati, Shoubaneh; Hernan-Caballero, Antonio; Kocevski, Dale; Koo, David C; Kodra, Dritan; Lee, Kyoung-Soo; Lin, Lihwaj; Lucas, Ray A; Mobasher, Bahram; McGrath, Elizabeth J; Nandra, Kirpal; Nayyeri, Hooshang; Newman, Jeffrey A; Pforr, Janine; Peth, Michael; Rafelski, Marc; Rodriguez-Monuz, Lucia; Salvato, Mara; Stefanon, Mauro; Wel, Arjen Van Der; Willner, Steven P; Wilklind, Tommy; Wuyts, Stijn
The Astrophysical journal. Supplement series, 07/2019, Volume: 243, Issue: 2Journal Article
We present a WFC3 F160W (H-band) selected catalog in the CANDELS/GOODS-N field containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts and stellar pa-rameters derived from the analysis of the multi-wavelength data. The catalog contains 35,445 sourcesover the 171 arcmin2of the CANDELS F160W mosaic. The 5σdetection limits (within an aperture ofradius 0.′′17) of the mosaic range betweenH= 27.8, 28.2 and 28.7 in the wide, intermediate and deepregions, that span approximately 50%, 15% and 35% of the total area. The multi-wavelength photom-etry includes broad-band data from UV (U band from KPNO and LBC), optical (HST/ACS F435W,F606W, F775W, F814W, and F850LP), near-to-mid IR (HST/WFC3 F105W, F125W, F140W andF160W, Subaru/MOIRCS Ks, CFHT/Megacam K, andSpitzer/IRAC 3.6, 4.5, 5.8, 8.0μm) and far IR(Spitzer/MIPS 24μm, HERSCHEL/PACS 100 and 160μm, SPIRE 250, 350 and 500μm) observations.In addition, the catalog also includes, optical medium-band data (R∼50) in 25 consecutive bands,λ= 500 to 950 nm, from the SHARDS survey and WFC3 IR spectroscopic observations with theG102 and G141 grisms (R∼210 and 130). The use of higher spectral resolution data to estimate pho-tometric redshifts provides very high, and nearly uniform, precision fromz= 0−2.5. The comparisonto 1,485 good quality spectroscopic redshifts up toz∼3 yields ∆z/(1+zspec)=0.0032 and an outlierfraction ofη=4.3%. In addition to the multi-band photometry, we release added-value catalogs withemission line fluxes, stellar masses, dust attenuations, UV- and IR-based star formation rates andrest-frame colors.
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