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http://hdl.handle.net/20.500.12386/32984
Titolo: | Photometry and astrometry with JWST -- I. NIRCam Point Spread Functions and the first JWST colour-magnitude diagrams of a globular cluster | Autori: | Nardiello, D. Bedin, L. R. Burgasser, A. Salaris, M. CASSISI, Santi Griggio, M. Scalco, M. |
Data pubblicazione: | 2022 | Rivista: | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | Numero: | 517 | Fascicolo: | 1 | Da pagina:: | 484 | Abstract: | As the James Webb Space Telescope (JWST) has become fully operational, early-release data are now available to begin building the tools and calibrations for precision point-source photometry and astrometry in crowded cluster environments. Here, we present our independent reduction of NIRCam imaging of the metal-poor globular cluster M92, which were collected under Director's Discretionary Early Release Science programme ERS-1334. We derived empirical models of the Point Spread Function (PSF) for filters F090W, F150W, F277W, and F444W, and find that these PSFs: (i) are generally under-sampled (FWHM~2 pixel) in F150W and F444W and severely under-sampled (FWHM~1 pixel) in F090W and F277W; (ii) have significant variation across the field of view, up to ~15-20 %; and (iii) have temporal variations of ~3-4 % across multi-epoch exposures. We deployed our PSFs to determine the photometric precision of NIRCam for stars in the crowded, central regions of M92, measured to be at the ~0.01 mag level. We use these data to construct the first JWST colour-magnitude diagrams of a globular cluster. Employing existing stellar models, we find that the data reach almost the bottom of the M92 main sequence (~0.1 M$_{\odot}$), and reveal 24 white dwarf candidate members of M92 in the brightest portion of the white dwarf cooling sequence. The latter are confirmed through a cross-match with archival HST UV and optical data. We also detect the presence of multiple stellar populations along the low-mass main sequence of M92. | URI: | http://hdl.handle.net/20.500.12386/32984 | URL: | https://academic.oup.com/mnras/article/517/1/484/6705429 http://arxiv.org/abs/2209.06547v1 |
ISSN: | 0035-8711 | DOI: | 10.1093/mnras/stac2659 | Fulltext: | open |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
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