GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies
| Autor: | Neil M. Nagar, M. Franco, Maurilio Pannella, C. Gómez-Guijarro, Laure Ciesla, E. Daddi, Casey Papovich, Stéphanie Juneau, Koryo Okumura, Henry C. Ferguson, Matthieu Béthermin, David Elbaz, Lihwai Lin, Mark Dickinson, Frédéric Bournaud, Mauro Giavalisco, Tao Wang, John D. Silverman, Steven L. Finkelstein, Hanae Inami, L. Zhou, Xinwen Shu, R. T. Coogan, Benjamin Magnelli, Kentaro Motohara, Daisuke Iono, Guilaine Lagache, Georgios E. Magdis, Wiphu Rujopakarn, Alexandra Pope, Corentin Schreiber, Mengyuan Xiao, David M. Alexander, Ricardo Demarco, James Mullaney, Ranga-Ram Chary |
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| Přispěvatelé: | Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), University of Hertfordshire [Hatfield] (UH), Nanjing University (NJU), Argelander Institute for Astronomy (AlfA), Rheinische Friedrich-Wilhelms-Universität Bonn, University of Oxford, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), National Optical Astronomy Observatory (NOAO), Universidad de Conception, Niels Bohr Institute [Copenhagen] (NBI), Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH), National Observatory of Athens (NOA), Durham University, University of Sheffield [Sheffield], Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Hiroshima University, Anhui Normal University, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Infrared Processing and Analysis Center (IPAC), California Institute of Technology (CALTECH), Max Planck Institute for Extraterrestrial Physics (MPE), Max-Planck-Gesellschaft, Space Telescope Science Institute (STSci), University of Texas at Austin [Austin], University of Massachusetts [Amherst] (UMass Amherst), University of Massachusetts System (UMASS), National Astronomical Observatory of Japan (NAOJ), Graduate University for Advanced Studies [Hayama] (SOKENDAI), Università degli studi di Trieste = University of Trieste, Ludwig-Maximilians-Universität München (LMU), Kavli Institute for the Physics and Mathematics of the Universe [Tokyo] (Kavli IPMU), The University of Tokyo Institutes for Advanced Study (UTIAS), The University of Tokyo (UTokyo)-The University of Tokyo (UTokyo), Chulalongkorn University [Bangkok], National Astronomical Research Institute of Thailand (NARIT), This work was supported by the Programme National Cosmology et Galaxies (PNCG) of CNRS/INSU with INP and IN2P3, co-funded by CEA and CNES., European Project: 648179,H2020,ERC-2014-CoG,ConTExt(2015), European Project: 716762,ClustersXCosmo, Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), University of Oxford [Oxford], University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU), École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), University of Trieste |
| Jazyk: | angličtina |
| Rok vydání: | 2020 |
| Předmět: |
submillimeter: galaxies
SPECTROSCOPIC SURVEY TELESCOPE IMAGER SCUBA FOS: Physical sciences CAMERA Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics star formation [Galaxies] 01 natural sciences high-redshift [Galaxies] galaxies [Submillimeter] galaxies: high-redshift 0103 physical sciences STAR-FORMING GALAXIES Astrophysics::Solar and Stellar Astrophysics FIELD 010303 astronomy & astrophysics License Astrophysics::Galaxy Astrophysics Physics 010308 nuclear & particles physics photometry [Galaxies] Astronomy and Astrophysics galaxies: fundamental parameters Creative commons evolution [Galaxies] Astrophysics - Astrophysics of Galaxies Galaxy SPITZER galaxies: photometry ORIGINS DEEP SURVEY STELLAR Space and Planetary Science Astrophysics of Galaxies (astro-ph.GA) galaxies: star formation fundamental parameters [Galaxies] Millimeter Astrophysics::Earth and Planetary Astrophysics galaxies: evolution [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
