Zobrazeno 1 - 10
of 132
pro vyhledávání: '"MUKERJEE, K."'
Autor:
Chaudhury, K., Chitnis, V. R., Rao, A. R., Singh, K. P., Bhattacharyya, Sudip, Dewangan, G. C., Chakraborty, S., Chandra, S., Stewart, G. C., Mukerjee, K., Dey, R. K.
Publikováno v:
MNRAS, Volume 478, Issue 4, Pages 4830-4836, 2018
We present the results of our study of the long term X-ray variability characteristics of the Narrow Line Seyfert 1 galaxy RE J1034+396. We use data obtained from the AstroSat satellite along with the light curves obtained from XMM-Newton and Swift-X
Externí odkaz:
http://arxiv.org/abs/1807.06460
Autor:
Bhargava, Yash, Rao, A. R., Singh, K. P., Choudhury, Manojendu, Bhattacharyya, S., Chandra, S., Dewangan, G. C., Mukerjee, K., Stewart, G. C., Bhattacharya, D., Mithun, N. P. S., Vadawale, S. V.
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 stability over the past 45 years and we find that we can use this infor
Externí odkaz:
http://arxiv.org/abs/1709.07441
Autor:
Martin-Carrillo, A., Kirsch, M. G. F., Caballero, I., Freyberg, M. J., Ibarra, A., Kendziorra, E., Lammers, U., Mukerjee, K., Schönherr, G., Stuhlinger, M., Saxton, R. D., Staubert, R., Suchy, S., Wellbrock, A., Webb, N., Guainazzi, M.
Reliable timing calibration is essential for the accurate comparison of XMM-Newton light curves with those from other observatories, to ultimately use them to derive precise physical quantities. The XMM-Newton timing calibration is based on pulsar an
Externí odkaz:
http://arxiv.org/abs/1204.0978
Autor:
Kirsch, M. G. F., Schoenherr, G., Kendziorra, E., Freyberg, M. J., Martin, M., Wilms, J., Mukerjee, K., Breitfellner, M. G., Smith, M. J. S., Staubert, R.
We discuss the current X-ray view of the Crab Nebula and Pulsar, summarising our analysis of observations of the source with the EPIC-pn camera on board the XMM-Newton observatory. Different modes of EPIC-pn were combined in order to yield a complete
Externí odkaz:
http://arxiv.org/abs/astro-ph/0604097
Autor:
Burrows, David N., Hill, J. E., Nousek, J. A., Kennea, J. A., Wells, A., Osborne, J. P., Abbey, A. F., Beardmore, A., Mukerjee, K, Short, A. D. T., Chincarini, G., Campana, S., Citterio, O., Moretti, A., Pagani, C., Tagliaferri, G., Giommi, P., Capalbi, M., Tamburelli, F., Angelini, L., Cusumano, G., Braeuninger, H. W., Burkert, W., Hartner, G. D.
Publikováno v:
SpaceSci.Rev.120:165,2005
The Swift Gamma-Ray Explorer is designed to make prompt multiwavelength observations of Gamma-Ray Bursts (GRBs) and GRB afterglows. The X-ray Telescope (XRT) enables Swift to determine GRB positions with a few arcseconds accuracy within 100 seconds o
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508071
Autor:
Sembay, S., Abbey, A., Altieri, B., Ambrosi, R., Baskill, D., Ferrando, P., Mukerjee, K., Read, A., Turner, M. J. L.
XMM-Newton was launched into space on a highly eccentric 48 hour orbit on December 10th 1999. XMM-Newton is now in its fifth year of operation and has been an outstanding success, observing the Cosmos with imaging, spectroscopy and timing capabilitie
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407347
Autor:
Kirsch, M. G. F., Mukerjee, K., Breitfellner, M. G., Djavidnia, S., Freyberg, M. J., Kendziorra, E., Smith, M. J. S.
Publikováno v:
Astron.Astrophys. 423 (2004) L9-L12
The accreting millisecond pulsar XTE J1807-294 was observed by XMM-Newton on March 22, 2003 after its discovery on February 21, 2003 by RXTE. The source was detected in its bright phase with an observed average count rate of 33.3 cts/s in the EPIC-pn
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407017
Hard X-ray light curves and spectral parameters from our analysis of X-ray data of five AM Her type systems - V2301 Oph, V1432 Aql, EP Draconis, GG Leonis, V834 Cen, and one intermediate polar - TV Col, observed using the Rossi X-ray Timing Explorer
Externí odkaz:
http://arxiv.org/abs/astro-ph/0302073
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Akademický článek
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