Sökning: WFRF:(Bakx Tom J. L. C.) > The bright extragal...
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000 | 07583naa a2200973 4500 | |
001 | oai:research.chalmers.se:4fe142f3-b500-425b-bd33-cbf6ede7136c | |
003 | SwePub | |
008 | 230707s2023 | |||||||||||000 ||eng| | |
024 | 7 | a https://research.chalmers.se/publication/5365082 URI |
024 | 7 | a https://doi.org/10.1093/mnras/stac37712 DOI |
040 | a (SwePub)cth | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a art2 swepub-publicationtype |
072 | 7 | a ref2 swepub-contenttype |
100 | 1 | a Bendo, G. J.u University of Manchester4 aut |
245 | 1 0 | a The bright extragalactic ALMA redshift survey (BEARS) – II. Millimetre photometry of gravitational lens candidates |
264 | 1 | c 2023 |
338 | a electronic2 rdacarrier | |
520 | a We present 101- and 151-GHz ALMA continuum images for 85 fields selected from Herschel observations that have 500-μm flux densities >80 mJy and 250–500-μm colours consistent with z > 2, most of which are expected to be gravitationally lensed or hyperluminous infrared galaxies. Approximately half of the Herschel 500-μm sources were resolved into multiple ALMA sources, but 11 of the 15 brightest 500-μm Herschel sources correspond to individual ALMA sources. For the 37 fields containing either a single source with a spectroscopic redshift or two sources with the same spectroscopic redshift, we examined the colour temperatures and dust emissivity indices. The colour temperatures only vary weakly with redshift and are statistically consistent with no redshift-dependent temperature variations, which generally corresponds to results from other samples selected in far-infrared, submillimetre, or millimetre bands but not to results from samples selected in optical or near-infrared bands. The dust emissivity indices, with very few exceptions, are largely consistent with a value of 2. We also compared spectroscopic redshifts to photometric redshifts based on spectral energy distribution templates designed for infrared-bright high-redshift galaxies. While the templates systematically underestimate the redshifts by ∼15 per cent, the inclusion of ALMA data decreases the scatter in the predicted redshifts by a factor of ∼2, illustrating the potential usefulness of these millimetre data for estimating photometric redshifts. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
650 | 7 | a TEKNIK OCH TEKNOLOGIERx Elektroteknik och elektronikx Annan elektroteknik och elektronik0 (SwePub)202992 hsv//swe |
650 | 7 | a ENGINEERING AND TECHNOLOGYx Electrical Engineering, Electronic Engineering, Information Engineeringx Other Electrical Engineering, Electronic Engineering, Information Engineering0 (SwePub)202992 hsv//eng |
653 | a submillimetre: galaxies | |
653 | a galaxies: ISM | |
653 | a galaxies: high-redshift | |
653 | a infrared: galaxies | |
700 | 1 | a Urquhart, S.u Open University4 aut |
700 | 1 | a Serjeant, S.u Open University4 aut |
700 | 1 | a Bakx, Tom J.L.C.u National Astronomical Observatory of Japan,Nagoya University4 aut |
700 | 1 | a Hagimoto, Masatou Nagoya University4 aut |
700 | 1 | a Cox, P.u Institut d 'Astrophysique de Paris4 aut |
700 | 1 | a Neri, R.u Institut de Radioastronomie Millimétrique (IRAM)4 aut |
700 | 1 | a Lehnert, M.u École Normale Supérieure de Lyon4 aut |
700 | 1 | a Dannerbauer, H.u Universidad de la Laguna,University of La Laguna,Instituto de Astrofísica de Canarias4 aut |
700 | 1 | a Amvrosiadis, A.u Durham University4 aut |
700 | 1 | a Andreani, P.u European Southern Observatory (ESO)4 aut |
700 | 1 | a Baker, A. J.u Rutgers University,University of the Western Cape4 aut |
