Zobrazeno 1 - 10
of 946
pro vyhledávání: '"Seetha, S."'
HD 12098 is an roAp star pulsating in the most distorted dipole mode yet observed in this class of star. Using TESS Sector 58 observations we show that there are photometric spots at both the magnetic poles of this star. It pulsates obliquely primari
Externí odkaz:
http://arxiv.org/abs/2402.06314
Publikováno v:
Technologies, Vol 11, Iss 5, p 130 (2023)
The academic and research communities are showing significant interest in the modern and highly promising technology of wireless mesh networks (WMNs) due to their low-cost deployment, self-configuration, self-organization, robustness, scalability, an
Externí odkaz:
https://doaj.org/article/0562b90dba094e429569598386de84cd
Autor:
Rao, A. R., Chand, Vikas, Hingar, M. K., Iyyani, S., Khanna, Rakesh, Kutty, A. P. K., Malkar, J. P., Paul, D., Bhalerao, V. B., Bhattacharya, D., Dewangan, G. C., Pawar, Pramod, Vibhute, A. M., Chattopadhyay, T., Mithun, N. P. S., Vadawale, S. V., Vagshette, N., Basak, R., Pradeep, P., Samuel, Essy, Sreekumar, S., Vinod, P., Navalgund, K. H., Pandiyan, R., Sarma, K. S., Seetha, S., Subbarao, K.
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
Externí odkaz:
http://arxiv.org/abs/1608.07388
Autor:
Rao, A. R., Patil, M. H., Bhargava, Yash, Khanna, Rakesh, Hingar, M. K., Kutty, A. P. K., Malkar, J. P., Basak, Rupal, Sreekumar, S., Samuel, Essy, Priya, P., Vinod, P., Bhattacharya, D., Bhalerao, V., Vadawale, S. V., Mithun, N. P. S., Pandiyan, R., Subbarao, K., Seetha, S., Sarma, K. Suryanarayana
Charged Particle Monitor (CPM) on-board the AstroSat satellite is an instrument designed to detect the flux of charged particles at the satellite location. A Cesium Iodide Thallium (CsI(Tl)) crystal is used with a Kapton window to detect protons with
Externí odkaz:
http://arxiv.org/abs/1608.06038
Autor:
Bhalerao, V., Bhattacharya, D., Vibhute, A., Pawar, P., Rao, A. R., Hingar, M. K., Khanna, Rakesh, Kutty, A. P. K., Malkar, J. P., Patil, M. H., Arora, Y. K., Sinha, S., Priya, P., Samuel, Essy, Sreekumar, S., Vinod, P., Mithun, N. P. S., Vadawale, S. V., Vagshette, N., Navalgund, K. H., Sarma, K. S., Pandiyan, R., Seetha, S., Subbarao, K.
The Cadmium Zinc Telluride Imager (CZTI) is a high energy, wide-field imaging instrument on AstroSat. CZT's namesake Cadmium Zinc Telluride detectors cover an energy range from 20 keV to > 200 keV, with 11% energy resolution at 60 keV. The coded aper
Externí odkaz:
http://arxiv.org/abs/1608.03408
In this paper, we attempt to find out the `spectro-temporal' characteristics during the jet ejection, of several outbursting Galactic black hole sources based on RXTE-PCA/HEXTE data in the energy band of 2 - 100 keV. We present results of detailed an
Externí odkaz:
http://arxiv.org/abs/1605.08351
We study the variations in the Cyclotron Resonant Scattering Feature (CRSF) during 2011 outburst of the high mass X-ray binary 4U 0115+63 using observations performed with Suzaku, RXTE, Swift and INTEGRAL satellites. The wide-band spectral data with
Externí odkaz:
http://arxiv.org/abs/1506.03376
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 3/30/2024, Vol. 529 Issue 1, p556-562, 7p
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We present the results of analysis of the X-ray transient source MAXI J1836-194 during its outburst in August 2011. MAXI GSC detected the source on 30th August 2011, when it started rising from the quiescence. We have studied the source using the obs
Externí odkaz:
http://arxiv.org/abs/1401.1135