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Discovering vanishing objects in POSS I red images using the Virtual Observatory
CSIC INTA, Ctr Astrobiol CAB, Camino Bajo Castillo S-N, E-28692 Madrid, Spain..
KTH, Centres, Nordic Institute for Theoretical Physics NORDITA. Inst Astrofis Canarias, Avda Via Lactea S-N, E-38205 Tenerife, Spain..
CSIC INTA, Ctr Astrobiol CAB, Camino Bajo Castillo S-N, E-28692 Madrid, Spain..
2022 (English)In: Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, E-ISSN 1365-2966, Vol. 515, no 1, p. 1380-1391Article in journal (Refereed) Published
Abstract [en]

In this paper, we report a search for vanishing sources in POSS I red images using virtual observatory (VO) archives, tools, and services. The search, conducted in the framework of the VASCO project, aims at finding POSS I (red) sources not present in recent catalogues like Pan-STARRS DR2 (limiting magnitude r = 21.4) or Gaia EDR3 (limiting magnitude G = 21). We found 298 165 sources visible only in POSS I plates, out of which 288 770 had a cross-match within 5 arcsec in other archives (mainly in the infrared), 189 were classified as asteroids, 35 as variable objects, 3592 as artefacts from the comparison to a second digitization (Supercosmos), and 180 as high proper motion objects without information on proper motion in Gaia EDR3. The remaining unidentified transients (5399) as well as the 172 163 sources not detected in the optical but identified in the infrared regime are available from a VO compliant archive and can be of interest in searches for strong M-dwarf flares, high-redshift supernovae, asteroids, or other categories of unidentified red transients. No point sources were detected by both POSS-I and POSS-II before vanishing, setting the rate of failed supernovae in the Milky Way during 70 yr to less than one in one billion.

Place, publisher, year, edition, pages
Oxford University Press (OUP) , 2022. Vol. 515, no 1, p. 1380-1391
Keywords [en]
astronomical data bases: surveys, astronomical data bases: virtual observatory tools
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-316125DOI: 10.1093/mnras/stac1552ISI: 000829115300005Scopus ID: 2-s2.0-85129524687OAI: oai:DiVA.org:kth-316125DiVA, id: diva2:1686518
Note

QC 20220810

Available from: 2022-08-10 Created: 2022-08-10 Last updated: 2023-02-07Bibliographically approved

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Villarroel, Brian

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