output
19922026
most citedNeutrino Masses and Leptogenesis with Heavy Higgs Triplets

518 citations

Showing 2017 · astro-ph.HEShow all

12 papers · 2 filters

astro-ph.HE2017★ 21 cited

Correlated X-ray/UV/optical emission and short term variability in a Seyfert 1 galaxy NGC 4593

Main Pal, Sachindra Naik

We present a detailed multi-frequency analysis of an intense monitoring programme of Seyfert 1 galaxy NGC 4593 over a duration of nearly for a month with Swift observatory. We used…

astro-ph.HE2017★ 5 cited

Transition Elements in Supernova Presolar Grains: Condensation vs. Implantation

Kuljeet K. Marhas, Piyush Sharda

We compute the concentrations of five transition elements (Cr, Fe, Co, Ni and Zn) in supernova presolar grains (Silicon Carbide Type X) from the time they condense till the end of…

astro-ph.HE2017★ 28 cited

Understanding the spectral and timing behavior of a newly discovered transient X-ray pulsar Swift J0243.6+6124

Gaurava K. Jaisawal, Sachindra Naik, J. Chenevez

We present the results obtained from timing and spectral studies of the newly discovered accreting X-ray binary pulsar Swift J0243.6+6124 using a NuSTAR observation in 2017 October…

astro-ph.HE2017★ 12 cited

A Suzaku View of Accretion Powered X-ray Pulsar GX 1+4

Yuki Yoshida, Shunji Kitamoto, Hiroo Suzuki +3

We present results obtained from a Suzaku observation of the accretion powered X-ray pulsar GX 1+4. Broad-band continuum spectrum of the pulsar was found to be better described by…

astro-ph.HE2017★ 8 cited

Complex Optical/UV and X-ray Variability of the Seyfert 1 galaxy 1H 0419-577

Main Pal, Gulab C. Dewangan, Ajit K. Kembhavi +2

We present detailed broadband UV/optical to X-ray spectral variability of the Seyfert 1 galaxy 1H 0419-577 using six XMM-Newton observations performed during 2002-2003. These obser…

astro-ph.HE2017★ 17 cited

A precise measurement of the orbital period parameters of Cygnus X-3

Yash Bhargava, A. R. Rao, K. P. Singh +9

We present X-ray light curves of Cygnus X-3 as measured by the recently launched AstroSat satellite. The light curve folded over the binary period of 4.8 hours shows a remarkable s…

astro-ph.HE2017★ 81 cited

Stochastic modeling of multiwavelength variability of the classical BL Lac object OJ 287 on timescales ranging from decades to hours

A. Goyal, L. Stawarz, S. Zola +109

We present the results of our power spectral density analysis for the BL Lac object OJ\,287, utilizing the {\it Fermi}-LAT survey at high-energy -rays, {\it Swift}-XRT in X-rays…

astro-ph.HE2017★ 44 cited

Decade long RXTE monitoring observations of Be/X-ray binary pulsar EXO 2030+375

Prahlad Epili, Sachindra Naik, Gaurava K. Jaisawal +1

We present a comprehensive timing and spectral studies of Be/X-ray binary pulsar EXO 2030+375 using extensive Rossi X-ray Timing Explorer observations from 1995 till 2011, covering…

astro-ph.HE2017★ 8 cited

Surprise in simplicity: an unusual spectral evolution of a single pulse GRB 151006A

R. Basak, S. Iyyani, V. Chand +4

We present a detailed analysis of GRB 151006A, the first GRB detected by Astrosat CZT Imager (CZTI). We study the long term spectral evolution by exploiting the capabilities of \em…

astro-ph.HE2017★ 40 cited

A tale of two transients: GW170104 and GRB170105A

V. Bhalerao, M. M. Kasliwal, D. Bhattacharya +30

We present multi-wavelength follow-up campaigns by the AstroSat-CZTI and GROWTH collaborations to search for an electromagnetic counterpart to the gravitational wave event GW170104…

astro-ph.HE2017★ 63 cited

Prompt emission polarimetry of Gamma Ray Bursts with ASTROSAT CZT-Imager

Tanmoy Chattopadhyay, Santosh V. Vadawale, E. Aarthy +10

X-ray and Gamma-ray polarization measurements of the prompt emission of Gamma-ray bursts (GRBs) are believed to be extremely important for testing various models of GRBs. So far, t…

astro-ph.HE2017★ 47 cited

Detection of Cyclotron Resonance Scattering Feature in High Mass X-ray Binary Pulsar SMC X-2

Gaurava K. Jaisawal, Sachindra Naik

We report broadband spectral properties of the high mass X-ray binary pulsar SMC X-2 by using three simultaneous and /XRT observations during its 2015 outburst. The…