Detection efficiency and photometry in supernova surveys The Stockholm VIMOS Supernova Survey I




Melinder J, Mattila S, Ostlin G, Trinchant LM, Fransson C

PublisherEDP SCIENCES S A

2008

Astronomy and Astrophysics

ASTRONOMY & ASTROPHYSICS

ASTRON ASTROPHYS

490

1

419

434

16

0004-6361

DOIhttps://doi.org/10.1051/0004-6361:20079206



Conclusions. Our study has shown that ISIS 2.2 works well for the SVISS data. We have found that the detection efficiency and photometric accuracy of the survey are affected by the stamp selection for the image subtraction and by host galaxy brightness. With our tools the subtraction results can be further optimised, any systematic effects can be controlled and photometric errors estimated, which is very important for the SVISS, as well as for future SN searches based on large imaging surveys such as Pan-STARRS and LSST.



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