Zobrazeno 1 - 10
of 13
pro vyhledávání: '"Narayana P. Bhat"'
Autor:
Samuele Ronchini, Suman Bala, Joshua Wood, James Delaunay, Simone Dichiara, Jamie A. Kennea, Tyler Parsotan, Gayathri Raman, Aaron Tohuvavohu, Naresh Adhikari, Narayana P. Bhat, Sylvia Biscoveanu, Elisabetta Bissaldi, Eric Burns, Sergio Campana, Koustav Chandra, William H. Cleveland, Sarah Dalessi, Massimiliano De Pasquale, Juan García-Bellido, Claudio Gasbarra, Misty M. Giles, Ish Gupta, Dieter Hartmann, Boyan A. Hristov, Michelle C. Hui, Rahul Kashyap, Daniel Kocevski, Bagrat Mailyan, Christian Malacaria, Hiroyuki Nakano, Giacomo Principe, Oliver J. Roberts, Bangalore Sathyaprakash, Lijing Shao, Eleonora Troja, Péter Veres, Colleen A. Wilson-Hodge
Publikováno v:
The Astrophysical Journal Letters, Vol 970, Iss 1, p L20 (2024)
GW230529 is the first compact binary coalescence detected by the LIGO–Virgo–KAGRA collaboration with at least one component mass confidently in the lower mass gap, corresponding to the range 3–5 M _⊙ . If interpreted as a neutron star–black
Externí odkaz:
https://doaj.org/article/a19fdd384d7c4f4db662851ceea76952
Autor:
Majda K. Suleiman, Kingsley Dixon, Lucy Commander, Paul Nevill, Ali M. Quoreshi, Narayana R. Bhat, Anitha J. Manuvel, Mini T. Sivadasan
Publikováno v:
Frontiers in Microbiology, Vol 10 (2019)
This research examined the general soil fungi and AM fungal communities associated with a Lonely Tree species (Vachellia pachyceras) existing in the Sabah Al-Ahmad Natural Reserve located at the Kuwait desert. The goals of the study were to describe
Externí odkaz:
https://doaj.org/article/bb0ccfa61e59473da6bbad7bf0e24231
Autor:
Maryla Wasiolek, Narayana P. Bhat, Biswajit Ray, Preeti Kumari, Khalid Hattar, Umeshwarnath Surendranathan
Publikováno v:
IEEE Transactions on Nuclear Science. 69:478-484
Autor:
Maryla Wasiolek, Biswajit Ray, Narayana P. Bhat, Umeshwarnath Surendranathan, Khalid Hattar, Preeti Kumari
Publikováno v:
IEEE Transactions on Nuclear Science. 68:1032-1039
In this article, we have evaluated the Read-Retry (RR) functionality of the 3-D NAND chip of multilevel-cell (MLC) configuration after total ionization dose (TID) exposure. The RR function is typically offered in the high-density state-of-the-art NAN
Observing gravitationally lensed objects in the time domain is difficult, and well-observed time-varying sources are rare. Lensed gamma-ray bursts (GRBs) offer improved timing precision to this class of objects complementing observations of quasars a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::050034e6baf0ace294f24fe6c189d9b2
http://arxiv.org/abs/2110.06065
http://arxiv.org/abs/2110.06065
Autor:
A. J. Castro-Tirado, Narayana P. Bhat, Bing Zhang, Liang Li, Asaf Pe'er, Felix Ryde, David Alexander Kann, K. L. Page, Sylvain Guiriec, Yu Wang, Peter Vereš, Magnus Axelsson
Gamma-ray bursts (GRBs) are the most powerful explosions in the universe. The composition of the jets is, however, subject to debate\cite{Peer2015,Zhang2018}. Whereas the traditional model invokes a relativistic matter-dominated fireball with a brigh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dbcad07a83fa8d8a7f338b528824c347
https://doi.org/10.21203/rs.3.rs-231408/v1
https://doi.org/10.21203/rs.3.rs-231408/v1
Analytical modeling of pulse-pileup distortion using the true pulse shape; applications to Fermi-GBM
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 717:21-36
Pulse-pileup affects most photon counting systems and occurs when photon detections occur faster than the detector's registration and recovery time. At high input rates, shaped pulses interfere and the source spectrum, as well as intensity informatio
Autor:
Narayana P. Bhat
Publikováno v:
EAS Publications Series. 61:45-52
Gamma-ray bursts (GRB) are extremely energetic events and produce highly diverse light curves. Light curves are believed to be resulting from internal shocks reflecting the activities of the GRB central engine. Hence their temporal studies can potent
A characteristic energy of individual gamma-ray burst (GRB) spectra can in most cases be determined from the peak energy of the energy density spectra ($\nu{\cal F}_{\nu}$), called '$E_{\rm peak}$'. Distributions of $E_{\rm peak}$ have been compiled
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1f53afd1393dd4a38df381820fcd21e3
Autor:
A. von Kienlin, Narayana P. Bhat, Robert B. Wilson, Valerie Connaughton, Helmut Steinle, G. G. Lichti, Michael S. Briggs, Chryssa Kouveliotou, Charles A. Meegan, W. S. Paciesas, R. M. Kippen, Roland Diehl, Gerald J. Fishman, Jochen Greiner, Robert D. Preece
Publikováno v:
Chinese Journal of Astronomy and Astrophysics. 6:365-368
The next large NASA mission in the field of γ-ray astronomy is the Gamma-Ray Large Area Space Telescope (GLAST), which is scheduled for a launch end of 2007. This satellite consists of the main instrument LAT (Large-Area Telescope) which is sensitiv