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1 |
Material Type: Article
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THE CO-TO-H 2 CONVERSION FACTOR AND DUST-TO-GAS RATIO ON KILOPARSEC SCALES IN NEARBY GALAXIESThe Astrophysical journal, 2013-11, Vol.777 (1), p.5 [Peer Reviewed Journal]ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/777/1/5Full text available |
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2 |
Material Type: Article
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Revealing Hidden Substructures in the M BH –σ Diagram, and Refining the Bend in the L–σ RelationThe Astrophysical journal, 2019-12, Vol.887 (1), p.10 [Peer Reviewed Journal]ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab50b7Full text available |
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3 |
Material Type: Article
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Evidence for a Systematic Offset of −80 μas in the Gaia DR2 ParallaxesThe Astrophysical journal, 2018-07, Vol.862 (1), p.61 [Peer Reviewed Journal]Copyright IOP Publishing Jul 20, 2018 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aacafcFull text available |
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4 |
Material Type: Article
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THE SINS SURVEY OF z similar to 2 GALAXY KINEMATICS: PROPERTIES OF THE GIANT STAR-FORMING CLUMPSThe Astrophysical journal, 2011-06 (2), p.jQuery1323908059692='48'-jQuery1323908059692='48' [Peer Reviewed Journal]ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/733/2/101Full text available |
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5 |
Material Type: Article
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THE CO-TO-H 2 CONVERSION FACTOR FROM INFRARED DUST EMISSION ACROSS THE LOCAL GROUPThe Astrophysical journal, 2011-08, Vol.737 (1), p.12 [Peer Reviewed Journal]ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/737/1/12Full text available |
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6 |
Material Type: Article
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THE RADIAL DISTRIBUTION OF H 2 AND CO IN TW HYA AS REVEALED BY RESOLVED ALMA OBSERVATIONS OF CO ISOTOPOLOGUESThe Astrophysical journal, 2016-06, Vol.823 (2), p.91 [Peer Reviewed Journal]ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/0004-637X/823/2/91Full text available |
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7 |
Material Type: Article
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ABIOTIC O 2 LEVELS ON PLANETS AROUND F, G, K, AND M STARS: POSSIBLE FALSE POSITIVES FOR LIFE?The Astrophysical journal, 2015-10, Vol.812 (2), p.137 [Peer Reviewed Journal]ISSN: 1538-4357 ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/812/2/137Full text available |
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8 |
Material Type: Article
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The Environmental Dependence of the X CO Conversion FactorThe Astrophysical journal, 2020-11, Vol.903 (2), p.142 [Peer Reviewed Journal]ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/abbdabFull text available |
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9 |
Material Type: Article
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Cosmos Photometric Redshifts with 30-Bands for 2-deg2The Astrophysical journal, 2009-01, Vol.690 (2), p.1236-1249 [Peer Reviewed Journal]ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/690/2/1236Full text available |
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10 |
Material Type: Article
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Characterizing Extreme Emission Line Galaxies. II. A Self-consistent Model of Their Ionizing SpectrumThe Astrophysical journal, 2022-10, Vol.938 (1), p.16 [Peer Reviewed Journal]ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac8f2cFull text available |
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11 |
Material Type: Article
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DISEQUILIBRIUM CARBON, OXYGEN, AND NITROGEN CHEMISTRY IN THE ATMOSPHERES OF HD 189733b AND HD 209458bThe Astrophysical journal, 2011-08 (1), p.jQuery1323905097223='48'-jQuery1323905097223='48' [Peer Reviewed Journal]ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/737/1/15Full text available |
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12 |
Material Type: Article
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Cluster Cepheids with High Precision Gaia Parallaxes, Low Zero-point Uncertainties, and Hubble Space Telescope PhotometryThe Astrophysical journal, 2022-10, Vol.938 (1), p.36 [Peer Reviewed Journal]2022. The Author(s). Published by the American Astronomical Society. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac8f24Full text available |
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13 |
Material Type: Article
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THE M BH - L SPHEROID RELATION AT HIGH AND LOW MASSES, THE QUADRATIC GROWTH OF BLACK HOLES, AND INTERMEDIATE-MASS BLACK HOLE CANDIDATESThe Astrophysical journal, 2013-02, Vol.764 (2), p.151 [Peer Reviewed Journal]ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/764/2/151Full text available |
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14 |
Material Type: Article
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The Hydrogen-poor Superluminous Supernovae from the Zwicky Transient Facility Phase I Survey. II. Light-curve Modeling and Characterization of UndulationsThe Astrophysical journal, 2023-01, Vol.943 (1), p.42 [Peer Reviewed Journal]2023. The Author(s). Published by the American Astronomical Society. ;ISSN: 0004-637X ;ISSN: 1538-4357 ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aca162Full text available |
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15 |
Material Type: Article
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The Young Supernova Experiment: Survey Goals, Overview, and OperationsThe Astrophysical journal, 2021-02, Vol.908 (2), p.143 [Peer Reviewed Journal]2021. The American Astronomical Society. All rights reserved. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/abd7f5Full text available |
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16 |
Material Type: Article
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The Hydrogen-poor Superluminous Supernovae from the Zwicky Transient Facility Phase I Survey. I. Light Curves and MeasurementsThe Astrophysical journal, 2023-01, Vol.943 (1), p.41 [Peer Reviewed Journal]2023. The Author(s). Published by the American Astronomical Society. ;ISSN: 0004-637X ;ISSN: 1538-4357 ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aca161Full text available |
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17 |
Material Type: Article
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The Explosion of Helium Stars Evolved with Mass LossThe Astrophysical journal, 2020-02, Vol.890 (1), p.51 [Peer Reviewed Journal]2020. The American Astronomical Society. All rights reserved. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab6458Full text available |
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18 |
Material Type: Article
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Measuring Turbulent Motion in Planet-forming Disks with ALMA: A Detection around DM Tau and Nondetections around MWC 480 and V4046 SgrThe Astrophysical journal, 2020-06, Vol.895 (2), p.109 [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/ab8cc5Full text available |
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19 |
Material Type: Article
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Multiwavelength Study of Massive Galaxies at z similar to 2. I. Star Formation and Galaxy GrowthThe Astrophysical journal, 2007-11, Vol.670 (1), p.156-172 [Peer Reviewed Journal]ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1086/521818Full text available |
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20 |
Material Type: Article
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Secure Mass Measurements From Transit Timing: 10 Kepler Exoplanets Between 3 and 8M⊕ with Diverse Densities and Incident FluxesThe Astrophysical journal, 2016-03, Vol.820 (1) [Peer Reviewed Journal]Copyright Determination: MAY_INCLUDE_COPYRIGHT_MATERIAL ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/0004-637X/820/1/39Full text available |