Gaia16bhu, Gaia16bhk, Gaia16bho and Gaia16bhr transients confirmed by Mercator/Maia imaging
ATel #9524; S. Blanco-Cuaresma, M. Roelens, T. Semaan, L. Palaversa, N. Mowlavi, L. Eyer (Department of Astronomy, University of Geneva, Switzerland)
on 21 Sep 2016; 17:11 UT
Credential Certification: Sergi Blanco-Cuaresma (Sergi.Blanco@unige.ch)
Subjects: Optical, Cataclysmic Variable, Supernovae, Transient
We report confirmation of Gaia Science Alerts transients
Gaia16bhu,
Gaia16bhk,
Gaia16bho and
Gaia16bhr.
Images were obtained in G and R bands of the Maia instrument mounted to the Flemish 1.2m Mercator telescope at Roque de los Muchachos observatory, La Palma, Canary Islands, Spain, on 2016 September 18-19.
These new sources (close a galaxy in the case of Gaia16bho) are not visible in archival 2MASS and DSS images:
Gaia16bhu,
Gaia16bhk,
Gaia16bho and
Gaia16bhr.
MAIA G band 400x400 pixel cut-out image is provided (N is up, E is left and scale is 0.276"/pix).
MJD |
Gaia16bhu |
Gaia16bhk |
Gaia16bho |
Gaia16bhr |
|
G |
R |
G |
R |
G |
R |
G |
R |
57650.2 |
~18.2 |
~17.7 |
~17.6 |
- |
~18.3 |
~18.2 |
~19.9 |
- |
57651.2 |
~18.2 |
- |
~17.7 |
~17.9 |
~18.2 |
- |
~19.7 |
~18.6 |
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).