V2492 Cyg light variations (Kospal+, 2013)

Kospal, A.; Abraham, P.; Acosta-Pulido, J. A.; Arevalo Morales, M. J.; Balog, Z.; Carnerero, M. I.; Szegedi-Elek, E.; Farkas, A.; Henning, T.; Kelemen, J.; Kovacs, T.; Kun, M.; Marton, G.; Meszaros, Sz.; Moor, A.; Pal, A.; Sarneczky, K.; Szakats, R.; Szalai, N.; Szing, A.; Toth, I.; Turner, N. J.; Vida, K.
Bibliographical reference

VizieR On-line Data Catalog: J/A+A/551/A62. Originally published in: 2013A&A...551A..62K

Advertised on:
6
2013
Number of authors
23
IAC number of authors
3
Citations
0
Refereed citations
0
Description
We obtained optical and near-infrared images with VRIJHKs filters between 2010 September 19 and 2012 October 12 using four telescopes: the Schmidt and RCC telescopes of the Konkoly Observatory (Hungary), as well as the IAC-80 and Telescopio Carlos Sanchez (TCS) telescopes of the Teide Observatory in the Canary Islands (Spain). We observed V2492 Cyg using the Spitzer Space Telescope in the post-helium phase at eight epochs between 2011 September 8 and 2012 September 16 (PID: 80165, PI: P. Abraham). We conducted a four-epoch far-infrared monitoring of V2492 Cyg with the Herschel Space Observatory between 2011 October 29 and 2012 January 11 (PID: DDTakospal2, PI: A. Kospal). We used the Photodetector Array Camera and Spectrometer (PACS) instrument. (1 data file).