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pro vyhledávání: '"Navale, Nilam"'
Autor:
Navale, Nilam R., Pawar, Devraj, Rao, A. R., Misra, Ranjeev, Chakraborty, Sudip, Bhattacharyya, Sudip, Bambole, Vaishali A.
XB 1254-690 is a neutron star low-mass X-ray binary with an orbital period of 3.88 hrs, and it exhibits energy-dependent intensity dips, thermonuclear bursts, and flares. We present the results of an analysis of a long observation of this source usin
Externí odkaz:
http://arxiv.org/abs/2407.05371
Autor:
Vaishnava, C. S., Mithun, N. P. S., Vadawale, Santosh V., Aarthy, Esakkiappan, Patel, Arpit R., Adalja, Hiteshkumar L., Tiwari, Neeraj Kumar, Ladiya, Tinkal, Navale, Nilam, Chattopadhyay, Tanmoy, Rao, A. R., Bhalerao, Varun, Bhattacharya, Dipankar
The Cadmium Zinc Telluride Imager (CZTI) onboard AstroSat consists of an array of a large number of pixellated CZT detectors capable of measuring the polarization of incident hard X-rays. The polarization measurement capability of CZTI for on-axis so
Externí odkaz:
http://arxiv.org/abs/2209.00222
MAXI J1820+070 is a newly discovered transient black hole X-ray binary, which showed several spectral and temporal features. In this work, we analyse the broadband X-ray spectra from all three simultaneously observing X-ray instruments onboard AstroS
Externí odkaz:
http://arxiv.org/abs/2009.02465
Autor:
Pandge, M. B., Bagchi, Joydeep, Sonkamble, S. S., Parekh, Viral, Patil, M. K., Dabhade, Pratik, Navale, Nilam R, Raychaudhury, Somak, Joe, Jacob
Publikováno v:
MNRAS, 472, 2017, 2042-2053
We present a detailed analysis of a young merging galaxy cluster \mac~(z=0.43), from {\it Chandra} X-ray and {\it Hubble Space Telescope} archival data. X-ray observations confirm that the X-ray emitting intra-cluster medium (ICM) in this system is a
Externí odkaz:
http://arxiv.org/abs/1701.00197
Autor:
Navale, Nilam R, Pawar, Devraj, Rao, A R, Misra, Ranjeev, Chakraborty, Sudip, Bhattacharyya, Sudip, Bambole, Vaishali A
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Aug2024, Vol. 532 Issue 3, p2955-2964, 10p
Autor:
Raghav, Anil, Bhaskar, Ankush, Yadav, Virendra, Bijewar, Nitinkumar, Pai, Chintamani, Koli, Ashish, Navale, Nilam, Singh, Gurinderpal, Dubey, Nitin, Pawar, Sushant, Parab, Pradnya, Narvankar, Gandhali, Rawoot, Vaibhav, Rawat, Vikas, Borse, Satish, Garad, Nagnath, Rozario, Carl, Kaushal, Nitin, Tiwari, Shailendrakumar, Press, M. R.
Temporal variation of secondary cosmic rays (SCR) flux was measured during the total lunar eclipse on December 10, 2011 and the subsequent full moon on January 8, 2012. The measurements were done at Department of Physics, University of Mumbai, Mumbai
Externí odkaz:
http://arxiv.org/abs/1212.4240
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Akademický článek
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