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pro vyhledávání: '"MANCHANDA, R"'
We present an improved background model for the Large Area X-ray Proportional Counter (LAXPC) detectors on-board AstroSat. Because of the large collecting area and high pressure, the LAXPC instrument has a large background count rate, which varies du
Externí odkaz:
http://arxiv.org/abs/2205.03136
Autor:
Yadav, J. S., Agrawal, P. C., Misra, Ranjeev, Roy, Jayashree, Pahari, Mayukh, Manchanda, R. K.
With its large effective area at hard X-rays, high time resolution and having co-aligned other instruments, AstroSat/LAXPC was designed to usher in a new era in rapid variability studies and wide spectral band measurements of the X-ray binaries. Over
Externí odkaz:
http://arxiv.org/abs/2102.06465
Autor:
Antia, H. M., Agrawal, P. C., Dedhia, Dhiraj, Katoch, Tilak, Manchanda, R. K., Misra, Ranjeev, Mukerjee, Kallol, Pahari, Mayukh, Roy, Jayashree, Shah, P., Yadav, J. S.
The Large Area X-ray Proportional Counter (LAXPC) instrument on-board AstroSat has three nominally identical detectors for timing and spectral studies in the energy range of 3--80 keV. The performance of these detectors during the five years after th
Externí odkaz:
http://arxiv.org/abs/2101.07514
Akademický článek
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Akademický článek
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Autor:
Roy, Jayashree, Agrawal, P. C., Iyer, N. K., Bhattacharya, D., Yadav, J. S., Antia, H. M., Chauhan, J. V., Choudhury, M., Dedhia, D. K., Katoch, T., Madhavani, P., Manchanda, R. K., Misra, R., Pahari, M., Paul, B., Shah, P.
The Be X-ray Binary 4U 0115+63 was observed by Large Area X-ray Proportional Counter (LAXPC) instrument on AstroSat on 2015 October 24 during the peak of a giant Type II outburst. Prominent intensity oscillations at ~ 1 and ~ 2 mHz frequency were det
Externí odkaz:
http://arxiv.org/abs/1901.09382
Autor:
Beri, Aru, Paul, Biswajit, Yadav, J S, Antia, H M, Agrawal, P C, Manchanda, R. K, Dedhia, Dhiraj, Chauhan, Jai Verdhan, Pahari, Mayukh, Misra, Ranjeev, Katoch, Tilak, Madhwani, P., Shah, Parag, Varun, Mate, Sujay
We present results from an observation of the Low Mass X-ray Binary 4U 1636-536 obtained with the LAXPC instrument aboard AstroSat. The observations of 4U 1636-536 made during the performance verification phase of AstroSat showed seven thermonuclear
Externí odkaz:
http://arxiv.org/abs/1811.10030
Autor:
Rawat, Divya, Pahari, Mayukh, Yadav, J S, Jain, Pankaj, Misra, Ranjeev, Bagri, Kalyani, Katoch, Tilak, Agrawal, P C, Manchanda, R K
In this work, we present a $\sim$90 ks continuous monitoring of the Galactic micro-quasar GRS 1915+105 with AstroSat when the source undergoes a major transition from a non-variable, $\chi$ class (similar to radio-quiet $\chi$ class) to a structured,
Externí odkaz:
http://arxiv.org/abs/1811.03393
Autor:
Bhattacharyya, Sudip, Yadav, J. S., Sridhar, Navin, Chauhan, Jai Verdhan, Agrawal, P. C., Antia, H. M., Pahari, Mayukh, Misra, Ranjeev, Katoch, Tilak, Manchanda, R. K., Paul, Biswajit
It has recently been shown that the persistent emission of a neutron star low-mass X-ray binary (LMXB) evolves during a thermonuclear (type-I) X-ray burst. The reason of this evolution, however, is not securely known. This uncertainty can introduce s
Externí odkaz:
http://arxiv.org/abs/1805.05393
Autor:
Levenback, C.F., Hermans, R.H., Bouda, J., Sharma, A., Luesley, D., Ellis, P., Cruickshank, D.J., Duncan, T.J., Kieser, K., Palle, C., Spirtos, N.M., O'Malley, D.M., Leitao, M.M., Geller, M., Dhar, K., Asher, V., Tobias, D.H., Borgfeldt, C., Lea, J.S., Lood, M., Bailey, J., Eyjolfsdottir, B., Attard-Montalto, S., Tewari, K.S., Persson, P., Manchanda, R., Jensen, P., Van Le, L., Van der Kolk, W.L., Van der Zee, A.G.J., Slomovitz, B.M., Baldwin, P.J.W., Van Doorn, H.C., De Hullu, J.A., Van der Velden, J., Gaarenstroom, K.N., Slangen, B.F.M., Kjolhede, P., Brännström, M., Vergote, I., Holland, C.M., Coleman, R., Van Dorst, E.B.L., Van Driel, W.J., Nunns, D., Widschwendter, M., Nugent, D., DiSilvestro, P.A., Mannel, R.S., Tjiong, M.Y., Boll, D., Cibula, D., Covens, A., Provencher, D., Runnebaum, I.B., Monk, B.J., Zanagnolo, V., Tamussino, K., Oonk, M.H.M.
Publikováno v:
In Gynecologic Oncology October 2022 167(1):3-10
