C
C. S. Stalin
Researcher at Indian Institute of Astrophysics
Publications - 56
Citations - 1481
C. S. Stalin is an academic researcher from Indian Institute of Astrophysics. The author has contributed to research in topics: Galaxy & Quasar. The author has an hindex of 19, co-authored 56 publications receiving 1295 citations. Previous affiliations of C. S. Stalin include National Centre for Radio Astrophysics & Institut d'Astrophysique de Paris.
Papers
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Journal ArticleDOI
POINT-AGAPE pixel lensing survey of M31: Evidence for a MACHO contribution to galactic halos
S. Calchi Novati,S. Paulin-Henriksson,Jin H. An,P. Baillon,Vasily Belokurov,Bernard Carr,M. Creze,Nick Evans,Y. Giraud-Heraud,Andrew Gould,Paul C. Hewett,Ph. Jetzer,Jean Kaplan,E. Kerins,Stephen J. Smartt,Stephen J. Smartt,C. S. Stalin,Yiannis Tsapras,M. J. Weston +18 more
TL;DR: The POINT-AGAPE collaboration carried out a search for gravitational microlensing toward M31 to reveal galactic dark matter in the form of MACHOs (Massive Astrophysical Compact Halo Objects) in the halos of the Milky Way and M31 as discussed by the authors.
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A Catalog of Narrow Line Seyfert 1 Galaxies from the Sloan Digital Sky Survey Data Release 12
TL;DR: In this paper, the authors presented a new catalog of narrow-line Seyfert 1 (NLSy1) galaxies from the Sloan Digital Sky Survey Data Release 12 (SDSS DR12).
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A Catalog of Narrow Line Seyfert 1 Galaxies from the Sloan Digital Sky Survey Data Release 12
TL;DR: In this paper, the authors presented a new catalog of narrow-line Seyfert 1 (NLSy1) galaxies from the Sloan Digital Sky Survey Data Release 12 (SDSS DR12).
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Multiband optical monitoring of the blazars S5 0716+714 and BL Lacertae
C. S. Stalin,C. S. Stalin,C. S. Stalin,Gopal-Krishna,Gopal-Krishna,Ram Sagar,Paul J. Wiita,Vijay Mohan,Ashwani Pandey +8 more
TL;DR: In this article, multiband optical photometric monitoring of two well known blazars, S5 0716+714 and BL Lacertae, carried out during 1996 and 2000−01 withan aim to study optical variations on time scales ranging from minutes to hours and longer.
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Intranight optical variability of radio‐quiet and radio lobe‐dominated quasars
TL;DR: In this paper, the authors present results of a program of multi-epoch, intranight optical monitoring of a sample of non-blazar-type active galactic nuclei (AGN), which includes seven radio-quiet quasars (RQQs) and an equal number of radio-loud, lobe-dominated quaars (LDQs), covering a redshift range from about 0.2 to 2.0.