Zobrazeno 1 - 10
of 1 132
pro vyhledávání: '"Chitnis, V."'
Autor:
C., Borwankar, M., Sharma, J., Hariharan, K., Venugopal, S., Godambe, N., Mankuzhyil, P., Chandra, M., Khurana, A., Pathania, N., Chouhan, K., Dhar V., R., Thubstan, S., Norlha, Keshavananda, D., Sarkar, A., Dar Z., V., Kotwal S., S., Godiyal, P., Kushwaha C., K., Singh K., P., Das M., A., Tolamatti, B., Ghosal, K., Chanchalani, P., Pandey, N., Bhatt, S., Bhattcharyya, S., Sahayanathan, K., Koul M., P., Dorjey, N., Dorji, R., Chitnis V., K., Tickoo A., C., Rannot R., K, Yadav K.
Publikováno v:
Astroparticle Physics 159 (2024) 102960
The Major Atmospheric Cherenkov Experiment (MACE) is a large size (21m) Imaging Atmospheric Cherenkov Telescope (IACT) installed at an altitude of 4270m above sea level at Hanle, Ladakh in northern India. Here we report the detection of Very High Ene
Externí odkaz:
http://arxiv.org/abs/2404.01649
Autor:
Agarwal, S., Banerjee, B., Shukla, A., Roy, J., Acharya, S., Vaidya, B., Chitnis, V. R., Wagner, S. M., Mannheim, K., Branchesi, M.
The evolution of the spectral energy distribution during flares constrains models of particle acceleration in blazar jets. The archetypical blazar BL Lac provided a unique opportunity to study spectral variations during an extended strong flaring epi
Externí odkaz:
http://arxiv.org/abs/2302.07904
Publikováno v:
The European Physical Journal Special Topics (2022)
Very high energy {\gamma}-rays are one of the most important messengers of the non-thermal Universe. The major motivation of very high energy {\gamma}-ray astronomy is to find sources of high energy cosmic rays. Several astrophysical sources are know
Externí odkaz:
http://arxiv.org/abs/2201.06789
Publikováno v:
The European Physical Journal Special Topics (2022)
Very High Energy (VHE) gamma rays constitute one of the main pillars of high energy astrophysics. Gamma rays are produced under extreme relativistic conditions in the Universe. VHE gamma$ rays can be detected indirectly on the ground. Detection of th
Externí odkaz:
http://arxiv.org/abs/2201.04719
Autor:
HiGRO Collaboration, Bhatt, N, Bhattacharyya, S, Borwankar, C, Chanchalani, K, Chandra, P, Chitnis, V, Chouhan, N, Das, M P, Dhar, VK, Ghosal, B, Godambe, S, Godiyal, S, Gour, K K, Jayaraman, H, Khurana, M, Kothari, M, Kotwal, S, Koul, M K, Kumar, N, Kushwaha, C P, Mankuzhiyil, N, Marandi, P, Nand, K, Norlha, S, Sarkar, D, Sharma, M, Singh, K K, Thubstan, R, Tolamatti, A, Venugopal, K, Yadav, K K
MACE (Major Atmospheric Cherenkov Experiment), an imaging atmospheric Cherenkov telescope, has recently been installed by the HiGRO (Himalayan Gamma-Ray Observatory) collaboration at Hanle (32.8$^\circ$N, 78.9$^\circ$E, 4270m asl) in Ladakh region of
Externí odkaz:
http://arxiv.org/abs/2107.04297
Autor:
Sarkar, A., Chitnis, V. R., Gupta, A. C., Gaur, H., Patel, S. R., Wiita, P. J., Volvach, A. E., Tornikoski, M., Chamani, W., Enestam, S., Lähteenmäki, A., Tammi, J., Vera, R. J. C, Volvach, L. N.
We performed a long-term optical (B, V, R bands), infra-red (J and K bands) and radio band (15, 22, 37 GHz band) study on the flat spectrum radio quasar, 3C 454.3, using the data collected over a period of more than 8 years (MJD 54500--57500). The te
Externí odkaz:
http://arxiv.org/abs/1910.14329
Autor:
Singh, B. B., Britto, R. J., Chitnis, V. R., Shukla, A., Saha, L., Sinha, A., Acharya, B. S., Vishwanath, P. R., Anupama, G. C., Bhattacharjee, P., Gothe, K. S., Nagesh, B. K., Prabhu, T. P., Rao, S. K, Srinivasan, R., Upadhya, S. S.
HAGAR is a system of seven Non-imaging Atmospheric Cherenkov Telescopes located at Hanle in the Ladakh region of the Indian Himalayas at an altitude of 4270 meters {\it amsl}. Since 2008, we have observed the Crab Nebula to assess the performance of
Externí odkaz:
http://arxiv.org/abs/1902.01081
Autor:
Kumar, Sandeep, Upadhya, S.S., Gothe, K.S., Parmar, N.K., Ranjan, M., Rao, S.K., Nagesh, B.K., Singh, B.B., Chitnis, V., Acharya, B.S., Bhatnagar, V.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A April 2023 1049
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The TeV blazar Ton 599 has exhibited a peculiar flare in 2017 November. The temporal variation of the source is studied using simultaneous $\gamma$-ray data from $\textit{Fermi}$ Large Area Telescope and radio data from Owens Valley Radio Observatory
Externí odkaz:
http://arxiv.org/abs/1809.05269