Supernovae candidates Gaia17aty, Gaia17atz and Gaia17aud confirmed by Euler imaging
ATel #10238; S. Blanco-Cuaresma, S. Saesen, M. Roelens, T. Semaan, L. Palaversa, N. Mowlavi, L. Eyer (Department of Astronomy, University of Geneva, Switzerland)
on 3 Apr 2017; 00:08 UT
Credential Certification: Sergi Blanco-Cuaresma (Sergi.Blanco@unige.ch)
Subjects: Supernovae, Transient
We report confirmation of Gaia Science Alerts supernovae candidates
Gaia17aty,
Gaia17atz and
Gaia17aud.
Images were obtained through modified Gunn R band filter of the ECAM instrument installed on the Swiss 1.2m Euler telescope at La Silla, on 2017 March 29th - 30th.
These new sources are not visible in archival 2MASS and DSS images. ECAM modified Gunn R band 300x300 pixel cut out images are provided (N is up, E is left, the scale is 0.215"/pix, dead pixels are masked) at the following links:
Gaia17aty,
Gaia17atz and
Gaia17aud.
| MJD |
Gaia17aty |
Gaia17atz |
Gaia17aud |
| 57,842 |
~16.39 |
~17.96 |
~17.83 |
| 57,843 |
~16.38 |
~18.00 |
- |
| 57,844 |
- |
- |
~17.85 |
The photometric calibrations were obtained using the
Cambridge Photometric Calibration Server (CPCS), designed and maintained by Sergey Koposov and Lukasz Wyrzykowski. We acknowledge ESA Gaia, DPAC and the Photometric Science Alerts Team (
http://gsaweb.ast.cam.ac.uk/alerts).
