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1 |
Material Type: Article
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The multi-phase winds of Markarian 231: from the hot, nuclear, ultra-fast wind to the galaxy-scale, molecular outflowAstronomy and astrophysics (Berlin), 2015-11, Vol.583, p.A99 [Peer Reviewed Journal]ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201526020Full text available |
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2 |
Material Type: Article
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Triggering active galactic nuclei in hierarchical galaxy formation: disk instability vs. interactionsAstronomy and astrophysics (Berlin), 2014-09, Vol.569, p.1-20 [Peer Reviewed Journal]ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201424217Full text available |
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3 |
Material Type: Article
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High-redshift Galaxies from Early JWST Observations: Constraints on Dark Energy ModelsAstrophysical journal. Letters, 2022-10, Vol.938 (1), p.L5 [Peer Reviewed Journal]2022. The Author(s). Published by the American Astronomical Society. ;2022. The Author(s). Published by the American Astronomical Society. 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: 2041-8205 ;EISSN: 2041-8213 ;DOI: 10.3847/2041-8213/ac96e9Full text available |
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4 |
Material Type: Article
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Space Densities and Emissivities of Active Galactic Nuclei at z > 4The Astrophysical journal, 2019-10, Vol.884 (1), p.19 [Peer Reviewed Journal]2019. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Oct 10, 2019 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab39e1Full text available |
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5 |
Material Type: Article
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A STRINGENT LIMIT ON THE WARM DARK MATTER PARTICLE MASSES FROM THE ABUNDANCE OF z = 6 GALAXIES IN THE HUBBLE FRONTIER FIELDSAstrophysical journal. Letters, 2016-07, Vol.825 (1), p.L1-L1 [Peer Reviewed Journal]2016. The American Astronomical Society. All rights reserved. ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 2041-8205 ;EISSN: 2041-8213 ;DOI: 10.3847/2041-8205/825/1/L1Full text available |
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6 |
Material Type: Article
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Galaxy formation in warm dark matter cosmologyMonthly notices of the Royal Astronomical Society, 2012-04, Vol.421 (3), p.2384-2394 [Peer Reviewed Journal]2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS 2012 ;2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS ;ISSN: 0035-8711 ;EISSN: 1365-2966 ;DOI: 10.1111/j.1365-2966.2012.20470.xFull text available |
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7 |
Material Type: Article
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The physics and the structure of the quasar-driven outflow in Mrk 231Astronomy and astrophysics (Berlin), 2012-07, Vol.543, p.A99 [Peer Reviewed Journal]2015 INIST-CNRS ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201218793 ;CODEN: AAEJAFFull text available |
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8 |
Material Type: Article
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Outflows in the Disks of Active GalaxiesThe Astrophysical journal, 2019-06, Vol.877 (2), p.74 [Peer Reviewed Journal]2019. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jun 01, 2019 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab1a3aFull text available |
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9 |
Material Type: Article
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Galactic outflow driven by the active nucleus and the origin of the gamma-ray emission in NGC 1068Astronomy and astrophysics (Berlin), 2016-12, Vol.596, p.A68 [Peer Reviewed Journal]ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201628667Full text available |
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10 |
Material Type: Article
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CONSTRAINING THE WARM DARK MATTER PARTICLE MASS THROUGH ULTRA-DEEP UV LUMINOSITY FUNCTIONS AT z = 2The Astrophysical journal, 2016-02, Vol.818 (1), p.90 [Peer Reviewed Journal]2016. The American Astronomical Society. All rights reserved. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/0004-637X/818/1/90Full text available |
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11 |
Material Type: Article
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THE BLAST WAVE MODEL FOR AGN FEEDBACK : EFFECTS ON AGN OBSCURATIONThe Astrophysical journal, 2008-10, Vol.686 (1), p.219-229 [Peer Reviewed Journal]2008 INIST-CNRS ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1086/591438 ;CODEN: ASJOABFull text available |
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12 |
Material Type: Article
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On the discovery of fast molecular gas in the UFO/BAL quasar APM 08279+5255 at z = 3.912Astronomy and astrophysics (Berlin), 2017-12, Vol.608 [Peer Reviewed Journal]Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201731387Digital Resources/Online E-Resources |
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13 |
Material Type: Article
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Star formation and mass assembly in high redshift galaxiesAstronomy and astrophysics (Berlin), 2009-09, Vol.504 (3), p.751-767 [Peer Reviewed Journal]2009 INIST-CNRS ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/200811434 ;CODEN: AAEJAFFull text available |
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14 |
Material Type: Article
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Fundamental Physics with the Hubble Frontier Fields: Constraining Dark Matter Models with the Abundance of Extremely Faint and Distant GalaxiesThe Astrophysical journal, 2017-02, Vol.836 (1), p.61 [Peer Reviewed Journal]2017. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Feb 10, 2017 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/836/1/61Full text available |
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15 |
Material Type: Article
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SUPER: II. Spatially resolved ionised gas kinematics and scaling relations in z ∼ 2 AGN host galaxiesAstronomy and astrophysics (Berlin), 2020-10 [Peer Reviewed Journal]info:eu-repo/semantics/openAccess ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/202038551Digital Resources/Online E-Resources |
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16 |
Material Type: Article
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Testing the Fidelity of Simulations of Black Hole-Galaxy Coevolution at z ∼ 1.5 with ObservationsThe Astrophysical journal, 2020-06, Vol.896 (2), p.159 [Peer Reviewed Journal]2020. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jun 01, 2020 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab91beFull text available |
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17 |
Material Type: Article
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Galaxy Formation in Sterile Neutrino Dark Matter ModelsThe Astrophysical journal, 2018-02, Vol.854 (1), p.1 [Peer Reviewed Journal]2018. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Feb 10, 2018 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aaa773Full text available |
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18 |
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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19 |
Material Type: Article
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The interaction-driven starburst contribution to the cosmic star formation rate densityAstronomy and astrophysics (Berlin), 2013-04, Vol.552, p.np-np [Peer Reviewed Journal]ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201220754Full text available |
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20 |
Material Type: Article
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Relative growth of black holes and the stellar components of galaxiesAstronomy and astrophysics (Berlin), 2016-10, Vol.594, p.A99 [Peer Reviewed Journal]ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201628415Full text available |