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| Result Number | Material Type | Add to My Shelf Action | Record Details and Options |
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| 1 |
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Chemical evolution of the Galactic bulge with different stellar populationsarXiv.org, 2024-052024. This work is published under http://creativecommons.org/licenses/by-nc-nd/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://creativecommons.org/licenses/by-nc-nd/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2405.12585Full text available |
| 2 |
Material Type: Article
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MAMMOTH-Subaru. II. Diverse Populations of Circumgalactic Ly\(\alpha\) Nebulae at Cosmic NoonarXiv.org, 2024-052024. 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. ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2405.13113Full text available |
| 3 |
Material Type: Article
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Forecasts for Galaxy Formation and Dark Matter Constraints from Dwarf Galaxy SurveysarXiv.org, 2024-052024. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2401.10318Full text available |
| 4 |
Material Type: Article
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The evolution of the radio luminosity function of group galaxies in COSMOSarXiv.org, 2024-052024. This work is published under http://creativecommons.org/licenses/by-nc-sa/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://creativecommons.org/licenses/by-nc-sa/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2204.02082Full text available |
| 5 |
Material Type: Article
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The ratio of [Eu/\(\alpha\)] differentiates accreted/in-situ Milky Way stars across metallicities, as indicated by both field stars and globular clustersarXiv.org, 2024-052024. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2405.08963Full text available |
| 6 |
Material Type: Article
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QSOFEED: The relationship between star formation and AGN FeedbackarXiv.org, 2024-052024. 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. ;http://creativecommons.org/licenses/by/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2405.06421Full text available |
| 7 |
Material Type: Article
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Pre-supernova stellar feedback in nearby starburst dwarf galaxiesarXiv.org, 2024-052024. 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. ;http://creativecommons.org/licenses/by/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2402.12497Full text available |
| 8 |
Material Type: Article
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Structure and Kinematics of Star-forming Elliptical Galaxies in SDSS-MaNGAarXiv.org, 2024-052024. This work is published under http://creativecommons.org/licenses/by-nc-nd/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://creativecommons.org/licenses/by-nc-nd/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2405.04166Full text available |
| 9 |
Material Type: Article
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A massive galaxy that formed its stars at \(z \sim 11\)arXiv.org, 2024-052024. 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. ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2308.05606Full text available |
| 10 |
Material Type: Article
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Two Distinct Classes of Quiescent Galaxies at Cosmic Noon Revealed by JWST PRIMER and UNCOVERarXiv.org, 2024-042024. 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. ;http://creativecommons.org/licenses/by/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2312.15012Full text available |
| 11 |
Material Type: Article
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The JWST-SUSPENSE Ultradeep Spectroscopic Program: Survey Overview and Star-Formation Histories of Quiescent Galaxies at 1 < z < 3arXiv.org, 2024-042024. 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. ;http://creativecommons.org/licenses/by/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2404.12432Full text available |
| 12 |
Material Type: Article
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The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning \(0.2 \lesssim z \lesssim 15\)arXiv.org, 2024-042024. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2310.01276Full text available |
| 13 |
Material Type: Article
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JWST-JADES. Possible Population III signatures at z=10.6 in the halo of GN-z11arXiv.org, 2024-042024. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2306.00953Full text available |
| 14 |
Material Type: Article
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The APO-K2 Catalog. II. Accurate Stellar Ages for Red Giant Branch Stars across the Milky WayarXiv.org, 2024-042024. 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. ;http://creativecommons.org/licenses/by/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2403.16250Full text available |
| 15 |
Material Type: Article
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Disentanglement of the chemodynamical assembly: mapping the Milky Way disksarXiv.org, 2024-042024. 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. ;http://creativecommons.org/licenses/by/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2404.09968Full text available |
| 16 |
Material Type: Article
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Stellar population astrophysics (SPA) with the TNG: Measurement of the He I 10830Å line in the open cluster Stock 2arXiv.org, 2024-042024. 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. ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2404.09975Full text available |
| 17 |
Material Type: Article
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Observational Tests of Active Galactic Nuclei Feedback: An Overview of Approaches and InterpretationarXiv.org, 2024-042024. 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. ;http://creativecommons.org/licenses/by/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2404.08050Full text available |
| 18 |
Material Type: Article
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Resolved UV and optical color gradients reveal environmental influence on galaxy evolution at redshift z\(\sim\)1.6arXiv.org, 2024-042024. 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. ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2404.07355Full text available |
| 19 |
Material Type: Article
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Stellar populations and origin of thick disks in AURIGA simulationsarXiv.org, 2024-042024. This work is published under http://creativecommons.org/licenses/by-nc-nd/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://creativecommons.org/licenses/by-nc-nd/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2311.13700Full text available |
| 20 |
Material Type: Article
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No top-heavy stellar initial mass function needed: the ionizing radiation of GS9422 can be powered by a mixture of AGN and starsarXiv.org, 2024-042024. This work is published under http://creativecommons.org/licenses/by-nc-sa/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://creativecommons.org/licenses/by-nc-sa/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2404.02333Full text available |
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