activity
20072022
most citedSN 2003du: 480 days in the Life of a Normal Type Ia Supernova

182 citations · 336 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2022★ 1 cited

FG Sge: new multicolor photometry and short-term dust shell clearing in 2019

V. P. Arkhipova, N. P. Ikonnikova, V. I. Shenavrin +6

We present the results of a new stage of the long-term photometric study of FG Sge which is a quickly evolving central star of the planetary nebula Hen 1-5. Our new observations ca…

astro-ph.SR2019★ 16 cited

Supernova 2018aoq and a distance to Seyfert galaxy NGC 4151

D. Yu. Tsvetkov, P. V. Baklanov, M. Sh. Potashov +9

We present optical photometric observations of SN 2018aoq from 2 to 100 days after explosion, and 7 spectra at epochs from 11 to 71 days. The light curves and spectra are typical f…

astro-ph.SR2017★ 1 cited

The light curves of type II-P SN 2017eaw: first 200 days

D. Yu. Tsvetkov, S. Yu. Shugarov, I. M. Volkov +7

We present UBVRI photometry of the supernova 2017eaw in NGC 6946, obtained in the period from May 14 until December 7, 2017. We derive dates and magnitudes of maximum light in the…

astro-ph.SR2015★ 2 cited

PSN J07285387+3349106 in NGC 2388: an extremely rapidly declining luminous supernova

D. Yu. Tsvetkov, I. M. Volkov, N. N. Pavlyuk

We present CCD BVRI photometry for PSN J07285387+3349106 in NGC 2388 collected from 2015 February 17 until March 17. Decaying by 3.6 mag in the R band in the first 20 days post-max…

astro-ph.SR2014★ 42 cited

Kiso Supernova Survey (KISS): Survey Strategy

Tomoki Morokuma, Nozomu Tominaga, Masaomi Tanaka +58

The Kiso Supernova Survey (KISS) is a high-cadence optical wide-field supernova (SN) survey. The primary goal of the survey is to catch the very early light of a SN, during the sho…

astro-ph.SR2014

Supernova 2014J at maximum light

D. Yu. Tsvetkov, V. G. Metlov, S. Yu. Shugarov +2

We present UBVRI photometry of the supernova 2014J in M82, obtained in the period from January 24 until March 3, 2014, as well as two spectra, taken on February 4 and March 5. We d…