| Zdroj: | Astronomy and Astrophysics-A&A Astronomy and Astrophysics-A&A, 2020, 643, pp.A53. ⟨10.1051/0004-6361/202038310⟩ Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643, pp.A53. ⟨10.1051/0004-6361/202038310⟩ Astronomy & Astrophysics Franco, M, Elbaz, D, Zhou, L, Magnelli, B, Schreiber, C, Ciesla, L, Dickinson, M, Nagar, N, Magdis, G, Alexander, D M, Béthermin, M, Demarco, R, Daddi, E, Wang, T, Mullaney, J, Inami, H, Shu, X, Bournaud, F, Chary, R, Coogan, R T, Ferguson, H, Finkelstein, S L, Giavalisco, M, Gómez-Guijarro, C, Iono, D, Juneau, S, Lagache, G, Lin, L, Motohara, K, Okumura, K, Pannella, M, Papovich, C, Pope, A, Rujopakarn, W, Silverman, J & Xiao, M 2020, ' GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies ', Astronomy and Astrophysics, vol. 643, A53 . https://doi.org/10.1051/0004-6361/202038310 Franco, M, Elbaz, D, Zhou, L, Magnelli, B, Schreiber, C, Ciesla, L, Dickinson, M, Nagar, N, Magdis, G, Alexander, D M, Bethermin, M, Demarco, R, Daddi, E, Wang, T, Mullaney, J, Inami, H, Shu, X, Bournaud, F, Chary, R, Coogan, R T, Ferguson, H, Finkelstein, S L, Giavalisco, M, Gomez-Guijarro, C, Iono, D, Juneau, S, Lagache, G, Lin, L, Motohara, K, Okumura, K, Pannella, M, Papovich, C, Pope, A, Rujopakarn, W, Silverman, J & Xiao, M 2020, ' GOODS-ALMA : Using IRAC and VLA to probe fainter millimeter galaxies ', Astronomy & Astrophysics, vol. 643, A53 . https://doi.org/10.1051/0004-6361/202038310 Astronomy & astrophysics, 2020, Vol.643, pp.A53 [Peer Reviewed Journal] |
| ISSN: | 0004-6361 |
| DOI: | 10.1051/0004-6361/202038310⟩ |
| Popis: | In this paper, we extend the source detection in the GOODS-ALMA field (69 arcmin$^2$, rms sensitivity $\sigma$ $\simeq$ 0.18 mJy.beam$^{-1}$), to deeper levels than presented in Franco et al. (2018). Using positional information at 3.6 and 4.5 $\mu$m (from Spitzer-IRAC), we explore the presence of galaxies detected at 1.1 mm with ALMA below our original blind detection limit of 4.8-$\sigma$ at which the number of spurious sources starts to dominate over that of real sources. In this Supplementary Catalog, we find a total of 16 galaxies, including 2 galaxies with no counterpart in HST images (also known as optically-dark galaxies) down to a 5$\sigma$ limiting depth of H = 28.2 AB (HST/WFC3 F160W). This brings the total sample of GOODS-ALMA 1.1 mm sources to 35 galaxies. Galaxies in the new sample cover a wider dynamic range in redshift ($z$ = 0.65 - 4.73), are on average twice as large (1.3 vs 0.65 kpc) and and have lower stellar mass (M$_{\star}^{\rm SC}$ = 7.6$\times$10$^{10}$M$_\odot$ vs M$_{\star}^{\rm MC}$ = 1.2$\times$10$^{11}$M$_\odot$). Although exhibiting larger physical sizes, these galaxies have still far-infrared sizes significantly more compact than inferred from their optical emission. We show that the astrometry of the HST image does not only suffer from a global astrometric shift, as already discussed in previous papers, but also from local shifts. These distortions were artificially introduced in the process of building the mosaic of the GOODS-South HST image. By comparing the positions of almost 400 galaxies detected by HST, Pan-STARRS and ALMA, we create a distortion map which can be used to correct for these astrometric issues. Comment: 18 pages, 13 figures. Accepted for publication in A&A |
| Databáze: | OpenAIRE |
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