BVRcIC photometry of V2615 Oph (Munari+, 2008)

Details BVRcIC photometry of V2615 Oph (Munari+, 2008) BVRcIC photometry of V2615 Oph (Munari+, 2008)

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..73870344m&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/387/344. Originally published in: 2008MNRAS.387..344M

Astronomy and Astrophysics

Astronomy

Novae, Binaries: Cataclysmic, Photometry: Ubvri

Scientific paper

The BVRcIc photometric evolution of NOph07 has been monitored, for seven months and over a 7mag decline, with three different telescopes: (a) the Sonoita Research Observatory (SRO) 0.35-m Celestron C14 robotic telescope (b) the 0.30-m Meade RCX-400 f/8 Schmidt-Cassegrain telescope owned by Associazione Astrofili Valle di Cembra (Trento, Italy), and (c) the 0.50-m f/8 Ritchey-Cretien telescope operated on top of Mt. Zugna by Museo Civico di Rovereto (Trento, Italy)
(1 data file).

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