WFRF:(Perez Fournon I.)
Sökning: WFRF:(Perez Fournon I.) > (2020-2024) > z -GAL: A NOEMA spe...
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 06738naa a2200805 4500 | |
| 001 | oai:research.chalmers.se:c754730d-71cd-41d5-acf6-84679282bbc0 | |
| 003 | SwePub | |
| 008 | 231029s2023 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://research.chalmers.se/publication/5380552 URI |
| 024 | 7 | a https://doi.org/10.1051/0004-6361/2023468032 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 Berta, S.u Institut de Radioastronomie Millimétrique (IRAM)4 aut |
| 245 | 1 0 | a z -GAL: A NOEMA spectroscopic redshift survey of bright Herschel galaxies: III. Physical properties |
| 264 | 1 | c 2023 |
| 338 | a electronic2 rdacarrier | |
| 520 | a The z-GAL survey observed 137 bright Herschel-selected targets with the IRAM Northern Extended Millimeter Array, with the aim to measure their redshift and study their properties. Several of them have been resolved into multiple sources. Consequently, robust spectroscopic redshifts have been measured for 165 individual galaxies in the range 0.8., <., z., <., 6.5. In this paper we analyse the millimetre spectra of the z-GAL sources, using both their continuum and line emission to derive their physical properties. At least two spectral lines are detected for each source, including transitions of 12CO, [CI], and H2O. The observed 12CO line ratios and spectral line energy distributions of individual sources resemble those of local starbursts. In seven sources the para-H2O (211-202) transition is detected and follows the IR versus H2O luminosity relation of sub-millimetre galaxies. The molecular gas mass of the z-GAL sources is derived from their 12CO, [CI], and sub-millimetre dust continuum emission. The three tracers lead to consistent results, with the dust continuum showing the largest scatter when compared to 12CO. The gas-to-dust mass ratio of these sources was computed by combining the information derived from 12CO and the dust continuum and has a median value of 107, similar to star-forming galaxies of near-solar metallicity. The same combined analysis leads to depletion timescales in the range between 0.1 and 1.0 Gyr, which place the z-GAL sources between the main sequence' of star formation and the locus of starbursts. Finally, we derived a first estimate of stellar masses "modulo possible gravitational magnification "by inverting known gas scaling relations: the z-GAL sample is confirmed to be mostly composed by starbursts, whereas ∼25% of its members lie on the main sequence of star-forming galaxies (within ±0.5 dex). | |
| 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 |
| 653 | a Galaxies: high-redshift | |
| 653 | a Galaxies: ISM | |
| 653 | a Submillimeter: galaxies | |
| 653 | a Galaxies: star formation | |
| 653 | a Galaxies: statistics | |
| 653 | a Galaxies: starburst | |
| 700 | 1 | a Stanley, F.u Institut de Radioastronomie Millimétrique (IRAM)4 aut |
| 700 | 1 | a Ismail, D.u Laboratoire d'Astrophysique de Marseille4 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 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 |
| 700 | 1 | a Jin, S.u Danmarks Tekniske Universitet,Technical University of Denmark4 aut |
| 700 | 1 | a Dannerbauer, H.u Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna4 aut |
| 700 | 1 | a Bakx, Tom,d 1990u Chalmers tekniska högskola,Chalmers University of Technology,National Astronomical Observatory of Japan,Nagoya University4 aut0 (Swepub:cth)bakx |
| 700 | 1 | a Beelen, A.u Laboratoire d'Astrophysique de Marseille4 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 Nanni, A.u Istituto nazionale di astrofisica (INAF)4 aut |
| 700 | 1 | a Omont, A.A.u Institut d 'Astrophysique de Paris4 aut |
| 700 | 1 | a van der Werf, P.u Universiteit Leiden (UL),Leiden University (UL)4 aut |
| 700 | 1 | a Krips, M.u Institut de Radioastronomie Millimétrique (IRAM)4 aut |
| 700 | 1 | a Baker, A. J.u Rutgers University,University of the Western Cape4 aut |
| 700 | 1 | a Bendo, G. J.u University of Manchester4 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 Institut de Radioastronomie Millimétrique (IRAM)4 aut |
| 700 | 1 | a Chartab, N.u University of California at Irvine (UCI)4 aut |
| 700 | 1 | a Cooray, A.u University of California at Irvine (UCI)4 aut |
| 700 | 1 | a Dye, S.u University Of Nottingham4 aut |
| 700 | 1 | a Eales, S.u Cardiff University4 aut |
| 700 | 1 | a Gavazzi, R.u Institut d 'Astrophysique de Paris4 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 Ivison, R. J.u Dublin Institute for Advanced Studies,University of Edinburgh,Macquarie University,European Southern Observatory (ESO)4 aut |
| 700 | 1 | a Jones, B. M.u Universität zu Köln,University of Cologne4 aut |
| 700 | 1 | a Lehnert, M.u CRAL Le Centre de Recherche Astronomique de Lyon4 aut |
| 700 | 1 | a Marchetti, L.u Istituto di Radioastronomia,University of Cape Town4 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 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 Serjeant, S.u Open University4 aut |
| 700 | 1 | a Urquhart, S.u Open University4 aut |
| 700 | 1 | a Vlahakis, C.u National Radio Astronomy Observatory4 aut |
| 710 | 2 | a Institut de Radioastronomie Millimétrique (IRAM)b Laboratoire d'Astrophysique de Marseille4 org |
| 773 | 0 | t Astronomy and Astrophysicsg 678q 678x 0004-6361x 1432-0746 |
| 856 | 4 | u https://research.chalmers.se/publication/538055/file/538055_Fulltext.pdfx primaryx freey FULLTEXT |
| 856 | 4 8 | u https://research.chalmers.se/publication/538055 |
| 856 | 4 8 | u https://doi.org/10.1051/0004-6361/202346803 |
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