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Material Type: Article
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De re metallica: the cosmic chemical evolution of galaxiesThe Astronomy and astrophysics review, 2019-12, Vol.27 (1), p.1-187, Article 3 [Peer Reviewed Journal]The Author(s) 2019 ;The Astronomy and Astrophysics Review is a copyright of Springer, (2019). All Rights Reserved. © 2019. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0935-4956 ;EISSN: 1432-0754 ;DOI: 10.1007/s00159-018-0112-2Full text available |
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Strangulation as the primary mechanism for shutting down star formation in galaxiesNature (London), 2015-05, Vol.521 (7551), p.192-195 [Peer Reviewed Journal]ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/nature14439 ;PMID: 25971510Full text available |
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Gas accretion as the origin of chemical abundance gradients in distant galaxiesNature (London), 2010-10, Vol.467 (7317), p.811-813 [Peer Reviewed Journal]2015 INIST-CNRS ;Copyright Nature Publishing Group Oct 14, 2010 ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/nature09451 ;PMID: 20944741 ;CODEN: NATUASFull text available |
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Star formation inside a galactic outflowNature (London), 2017-04, Vol.544 (7649), p.202-206 [Peer Reviewed Journal]COPYRIGHT 2017 Nature Publishing Group ;COPYRIGHT 2017 Nature Publishing Group ;Copyright Nature Publishing Group Apr 13, 2017 ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/nature21677 ;PMID: 28346938 ;CODEN: NATUASFull text available |
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Suppression of black-hole growth by strong outflows at redshifts 5.8-6.6Nature (London), 2022-05, Vol.605 (7909), p.244-247 [Peer Reviewed Journal]2022. The Author(s), under exclusive licence to Springer Nature Limited. ;Copyright Nature Publishing Group May 12, 2022 ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/s41586-022-04608-1 ;PMID: 35546195Full text available |
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Material Type: Article
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Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913Nature communications, 2022-08, Vol.13 (1), p.4574-4574, Article 4574 [Peer Reviewed Journal]The Author(s) 2022. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;Attribution ;The Author(s) 2022 ;ISSN: 2041-1723 ;EISSN: 2041-1723 ;DOI: 10.1038/s41467-022-32297-x ;PMID: 35931777Full text available |
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Identification and properties of intense star-forming galaxies at redshifts z > 10Nature astronomy, 2023-05, Vol.7 (5), p.611-621 [Peer Reviewed Journal]The Author(s), under exclusive licence to Springer Nature Limited 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 2397-3366 ;EISSN: 2397-3366 ;DOI: 10.1038/s41550-023-01921-1Full text available |
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Material Type: Article
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The REACH radiometer for detecting the 21-cm hydrogen signal from redshift z ≈ 7.5–28Nature astronomy, 2022-08, Vol.6 (8), p.984-998 [Peer Reviewed Journal]The Author(s), under exclusive licence to Springer Nature Limited 2022. corrected publication 2022. Springer Nature or its licensor holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. ;ISSN: 2397-3366 ;EISSN: 2397-3366 ;DOI: 10.1038/s41550-022-01709-9Full text available |
9 |
Material Type: Article
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A supernova origin for dust in a high-redshift quasarNature, 2004-09, Vol.431 (7008), p.533-535 [Peer Reviewed Journal]COPYRIGHT 2004 Nature Publishing Group ;COPYRIGHT 2004 Nature Publishing Group ;Copyright Macmillan Journals Ltd. Sep 30, 2004 ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/nature02930 ;PMID: 15457250 ;CODEN: NATUASFull text available |
10 |
Material Type: Article