700 | 1 | a Beelen, A.u Laboratoire d'Astrophysique de Marseille4 aut |
700 | 1 | a Berta, S.u Institut de Radioastronomie Millimétrique (IRAM)4 aut |
700 | 1 | a Borsato, E.u Università Degli Studi di Padova,University of Padua4 aut |
700 | 1 | a Buat, V.u Laboratoire d'Astrophysique de Marseille4 aut |
700 | 1 | a Butler, K. M.u Universiteit Leiden (UL),Leiden University (UL)4 aut |
700 | 1 | a Cooray, A.u University of California at Irvine (UCI)4 aut |
700 | 1 | a De Zotti, G.u Istituto nazionale di astrofisica (INAF)4 aut |
700 | 1 | a Dunne, L.u Cardiff University4 aut |
700 | 1 | a Dye, S.u University Of Nottingham4 aut |
700 | 1 | a Eales, S.u Cardiff University4 aut |
700 | 1 | a Enia, A. F.M.u Istituto nazionale di astrofisica (INAF),Universita di Bologna,University of Bologna4 aut |
700 | 1 | a Fan, Lulu,d 1982u University of Science and Technology of China4 aut0 (Swepub:cth)flulu |
700 | 1 | a Gavazzi, R.u Laboratoire d'Astrophysique de Marseille,Institut d 'Astrophysique de Paris4 aut |
700 | 1 | a González-Nuevo, J.u Universidad de Oviedo,University of Oviedo4 aut |
700 | 1 | a Harris, A. I.u University of Maryland4 aut |
700 | 1 | a Herrera, C. N.u Institut de Radioastronomie Millimétrique (IRAM)4 aut |
700 | 1 | a Hughes, D.u Instituto Nacional de Astrofísica, Óptica y Electrońica (INAOE),National Institute of Astrophysics, Optics and Electronics (INAOE)4 aut |
700 | 1 | a Ismail, D.u Laboratoire d'Astrophysique de Marseille4 aut |
700 | 1 | a Jones, B. M.u Universität zu Köln,University of Cologne4 aut |
700 | 1 | a Kohno, K.u University of Tokyo, Japan4 aut |
700 | 1 | a Krips, M.u Institut de Radioastronomie Millimétrique (IRAM)4 aut |
700 | 1 | a Lagache, Guilaineu Laboratoire d'Astrophysique de Marseille4 aut |
700 | 1 | a Marchetti, L.u Istituto nazionale di astrofisica (INAF),University of Cape Town4 aut |
700 | 1 | a Massardi, M.u Istituto nazionale di astrofisica (INAF),Scuola Internazionale Superiore di Studi Avanzati4 aut |
700 | 1 | a Messias, H.u Atacama Large Millimeter-submillimeter Array (ALMA),European Southern Observatory Santiago4 aut |
700 | 1 | a Negrello, M.u Cardiff University4 aut |
700 | 1 | a Omont, A.A.u Institut d 'Astrophysique de Paris4 aut |
700 | 1 | a Perez-Fournon, I.u Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna4 aut |
700 | 1 | a Riechers, D. A.u Universität zu Köln,University of Cologne4 aut |
700 | 1 | a Scott, D.u University of British Columbia (UBC)4 aut |
700 | 1 | a Smith, M. W.L.u Cardiff University4 aut |
700 | 1 | a Stanley, F.u Institut de Radioastronomie Millimétrique (IRAM)4 aut |
700 | 1 | a Tamura, Y.u Nagoya University4 aut |
700 | 1 | a Temi, P.u NASA Ames Research Center4 aut |
700 | 1 | a van der Werf, P.u Universiteit Leiden (UL),Leiden University (UL)4 aut |
700 | 1 | a Verma, A.u University Of Oxford4 aut |
700 | 1 | a Vlahakis, C.u National Radio Astronomy Observatory4 aut |
700 | 1 | a Weiss, A.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
700 | 1 | a Yang, Chentao,d 1988u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)chentao |
700 | 1 | a Young, A. J.u Rutgers University4 aut |
710 | 2 | a University of Manchesterb Open University4 org |
773 | 0 | t Monthly Notices of the Royal Astronomical Societyg 522:2, s. 2995-3017q 522:2<2995-3017x 0035-8711x 1365-2966 |
856 | 4 | u https://research.chalmers.se/publication/536508/file/536508_Fulltext.pdfx primaryx freey FULLTEXT |
856 | 4 8 | u https://research.chalmers.se/publication/536508 |
856 | 4 8 | u https://doi.org/10.1093/mnras/stac3771 |
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