Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Debdutta Paul"'
Autor:
Ajay Ratheesh, A. R. Rao, S. Sreekumar, Santosh V. Vadawale, A. Vibhute, P. Pradeep, Debdutta Paul, Dipankar Bhattacharya, N. P. S. Mithun
The Cadmium Zinc Telluride (CZT) Imager onboard AstroSat, consists of pixelated CZT detectors, which are sensitive to hard X-rays above 20 keV. The individual pixels are triggered by ionising events occurring in them, and the detectors operate in a s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::49b1e526fcf4492a2af5fe13a51db8cc
http://arxiv.org/abs/1912.03547
http://arxiv.org/abs/1912.03547
Autor:
Debdutta Paul
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 477:4275-4284
The luminosity function of short Gamma Ray Bursts (GRBs) is modelled by using the available catalogue data of all short GRBs (sGRBs) detected till October, 2017. The luminosities are estimated via the `pseudo-redshifts' obtained from the `Yonetoku co
Autor:
Debdutta Paul
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 473:3385-3393
I have used a sample of long Gamma Ray Bursts (GRBs) common to both \emph{Swift} and \emph{Fermi} to re-derive the parameters of the Yonetoku correlation. This allowed me to self-consistently estimate pseudo redshifts of all the bursts with unknown r
Autor:
Debdutta Paul
Publikováno v:
Scopus-Elsevier
Debdutta Paul
Debdutta Paul
Gamma-ray bursts (GRBs) are transients associated with the formation of compact objects. It had long been theorised that mergers of two neutron stars leading to the formation of a heavier neutron star or a black hole are the progenitors of the so-cal
We study the angular dependence of the flux from partially synchrotron self-absorbed conical jets (proposed by Blandford \& K{\"o}nigl). We consider the jet viewed from either a side or close to on axis, and in the latter case, either from the jet to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8cf3f638be0aa20553a1651b3a1c281d
http://arxiv.org/abs/1606.03428
http://arxiv.org/abs/1606.03428
Autor:
Debdutta Paul, A. P. K. Kutty, Tanmoy Chattopadhyay, R. Pandiyan, A. R. Rao, N. P. S. Mithun, Gulab C. Dewangan, S. Seetha, Varun Bhalerao, P. K. Pawar, K. Subbarao, S. Sreekumar, P. Pradeep, N. D. Vagshette, A. Vibhute, P. Vinod, Vikas Chand, Rakesh Khanna, Dipankar Bhattacharya, M. K. Hingar, J. P. Malkar, Rupal Basak, Essy Samuel, Santosh V. Vadawale, K. H. Navalgund, K. S. Sarma, Shabnam Iyyani
Publikováno v:
The Astrophysical Journal. 833:86
AstroSat is a multi-wavelength satellite launched on 2015 September 28. The CZT Imager of AstroSat on its very first day of operation detected a long duration gamma-ray burst (GRB) namely GRB 151006A. Using the off-axis imaging and spectral response