Published March 2022
| Accepted Version + Published
Journal Article
Open
The Search for a Counterpart to NuSTAR J053449+2126.0
Abstract
(ATel #15171) have recently reported the discovery of an X-ray source, NuSTAR J053449+2126.0, during a calibration observation which took place on 2020 April 25. We scan the Zwicky Transient Facility alerts and archival photometry to determine the nature of the source. Palomar Gattini-IR is searched as well. We identify no obvious counterpart candidate. Follow-up X-ray and optical studies are needed to determine the true counterpart.
Additional Information
© 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Received February 2022; Revised March 2022; Accepted March 2022.Attached Files
Published - Rodriguez_2022p50.pdf
Accepted Version - 2203.08613.pdf
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Additional details
- Eprint ID
- 114282
- Resolver ID
- CaltechAUTHORS:20220413-235588800
- Created
-
2022-04-13Created from EPrint's datestamp field
- Updated
-
2022-06-30Created from EPrint's last_modified field
- Caltech groups
- Astronomy Department, Division of Geological and Planetary Sciences