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Photometric follow-up of SN2018zd/Gaia18anr from Bialkow

ATel #12079; P. Mikolajczyk (Wroclaw University Astronomical Observatory), L. Wyrzykowski (Warsaw University Astronomical Observatory)
on 4 Oct 2018; 15:21 UT
Credential Certification: Lukasz Wyrzykowski (wyrzykow@astrouw.edu.pl)

Subjects: Optical, Supernovae, Transient

We report here on the photometric observations of the Type IIn supernova SN 2018zd (otherwise known as Gaia18anr), discovered by Koichi Itagaki and classified by Zhang et al. (ATel #11379), with the 60-cm Cassegrain reflector in Astronomical Observatory of the University of Wroclaw (Bialkow, Poland) over the period of 3 months (from April 14 2018 to July 15 2018). Observations took place during twelve photometric nights and data has been collected in four bands of the Johnson-Cousins photometric system: B, V, Rc and Ic. I observed substantial and consistent decrease in brightness in all four photometric bands, till the point where measurements became partly unreliable due to the limitations of aforementioned telescope. We found that Gaia measurements in G-band are more or less consistent with Rc band measurements over long period of time. We also found that during two nights: May 13, 2018 and May 19, 2018 a little increase in brightness may be spotted in all used photometric bands. Such an effect may be spotted also in the data taken from other nights. Taking into account the precision of Gaia18anr photometry (especially during the first month of observations), we suggest it may be a photometric manifestation of decay processes of radioactive elements.

The follow-up photometric data are shown on Gaia alerts follow-up webpage and can be requested from the author.

We acknowledge the Gaia Photometric Alerts group (http://gsaweb.ast.cam.ac.uk/alerts). We also acknowledge the use of the Cambridge Photometric Calibration Server (http://gsaweb.ast.cam.ac.uk/followup), developed and maintained by Lukasz Wyrzykowski, Sergey Koposov, Arancha Delgado, Pawel Zielinski, funded by the European Union's Horizon 2020 research and innovation programme under grant agreement No 730890 (OPTICON).

Follow-up observations on Gaia Alerts webpage