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Spectroscopic classification of supernova Gaia16apd with the Nordic Optical Telescope

ATel #9071; T. Kangas (Turku), N. Elias-Rosa (INAF-Padova), P. Lundqvist (Stockholm), S. Mattila (Turku), M. Stritzinger (Aarhus U), H. Kuncarayakti (MAS, DAS), J. Harmanen (Turku), A. Pastorello (INAF-Padova), S. Benetti (INAF-Padova), E. Cappellaro (INAF-Padova), N. Blagorodnova (Caltech), S. Davis (FSU), S. Dong (KIAA-PKU), M. Fraser (IoA), C. Gall (Aarhus U), D. Harrison (IoA), S. Hodgkin (IoA), E. Y. Hsiao (FSU), P. Jonker (SRON), E. Kankare (QUB), Z. Kostrzewa-Rutkowska (Warsaw/SRON), M. Nielsen (Aarhus U), Paolo Ochner (INAF-Padova), J. L. Prieto (UDP, MAS), T. Reynolds (Turku, NOT), C. Romero-Canizales (MAS, UDP), F. Taddia (OKC), L. Tartaglia (INAF-Padova), G. Terreran (INAF-Padova/QUB), L. Tomasella (INAF-Padova), L. Wyrzykowski (Warsaw Observatory)
on 21 May 2016; 13:00 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Tuomas Kangas (tjakan@utu.fi)

Subjects: Optical, Supernovae, Transient

Referred to by ATel #: 9074, 9158

The NOT Unbiased Transient Survey (NUTS; ATel #8992) collaboration reports the spectroscopic classification of the supernova Gaia16apd in the galaxy SDSS J120251.71+441527.4. The candidate was discovered by the Gaia Photometric Science survey.

The observations were performed with the 2.56 m Nordic Optical Telescope equipped with ALFOSC (range 320-960 nm; FWHM resolution 1.6 nm) on 2016-05-20.92 UT.

 
Name               |  Host galaxy             |   Redshift   |  Discovery (UT) |  Discovery mag    |  Type    | Phase      | Notes 
Gaia16apd          | SDSS J120251.71+441527.4 |    0.102     |  2016-05-16.80  |   17.35           | SLSN-I   | ~-5 d      | (1) 

(1) The transient matches the type Ic superluminous supernova SN 2010gx at a few days before maximum brightness. The spectrum is blue, with clear broad O II absorption lines in the blue part. At the redshift of the host galaxy, the absolute magnitude from the Gaia photometry is -21.0.

We acknowledge ESA Gaia, DPAC and the Photometric Science Alerts Team (http://gsaweb.ast.cam.ac.uk/alerts).