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Sökning: WFRF:(Bakx Tom J. L. C.) > The bright extragal...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00007583naa a2200973 4500
001oai:research.chalmers.se:4fe142f3-b500-425b-bd33-cbf6ede7136c
003SwePub
008230707s2023 | |||||||||||000 ||eng|
024a https://research.chalmers.se/publication/5365082 URI
024a https://doi.org/10.1093/mnras/stac37712 DOI
040 a (SwePub)cth
041 a engb eng
042 9 SwePub
072 7a art2 swepub-publicationtype
072 7a ref2 swepub-contenttype
100a Bendo, G. J.u University of Manchester4 aut
2451 0a The bright extragalactic ALMA redshift survey (BEARS) – II. Millimetre photometry of gravitational lens candidates
264 1c 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 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
650 7a TEKNIK OCH TEKNOLOGIERx Elektroteknik och elektronikx Annan elektroteknik och elektronik0 (SwePub)202992 hsv//swe
650 7a 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
700a Urquhart, S.u Open University4 aut
700a Serjeant, S.u Open University4 aut
700a Bakx, Tom J.L.C.u National Astronomical Observatory of Japan,Nagoya University4 aut
700a Hagimoto, Masatou Nagoya University4 aut
700a Cox, P.u Institut d 'Astrophysique de Paris4 aut
700a Neri, R.u Institut de Radioastronomie Millimétrique (IRAM)4 aut
700a Lehnert, M.u École Normale Supérieure de Lyon4 aut
700a Dannerbauer, H.u Universidad de la Laguna,University of La Laguna,Instituto de Astrofísica de Canarias4 aut
700a Amvrosiadis, A.u Durham University4 aut
700a Andreani, P.u European Southern Observatory (ESO)4 aut
700a Baker, A. J.u Rutgers University,University of the Western Cape4 aut
700a Beelen, A.u Laboratoire d'Astrophysique de Marseille4 aut
700a Berta, S.u Institut de Radioastronomie Millimétrique (IRAM)4 aut
700a Borsato, E.u Università Degli Studi di Padova,University of Padua4 aut
700a Buat, V.u Laboratoire d'Astrophysique de Marseille4 aut
700a Butler, K. M.u Universiteit Leiden (UL),Leiden University (UL)4 aut
700a Cooray, A.u University of California at Irvine (UCI)4 aut
700a De Zotti, G.u Istituto nazionale di astrofisica (INAF)4 aut
700a Dunne, L.u Cardiff University4 aut
700a Dye, S.u University Of Nottingham4 aut
700a Eales, S.u Cardiff University4 aut
700a Enia, A. F.M.u Istituto nazionale di astrofisica (INAF),Universita di Bologna,University of Bologna4 aut
700a Fan, Lulu,d 1982u University of Science and Technology of China4 aut0 (Swepub:cth)flulu
700a Gavazzi, R.u Laboratoire d'Astrophysique de Marseille,Institut d 'Astrophysique de Paris4 aut
700a González-Nuevo, J.u Universidad de Oviedo,University of Oviedo4 aut
700a Harris, A. I.u University of Maryland4 aut
700a Herrera, C. N.u Institut de Radioastronomie Millimétrique (IRAM)4 aut
700a Hughes, D.u Instituto Nacional de Astrofísica, Óptica y Electrońica (INAOE),National Institute of Astrophysics, Optics and Electronics (INAOE)4 aut
700a Ismail, D.u Laboratoire d'Astrophysique de Marseille4 aut
700a Jones, B. M.u Universität zu Köln,University of Cologne4 aut
700a Kohno, K.u University of Tokyo, Japan4 aut
700a Krips, M.u Institut de Radioastronomie Millimétrique (IRAM)4 aut
700a Lagache, Guilaineu Laboratoire d'Astrophysique de Marseille4 aut
700a Marchetti, L.u Istituto nazionale di astrofisica (INAF),University of Cape Town4 aut
700a Massardi, M.u Istituto nazionale di astrofisica (INAF),Scuola Internazionale Superiore di Studi Avanzati4 aut
700a Messias, H.u Atacama Large Millimeter-submillimeter Array (ALMA),European Southern Observatory Santiago4 aut
700a Negrello, M.u Cardiff University4 aut
700a Omont, A.A.u Institut d 'Astrophysique de Paris4 aut
700a Perez-Fournon, I.u Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna4 aut
700a Riechers, D. A.u Universität zu Köln,University of Cologne4 aut
700a Scott, D.u University of British Columbia (UBC)4 aut
700a Smith, M. W.L.u Cardiff University4 aut
700a Stanley, F.u Institut de Radioastronomie Millimétrique (IRAM)4 aut
700a Tamura, Y.u Nagoya University4 aut
700a Temi, P.u NASA Ames Research Center4 aut
700a van der Werf, P.u Universiteit Leiden (UL),Leiden University (UL)4 aut
700a Verma, A.u University Of Oxford4 aut
700a Vlahakis, C.u National Radio Astronomy Observatory4 aut
700a Weiss, A.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut
700a Yang, Chentao,d 1988u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)chentao
700a Young, A. J.u Rutgers University4 aut
710a University of Manchesterb Open University4 org
773t Monthly Notices of the Royal Astronomical Societyg 522:2, s. 2995-3017q 522:2<2995-3017x 0035-8711x 1365-2966
856u https://research.chalmers.se/publication/536508/file/536508_Fulltext.pdfx primaryx freey FULLTEXT
8564 8u https://research.chalmers.se/publication/536508
8564 8u https://doi.org/10.1093/mnras/stac3771

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