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Material Type: Article
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The Large Early Galaxy Astrophysics Census (LEGA-C) Data Release 3: 3000 High-quality Spectra of K s -selected Galaxies at z > 0.6The Astrophysical journal. Supplement series, 2021-10, Vol.256 (2), p.44 [Peer Reviewed Journal]2021. The American Astronomical Society. All rights reserved. ;ISSN: 0067-0049 ;EISSN: 1538-4365 ;DOI: 10.3847/1538-4365/ac1356Full text available |
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Material Type: Article
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Stellar Population Inference with ProspectorThe Astrophysical journal. Supplement series, 2021-06, Vol.254 (2), p.22 [Peer Reviewed Journal]2021. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jun 2021 ;ISSN: 0067-0049 ;EISSN: 1538-4365 ;DOI: 10.3847/1538-4365/abef67Full text available |
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3 |
Material Type: Article
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A repeating fast radio burst source in a globular clusterNature (London), 2022-02, Vol.602 (7898), p.585-589 [Peer Reviewed Journal]2022. The Author(s), under exclusive licence to Springer Nature Limited. ;Copyright Nature Publishing Group Feb 24, 2022 ;ISSN: 0028-0836 ;ISSN: 1476-4687 ;EISSN: 1476-4687 ;DOI: 10.1038/s41586-021-04354-w ;PMID: 35197615Full text available |
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Material Type: Article
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Rapid Stellar and Binary Population Synthesis with COMPASThe Astrophysical journal. Supplement series, 2022-02, Vol.258 (2), p.34 [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: 0067-0049 ;EISSN: 1538-4365 ;DOI: 10.3847/1538-4365/ac416cFull text available |
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Material Type: Article
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The Occurrence of Rocky Habitable-zone Planets around Solar-like Stars from Kepler DataThe Astronomical journal, 2021-01, Vol.161 (1), p.36 [Peer Reviewed Journal]Copyright IOP Publishing Jan 2021 ;ISSN: 0004-6256 ;EISSN: 1538-3881 ;DOI: 10.3847/1538-3881/abc418Full text available |
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Material Type: Article
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The TESS Input Catalog and Candidate Target ListThe Astronomical journal, 2018-09, Vol.156 (3), p.102 [Peer Reviewed Journal]2018. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Sep 2018 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6256 ;EISSN: 1538-3881 ;DOI: 10.3847/1538-3881/aad050Full text available |
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7 |
Material Type: Article
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Analysis of the Spatially Resolved V−3.6 m Colors and Dust Extinction in 257 Nearby NGC and IC GalaxiesThe Astrophysical journal, 2019-10, Vol.884 (1) [Peer Reviewed Journal]2019. The American Astronomical Society. All rights reserved. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab385cFull text available |
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Material Type: Article
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The Chemical Composition of Extreme-velocity Stars This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile. † † This paper includes data gathered with the 3.5 m Telescope at Apache Point ObservatoryThe Astronomical journal, 2022-05, Vol.163 (6) [Peer Reviewed Journal]2022. The Author(s). Published by the American Astronomical Society. ;ISSN: 0004-6256 ;EISSN: 1538-3881 ;DOI: 10.3847/1538-3881/ac62d9Full text available |
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9 |
Material Type: Article
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COSMIC Variance in Binary Population SynthesisThe Astrophysical journal, 2020-07, Vol.898 (1), p.71 [Peer Reviewed Journal]2020. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jul 01, 2020 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab9d85Full text available |
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10 |
Material Type: Article
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Hubble Space Telescope Observations of NGC 253 Dwarf Satellites: Three Ultra-faint Dwarf Galaxies This paper includes data gathered with the 6.5 m Magellan Telescope at Las Campanas Observatory, ChileThe Astrophysical journal, 2022-02, Vol.926 (1) [Peer Reviewed Journal]2022. The Author(s). Published by the American Astronomical Society. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac4418Full text available |
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11 |
Material Type: Article
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On the Stellar Populations of Galaxies at z = 9–11: The Growth of Metals and Stellar Mass at Early TimesThe Astrophysical journal, 2022-03, Vol.927 (2), p.170 [Peer Reviewed Journal]2022. The Author(s). Published by the American Astronomical Society. ;Copyright Determination: MAY_INCLUDE_COPYRIGHT_MATERIAL ;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: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac4cadFull text available |
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12 |
Material Type: Article
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The CALIFA survey across the Hubble sequence: Spatially resolved stellar population properties in galaxiesAstronomy and astrophysics (Berlin), 2015-09, Vol.581, p.1-44 [Peer Reviewed Journal]ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201525938Full text available |
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13 |
Material Type: Article
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Nearby supernova host galaxies from the CALIFA Survey: I. Sample, data analysis, and correlation to star-forming regionsAstronomy and astrophysics (Berlin), 2014-12, Vol.572, p.1-24 [Peer Reviewed Journal]ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201424717Full text available |
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14 |
Material Type: Article
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One Large Blob and Many Streams Frosting the nearby Stellar Halo in Gaia DR2Astrophysical journal. Letters, 2018-06, Vol.860 (1), p.L11 [Peer Reviewed Journal]2018. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jun 10, 2018 ;ISSN: 2041-8205 ;EISSN: 2041-8213 ;DOI: 10.3847/2041-8213/aac882Full text available |
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15 |
Material Type: Article
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THE EFFECTS OF STELLAR ROTATION. II. A COMPREHENSIVE SET OF STARBURST99 MODELSThe Astrophysical journal. Supplement series, 2014-05, Vol.212 (1), p.1-18 [Peer Reviewed Journal]ISSN: 0067-0049 ;EISSN: 1538-4365 ;DOI: 10.1088/0067-0049/212/1/14Full text available |
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16 |
Material Type: Article
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A dominant population of optically invisible massive galaxies in the early UniverseNature (London), 2019-08, Vol.572 (7768), p.211-214 [Peer Reviewed Journal]COPYRIGHT 2019 Nature Publishing Group ;Copyright Nature Publishing Group Aug 8, 2019 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/s41586-019-1452-4 ;PMID: 31391562Full text available |
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17 |
Material Type: Article
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How to Measure Galaxy Star Formation Histories. I. Parametric ModelsThe Astrophysical journal, 2019-03, Vol.873 (1), p.44 [Peer Reviewed Journal]2019. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Mar 01, 2019 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab04a2Full text available |
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18 |
Material Type: Article
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A Search for H-Dropout Lyman Break Galaxies at z ∼ 12–16The Astrophysical journal, 2022-04, Vol.929 (1), p.1 [Peer Reviewed Journal]2022. The Author(s). Published by the American Astronomical Society. ;Copyright Determination: PUBLIC_USE_PERMITTED ;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: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac53a9Full text available |
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19 |
Material Type: Article
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CIGALE: a python Code Investigating GALaxy EmissionAstronomy and astrophysics (Berlin), 2019-02, Vol.622 [Peer Reviewed Journal]Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201834156Digital Resources/Online E-Resources |
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20 |
Material Type: Article
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Target Selection for the SDSS-IV APOGEE-2 SurveyThe Astronomical journal, 2017-11, Vol.154 (5), p.198 [Peer Reviewed Journal]2017. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Nov 2017 ;ISSN: 0004-6256 ;ISSN: 1538-3881 ;EISSN: 1538-3881 ;DOI: 10.3847/1538-3881/aa8df9Full text available |