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Photometry and astrometry with JWST‑II: NIRCam distortion correction
DOI: 10.1002/asna.20230006 Bibcode: 2023AN....34430006G

Bedin, L. R.; Nardiello, D.; Griggio, M.

In preparation to make the most of our own planned James Webb Space Telescope investigations, we take advantage of publicly available calibration and early‑science observations to independently derive and test a geometric‑distortion solution for NIRCam detectors. Our solution is able to correct the distortion to better than 0.2 mas. Current data i…

2023 Astronomische Nachrichten
Gaia eHST JWST 13
Decomposition of the central structure of NGC 2273 in the NIR: A case study
DOI: 10.1002/asna.20230094 Bibcode: 2023AN....34430094S

Quirrenbach, A.; Gredel, R.; Thompson, D. +11 more

The Seyfert 2 galaxy NGC 2273 is a prime target to explore how active nuclei can be fed. It has a star‑forming innermost nuclear ring with a radius of 0.33kpc from where material may be funneled to the supermassive black hole in its center. In this article, we discuss high‑resolution adaptive optics aided JHKs images of NGC 2273 taken with the Lar…

2023 Astronomische Nachrichten
eHST 0
Possible optical counterparts of ULXs in NGC 1672
DOI: 10.1002/asna.20230027 Bibcode: 2023AN....34430027A

Sonbas, Eda; Allak, Sinan; Akyuz, Aysun +1 more

In this study, we use archival data from Hubble Space Telescope (HST), Chandra, XMM‑Newton, and Swift‑XRT, to probe the nature of 9 (X1‑X9) candidate ultraluminous X‑ray sources (ULXs) in NGC 1672. Our study focuses on using the precise source positions obtained via improved astrometry based on Chandra and HST observations to search for and identi…

2023 Astronomische Nachrichten
XMM-Newton eHST 0