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The Metallicity Evolution of Galaxies through the Cosmic EpochsProceedings of the International Astronomical Union, 2010-12, Vol.6 (S277), p.170-173 [Peer Reviewed Journal]Copyright © International Astronomical Union 2011 ;ISSN: 1743-9213 ;EISSN: 1743-9221 ;DOI: 10.1017/S1743921311022708Full text available |
11 |
Material Type: Article
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Comparison of star formation rates from Hα and infrared luminosity as seen by HerschelMonthly notices of the Royal Astronomical Society, 2012-10, Vol.426 (1), p.330-341 [Peer Reviewed Journal]2012 The Authors 2012 ;2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS ;ISSN: 0035-8711 ;EISSN: 1365-2966 ;DOI: 10.1111/j.1365-2966.2012.21710.xFull text available |
12 |
Material Type: Article
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Author Correction: The REACH radiometer for detecting the 21-cm hydrogen signal from redshift z ≈ 7.5–28Nature astronomy, 2022-11, Vol.6 (11), p.1332-1332 [Peer Reviewed Journal]The Author(s), under exclusive licence to Springer Nature Limited 2022. corrected publication 2022. ;ISSN: 2397-3366 ;EISSN: 2397-3366 ;DOI: 10.1038/s41550-022-01817-6Full text available |
13 |
Material Type: Article
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Ionized gas outflows and global kinematics of low-z luminous star-forming galaxiesProceedings of the International Astronomical Union, 2014-07, Vol.10 (S309), p.73-76 [Peer Reviewed Journal]Copyright © International Astronomical Union 2015 ;ISSN: 1743-9213 ;EISSN: 1743-9221 ;DOI: 10.1017/S174392131400934XFull text available |
14 |
Material Type: Article
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LSD and AMAZE: the mass-metallicity relation at z > 3Proceedings of the International Astronomical Union, 2008-06, Vol.4 (S255), p.106-110 [Peer Reviewed Journal]Copyright © International Astronomical Union 2008 ;ISSN: 1743-9213 ;EISSN: 1743-9221 ;DOI: 10.1017/S1743921308024654Full text available |
15 |
Material Type: Article
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Gas and dust in the most distant quasarsProceedings of the International Astronomical Union, 2004-03, Vol.2004 (IAUS222), p.229-234 [Peer Reviewed Journal]2004 International Astronomical Union ;ISSN: 1743-9213 ;EISSN: 1743-9221 ;DOI: 10.1017/S1743921304002169Full text available |
16 |
Material Type: Article
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Metallicity Evolution of AGNsProceedings of the International Astronomical Union, 2009-08, Vol.5 (S267), p.73-79 [Peer Reviewed Journal]Copyright © International Astronomical Union 2010 ;ISSN: 1743-9213 ;EISSN: 1743-9221 ;DOI: 10.1017/S1743921310005594Full text available |
17 |
Material Type: Article
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Metallicity of the high-redshift Universe traced by radio galaxiesProceedings of the International Astronomical Union, 2009-08, Vol.5 (S265), p.179-180 [Peer Reviewed Journal]Copyright © International Astronomical Union 2010 ;ISSN: 1743-9213 ;EISSN: 1743-9221 ;DOI: 10.1017/S1743921310000499Full text available |
18 |
Material Type: Article
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Large Grains in our and External GalaxiesAstrophysics and space science, 2002-07, Vol.281 (1-2), p.233-242 [Peer Reviewed Journal]Kluwer Academic Publishers 2002 ;ISSN: 0004-640X ;EISSN: 1572-946X ;DOI: 10.1023/A:1019506703088Full text available |
19 |
Material Type: Article
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Strangulation as the primarymechanismfor shutting down star formation in galaxiesNature (London), 2015-05, Vol.521 (7551), p.192 [Peer Reviewed Journal]Copyright Nature Publishing Group May 14, 2015 ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;CODEN: NATUASFull text available |
20 |
Material Type: Article
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The importance of following the evolution of the dust in galaxies on their SEDsProceedings of the International Astronomical Union, 2008-06, Vol.4 (S255), p.147-151 [Peer Reviewed Journal]Copyright © International Astronomical Union 2008 ;ISSN: 1743-9213 ;EISSN: 1743-9221 ;DOI: 10.1017/S1743921308024721Full text available |