The Panchromatic Hubble Andromeda Treasury. XXI. The Legacy Resolved Stellar Photometry Catalog
We present the final legacy version of stellar photometry for the Panchromatic Hubble Andromeda Treasury (PHAT) survey. We have reprocessed all of the Hubble Space Telescope Wide Field Camera 3 and Advanced Camera for Surveys near-ultraviolet (F275W, F336W), optical (F475W, F814W), and near-infrared...
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| Veröffentlicht in: | The Astrophysical journal. Supplement series 2023-10, Vol.268 (2), p.48 |
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| creator | Williams, Benjamin F. Durbin, Meredith Lang, Dustin Dalcanton, Julianne J. Dolphin, Andrew E. Smercina, Adam Merica-Jones, Petia Yanchulova Weisz, Daniel R. Bell, Eric F. Gilbert, Karoline M. Girardi, Léo Gordon, Karl Guhathakurta, Puragra Johnson, L. Clifton Lauer, Tod R. Seth, Anil Skillman, Evan |
| description | We present the final legacy version of stellar photometry for the Panchromatic Hubble Andromeda Treasury (PHAT) survey. We have reprocessed all of the Hubble Space Telescope Wide Field Camera 3 and Advanced Camera for Surveys near-ultraviolet (F275W, F336W), optical (F475W, F814W), and near-infrared (F110W, F160W) imaging from the PHAT survey using an improved method that optimized the survey depth and chip-gap coverage by including all overlapping exposures in all bands in the photometry. An additional improvement was gained through the use of charge transfer efficiency (CTE)–corrected input images, which provide more complete star finding as well as more reliable photometry for the NUV bands, which had no CTE correction in the previous version of the PHAT photometry. While this method requires significantly more computing resources and time than earlier versions where the photometry was performed on individual pointings, it results in smaller systematic instrumental completeness variations as demonstrated by cleaner maps in stellar density, and it results in optimal constraints on stellar fluxes in all bands from the survey data. Our resulting catalog has 138 million stars, 18% more than the previous catalog, with lower density regions gaining as much as 40% more stars. The new catalog produces nearly seamless population maps that show relatively well-mixed distributions for populations associated with ages older than 1–2 Gyr and highly structured distributions for the younger populations. |
| doi_str_mv | 10.3847/1538-4365/acea61 |
| format | Article |
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XXI. The Legacy Resolved Stellar Photometry Catalog</title><source>IOP Publishing Free Content</source><source>DOAJ Directory of Open Access Journals</source><source>EZB-FREE-00999 freely available EZB journals</source><source>IOPscience extra</source><source>Alma/SFX Local Collection</source><creator>Williams, Benjamin F. ; Durbin, Meredith ; Lang, Dustin ; Dalcanton, Julianne J. ; Dolphin, Andrew E. ; Smercina, Adam ; Merica-Jones, Petia Yanchulova ; Weisz, Daniel R. ; Bell, Eric F. ; Gilbert, Karoline M. ; Girardi, Léo ; Gordon, Karl ; Guhathakurta, Puragra ; Johnson, L. Clifton ; Lauer, Tod R. ; Seth, Anil ; Skillman, Evan</creator><creatorcontrib>Williams, Benjamin F. ; Durbin, Meredith ; Lang, Dustin ; Dalcanton, Julianne J. ; Dolphin, Andrew E. ; Smercina, Adam ; Merica-Jones, Petia Yanchulova ; Weisz, Daniel R. ; Bell, Eric F. ; Gilbert, Karoline M. ; Girardi, Léo ; Gordon, Karl ; Guhathakurta, Puragra ; Johnson, L. 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| subjects | Andromeda Galaxy Cameras Charge efficiency Charge transfer Density Field cameras HST photometry Hubble Space Telescope Infrared imaging Multi-color photometry Photometry Polls & surveys Populations Space telescopes Stars Stellar populations |
| title | The Panchromatic Hubble Andromeda Treasury. XXI. The Legacy Resolved Stellar Photometry Catalog |
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