Pre-eruption light curves for Nova U Sco Virtual Observatory Resource

Authors

1. Schaefer B.E.
2. Pagnotta A.
3. Xiao L.
4. Darnley M.J.
5. Bode M.F.
6. Harris B.G.,Dvorak S.
7. Menke J.
8. Linnolt M.
9. Templeton M.
10. Henden A.A.
11. Pojmanski G.,Pilecki B.
12. Szczygiel D.M.
13. Watanabe Y.

Published by

CDS

Abstract

We report the discovery by B.G. Harris and S. Dvorak on JD 2455224.9385 (2010 January 28.4385 UT) of the predicted eruption of the recurrent nova U Scorpii (U Sco). We also report 815 magnitudes (and 16 useful limits) on the pre-eruption light curve in the UBVRI and Sloan r' and i' bands from 2000.4 up to 9hr before the peak of the 2010 January eruption.

Keywords

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

Bibliographic source Bibcode

2010AJ....140..925S

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https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/140/925

IVOA Identifier IVOID

ivo://CDS.VizieR/J/AJ/140/925

Document Object Identifer DOI

doi:10.26093/cds/vizier.51400925

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