UBVJHKLM Photometry of Nova Cygni 1992 Virtual Observatory Resource

Authors

1. Kolotilov E.A.
2. Nadzhip A.E.
3. Shenavrin V.I.
4. Yudin B.F.

Published by

CDS

Abstract

The results of photometric UBVJHKLM observations of Nova Cygni 1992 performed from the 83d until the 290th day after the nova outburst are presented. The accuracy of the brightness estimate was better than 0.03mag for UBVJHK, 0.05mag for L, and 0.1mag for M bands.

Keywords

1. novae
2. infrared-photometry
3. visible-astronomy
4. Wide-band photometry

Bibliographic source Bibcode

1994AZh....71..618K

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/71/618

IVOA Identifier IVOID

ivo://CDS.VizieR/J/AZh/71/618

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AZh/71/618
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AZh/71/618
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AZh/71/618

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).