Supernova SN 2020nlb in Messier 85 brighter, again! 01 July 2020
Supernova SN 2020nlb in the galaxy Messier 85 is still rising: for the 6th night in a row, we have found it brighter!
The image above comes from the average of five, 120-seconds exposures, unfiltered, remotely taken with the “Elena” (PlaneWave 17″+Paramount ME+SBIG STL-6303E) robotic unit available as part of the Virtual Telescope Project. The supernova candidate is indicated by an arrow, in the upper left inset. The sky was bright because of twilight.
Again, we have found this transient brighter, for the 6th night in a row. Since its discovery, it steadily increased in brightness, as expected from an object caught so early in its explosion. Here we show our preliminary brightness estimates for SN 2020nlb:
- June 25.8271, mag. 16.8;
- June 26.8442, mag. 15.6;
- June 27.8392, mag. 15.0;
- June 28.8707, mag. 14.4;
- June 29.8399, mag. 13.9;
- June 30.8498, mag. 13.6;
- July 01.8639, mag. 13.3.
Those are unfiltered magnitudes, (R-mags for the reference stars from the Gaia DR1 star catalogue). The transient is clearly rising. This being a type Ia supernova, considering the distance of the host galaxy (Messier 85), it could reach magnitude 12.0/12.5 or so, assuming it behaves normally and there is no absorption.
Of course, we plan extensive follow-up of this object.
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