Margarita Safonova
Indian Institute of Astrophysics
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Publication
Featured researches published by Margarita Safonova.
The Astrophysical Journal | 2015
Subhash Bose; Firoza Sutaria; Brijesh Kumar; Chetna Duggal; Kuntal Misra; Peter J. Brown; Mridweeka Singh; Vikram V. Dwarkadas; Donald G. York; Sayan Chakraborti; H. C. Chandola; Julie Dahlstrom; Alak Ray; Margarita Safonova
We present optical photometric and spectroscopic observations of supernova 2013ej. It is one of the brightest type II supernovae exploded in a nearby (
New Astronomy | 2010
Margarita Safonova; C. Stalin
\sim 10
Monthly Notices of the Royal Astronomical Society | 2017
P. T. Rahna; Jayant Murthy; Margarita Safonova; Firoza Sutaria; S. B. Gudennavar; S. G. Bubbly
Mpc) galaxy NGC 628. The light curve characteristics are similar to type II SNe, but with a relatively shorter (
arXiv: Instrumentation and Methods for Astrophysics | 2014
A. G. Sreejith; Mayuresh Sarpotdar; Akshata Nayak; Margarita Safonova; Jayant Murthy
\sim85
Journal of Astronomical Telescopes, Instruments, and Systems | 2016
Kaipacheri Nirmal; A. G. Sreejith; Joice Mathew; Mayuresh Sarpotdar; S. Ambily; Ajin Prakash; Margarita Safonova; Jayant Murthy
day) and steeper (
The Astrophysical Journal | 2014
S. Calchi Novati; V. Bozza; I. Bruni; M. Dall'Ora; F. De Paolis; M. Dominik; R. Gualandi; G. Ingrosso; Ph. Jetzer; L. Mancini; A. A. Nucita; Margarita Safonova; G. Scarpetta; Mauro Sereno; F. Strafella; Annapurni Subramaniam; A. Gould
\sim1.7
Astrophysics and Space Science | 2013
S. Ravichandran; K. Preethi; Margarita Safonova; J Murthy
mag (100 d)
Proceedings of SPIE | 2016
A. G. Sreejith; Joice Mathew; Mayuresh Sarpotdar; K. Nirmal; S. Ambily; Ajin Prakash; Margarita Safonova; Jayant Murthy
^{-1}
Planetary and Space Science | 2015
Nalin H. Samarasinha; Beatrice E. A. Mueller; Matthew M. Knight; Tony L. Farnham; John Briol; Noah Brosch; John Caruso; Xing Gao; Edward Leocadio Gomez; Tim Lister; Carl W. Hergenrother; Susan Hoban; Roy Prouty; Mike Holloway; N. C. Howes; E. Guido; Man-To Hui; Joseph H. Jones; Tyler B. Penland; Samuel R. Thomas; Jim Wyrosdick; Nikolai Kiselev; Aleksandra V. Ivanova; Thomas G. Kaye; Jean-Baptist Kikwaya Eluo; Betty P.S. Lau; Z.-Y. Lin; José Luis Martin; A. S. Moskvitin; M. Nicolini
in V) plateau phase. The SN shows a large drop of 2.4 mag in V band brightness during plateau to nebular transition. The absolute ultraviolet (UV) light curves are identical to SN 2012aw, showing a similar UV plateau trend extending up to 85 days. The radioactive
International Conference on Optics and Photonics 2015 | 2015
A. G. Sreejith; Margarita Safonova; Jayant Murthy
^{56}
