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1 |
Material Type: Article
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A Near-infrared Period-Luminosity Relation for Miras in NGC 4258, an Anchor for a New Distance LadderThe Astrophysical journal, 2018-04, Vol.857 (1), p.67 [Peer Reviewed Journal]2018. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Apr 10, 2018 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aab6b3Full text available |
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Material Type: Article
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Hubble Space Telescope Observations of Mira Variables in the SN Ia Host NGC 1559: An Alternative Candle to Measure the Hubble ConstantThe Astrophysical journal, 2020-01, Vol.889 (1), p.5 [Peer Reviewed Journal]2020. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jan 20, 2020 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab5dbdFull text available |
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3 |
Material Type: Article
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Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDMThe Astrophysical journal, 2019-05, Vol.876 (1), p.85 [Peer Reviewed Journal]2019. The American Astronomical Society. ;Copyright IOP Publishing May 01, 2019 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab1422Full text available |
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4 |
Material Type: Article
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THE CARNEGIE-CHICAGO HUBBLE PROGRAM. I. AN INDEPENDENT APPROACH TO THE EXTRAGALACTIC DISTANCE SCALE USING ONLY POPULATION II DISTANCE INDICATORSThe Astrophysical journal, 2016-12, Vol.832 (2), p.210 [Peer Reviewed Journal]Copyright IOP Publishing Dec 01, 2016 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/0004-637X/832/2/210Full text available |
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5 |
Material Type: Article
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THE CARNEGIE HUBBLE PROGRAM: THE DISTANCE AND STRUCTURE OF THE SMC AS REVEALED BY MID-INFRARED OBSERVATIONS OF CEPHEIDSThe Astrophysical journal, 2016-01, Vol.816 (2), p.1-10 [Peer Reviewed Journal]2016. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jan 10, 2016 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/0004-637X/816/2/49Full text available |
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6 |
Material Type: Article
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On the Use of Field RR Lyrae as Galactic Probes. I. The Oosterhoff Dichotomy Based on Fundamental Variables Partially based on observations collected under ESO programs 297.D-5047 (PI: G. Bono) and 083.B-0281 (PI: D. Romano)The Astrophysical journal, 2019-09, Vol.882 (2) [Peer Reviewed Journal]2019. The American Astronomical Society. All rights reserved. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab3977Full text available |
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7 |
Material Type: Article
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A New Cepheid Distance to the Giant Spiral M101 Based on Image Subtraction of Hubble Space Telescope/Advanced Camera for Surveys ObservationsThe Astrophysical journal, 2011-06, Vol.733 (2), p.124-jQuery1323908181161='48' [Peer Reviewed Journal]2015 INIST-CNRS ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/733/2/124 ;CODEN: ASJOABFull text available |
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8 |
Material Type: Article
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New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble ConstantThe Astrophysical journal, 2018-03, Vol.855 (2), p.136 [Peer Reviewed Journal]2018. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Mar 10, 2018 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aaadb7Full text available |
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9 |
Material Type: Article
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KLLR: A Scale-dependent, Multivariate Model Class for Regression AnalysisThe Astrophysical journal, 2022-06, Vol.931 (2), p.166 [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: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac6ac7Full text available |
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10 |
Material Type: Article
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Rotation of Late-type Stars in Praesepe with K2The Astrophysical journal, 2017-04, Vol.839 (2), p.92 [Peer Reviewed Journal]2017. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Apr 20, 2017 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aa6aa4Full text available |
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11 |
Material Type: Article
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OPTICAL IDENTIFICATION OF CEPHEIDS IN 19 HOST GALAXIES OF TYPE Ia SUPERNOVAE AND NGC 4258 WITH THE HUBBLE SPACE TELESCOPEThe Astrophysical journal, 2016-10, Vol.830 (1), p.10 [Peer Reviewed Journal]Copyright IOP Publishing Oct 10, 2016 ;ISSN: 0004-637X ;ISSN: 1538-4357 ;EISSN: 1538-4357 ;DOI: 10.3847/0004-637X/830/1/10Full text available |
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12 |
Material Type: Article
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Metallicities of Classical Cepheids in the Inner Galactic DiskThe Astrophysical journal, 2023-09, Vol.954 (2), p.198 [Peer Reviewed Journal]2023. The Author(s). Published by the American Astronomical Society. ;2023. 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/aced93Full text available |
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13 |
Material Type: Article
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Short-term Variability of Evolved Massive Stars with TESSThe Astrophysical journal, 2019-06, Vol.878 (2), p.155 [Peer Reviewed Journal]2019. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jun 20, 2019 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab223fFull text available |
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14 |
Material Type: Article
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The Geometry of the Sagittarius Stream from Pan-STARRS1 3π RR LyraeThe Astrophysical journal, 2017-11, Vol.850 (1), p.96 [Peer Reviewed Journal]2017. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Nov 20, 2017 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aa960cFull text available |
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15 |
Material Type: Article
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FERMI-LAT GAMMA-RAY DETECTIONS OF CLASSICAL NOVAE V1369 CENTAURI 2013 AND V5668 SAGITTARII 2015The Astrophysical journal, 2016-08, Vol.826 (2), p.142-142 [Peer Reviewed Journal]2016. The American Astronomical Society. All rights reserved. ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-637X ;ISSN: 1538-4357 ;EISSN: 1538-4357 ;DOI: 10.3847/0004-637X/826/2/142Full text available |
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16 |
Material Type: Article
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THE VVV SURVEY REVEALS CLASSICAL CEPHEIDS TRACING A YOUNG AND THIN STELLAR DISK ACROSS THE GALAXY'S BULGEAstrophysical journal. Letters, 2015-10, Vol.812 (2), p.1-7 [Peer Reviewed Journal]2015. The American Astronomical Society. All rights reserved. ;ISSN: 2041-8205 ;ISSN: 2041-8213 ;EISSN: 2041-8213 ;DOI: 10.1088/2041-8205/812/2/L29Full text available |
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17 |
Material Type: Article
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The Fate of Binaries in the Galactic Center: The Mundane and the ExoticThe Astrophysical journal, 2019-06, Vol.878 (1), p.58 [Peer Reviewed Journal]2019. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jun 10, 2019 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab1e4dFull text available |
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18 |
Material Type: Article
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A FWHM-K2 CORRELATION IN BLACK HOLE TRANSIENTSThe Astrophysical journal, 2015-07, Vol.808 (1) [Peer Reviewed Journal]2015. The American Astronomical Society. All rights reserved. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/808/1/80Full text available |
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19 |
Material Type: Article
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VARIABLE STARS AND STELLAR POPULATIONS IN ANDROMEDA XXV. III. A CENTRAL CLUSTER OR THE GALAXY NUCLEUS?The Astrophysical journal, 2016-09, Vol.829 (1), p.26 [Peer Reviewed Journal]Copyright IOP Publishing Sep 20, 2016 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/0004-637X/829/1/26Full text available |
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20 |
Material Type: Article
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A Catalog of Potential Post–Common Envelope BinariesThe Astrophysical journal, 2021-10, Vol.920 (2), p.86 [Peer Reviewed Journal]2021. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Oct 01, 2021 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac13acFull text available |