Zobrazeno 1 - 10
of 7 948
pro vyhledávání: '"Sahu, A K"'
Autor:
Hou, Changshun, Zhai, Ziwei, Choudhury, Nilotpal, Harris, Tom, Sahu, Jayanta K., Nilsson, Johan
A thulium-doped fiber laser operating quasi-continuous-wave generated 198 W of instantaneous output power in 0.2-ms pulses at 50 Hz repetition rate. The duty cycle becomes 1% and the average output power 2.0 W. This was cladding-pumped with 408 W fro
Externí odkaz:
http://arxiv.org/abs/2412.01793
Autor:
Paul, Debjoty, Yadav, Shivesh, Gupta, Shikhar, Patra, Bikash, Kulkarni, Nilesh, Mondal, Debashis, Gavankar, Kaushal, Samanta, Saheli, Sahu, Sourav K., Satpati, Biswarup, Singh, Bahadur, Benton, Owen, Chatterjee, Shouvik
Applying strain to epitaxial thin films has proven to be an effective approach for controlling material properties, paving the way for "materials by design". In this study, we explore this concept in the context of topological Kagome antiferromagnets
Externí odkaz:
http://arxiv.org/abs/2411.01824
Autor:
Warwick, B., Lyman, J., Pursiainen, M., Coppejans, D. L., Galbany, L., Jones, G. T., Killestein, T. L., Kumar, A., Oates, S. R., Ackley, K., Anderson, J. P., Aryan, A., Breton, R. P., Chen, T. W., Clark, P., Dhillon, V. S., Dyer, M. J., Gal-Yam, A., Galloway, D. K., Gutiérrez, C. P., Gromadzki, M., Inserra, C., Jiménez-Ibarra, F., Kelsey, L., Kotak, R., Kravtsov, T., Kuncarayakti, H., Magee, M. R., Matilainen, K., Mattila, S., Müller-Bravo, T. E., Nicholl, M., Noysena, K., Nuttall, L. K., O'Brien, P., O'Neill, D., Pallé, E., Pessi, T., Petrushevska, T., Pignata, G., Pollacco, D., Ragosta, F., Ramsay, G., Sahu, A., Sahu, D. K., Singh, A., Sollerman, J., Stanway, E., Starling, R., Steeghs, D., Teja, R. S., Ulaczyk, K.
SN 2023tsz is a Type Ibn supernova (SNe Ibn) discovered in an extremely low-mass host. SNe Ibn are an uncommon subtype of stripped-envelope core-collapse SNe. They are characterised by narrow helium emission lines in their spectra and are believed to
Externí odkaz:
http://arxiv.org/abs/2409.14147
Autor:
Gangopadhyay, Anjasha, Dukiya, Naveen, Moriya, Takashi J, Tanaka, Masaomi, Maeda, Keiichi, Howell, D. Andrew, Singh, Mridweeka, Singh, Avinash, Sollerman, Jesper, Kawabata, Koji S, Brennan, Sean J, Pellegrino, Craig, Dastidar, Raya, Nakaoka, Tatsuya, Kawabata, Miho, Misra, Kuntal, Schulze, Steve, Chandra, Poonam, Taguchi, Kenta, Sahu, Devendra K, McCully, Curtis, Bostroem, K. Azalee, Gonzalez, Estefania Padilla, Newsome, Megan, Hiramatsu, Daichi, Takei, Yuki, Yamanaka, Masayuki, Tajitsu, Akito, Isogai, Keisuke
We present the long-term photometric and spectroscopic analysis of a transitioning SN~IIn/Ibn from $-$10.8 d to 150.7 d post $V$-band maximum. SN~2021foa shows prominent He {\sc i} lines comparable in strength to the H$\alpha$ line around peak, placi
Externí odkaz:
http://arxiv.org/abs/2409.02666
Autor:
Teja, Rishabh Singh, Goldberg, Jared A., Sahu, D. K., Anupama, G. C., Singh, Avinash, Swain, Vishwajeet, Bhalerao, Varun
We present detailed multi-band photometric and spectroscopic observations and analysis of a rare core-collapse supernova SN 2021wvw, that includes photometric evolution up to 250 d and spectroscopic coverage up to 100 d post-explosion. A unique event
Externí odkaz:
http://arxiv.org/abs/2407.13207
Autor:
Joshi, Arti, Catelan, Márcio, Scaringi, Simone, Schwope, Axel, Anupama, G. C., Rawat, Nikita, Sahu, Devendra K., Singh, Mridweeka, Dastidar, Raya, Subramanian, Rama Venkata, Rao, Srinivas M
We present the analysis of optical photometric and spectroscopic observations of two non-magnetic cataclysmic variables, namely CRTS J080846.2+313106 and V416 Dra. CRTS J080846.2+313106 has been found to vary with a period of 4.9116$\pm$0.0003 h, whi
Externí odkaz:
http://arxiv.org/abs/2407.07387
Autor:
Singh, Avinash, Teja, R. S., Moriya, T. J., Maeda, K., Kawabata, K. S., Tanaka, M., Imazawa, R., Nakaoka, T., Gangopadhyay, A., Yamanaka, M., Swain, V., Sahu, D. K., Anupama, G. C., Kumar, B., Anche, R. M., Sano, Y., Raj, A., Agnihotri, V. K., Bhalerao, V., Bisht, D., Bisht, M. S., Belwal, K., Chakrabarti, S. K., Fujii, M., Nagayama, T., Matsumoto, K., Hamada, T., Kawabata, M., Kumar, A., Kumar, R., Malkan, B. K., Smith, P., Sakagami, Y., Taguchi, K., Tominaga, N., Watanabe, A.
We present a detailed investigation of photometric, spectroscopic, and polarimetric observations of the Type II SN 2023ixf. Earlier studies have provided compelling evidence for a delayed shock breakout from a confined dense circumstellar matter (CSM
Externí odkaz:
http://arxiv.org/abs/2405.20989
Publikováno v:
MNRAS 528, 2024, 6176 - 6192
ASASSN-20hx, a.k.a AT2020ohl, is an ambiguous nuclear transient (ANT), which was discovered in the nearby galaxy NGC6297 by the All-Sky Automated Survey for Supernovae (ASAS-SN). We have investigated the evolution of AT2020ohl using a multi-wavelengt
Externí odkaz:
http://arxiv.org/abs/2405.16107
Autor:
Lin, Zheyu, Jiang, Ning, Wang, Tinggui, Kong, Xu, Li, Dongyue, He, Han, Wang, Yibo, Zhu, Jiazheng, Li, Wentao, Jiang, Ji-an, Singh, Avinash, Teja, Rishabh Singh, Sahu, D. K., Jin, Chichuan, Maeda, Keiichi, Huang, Shifeng
The unluckiest star orbits a supermassive black hole elliptically. Every time it reaches the pericenter, it shallowly enters the tidal radius and gets partially tidal disrupted, producing a series of flares. Confirmation of a repeated partial tidal d
Externí odkaz:
http://arxiv.org/abs/2405.10895
Autor:
Murai, Yuta, Tanaka, Masaomi, Kawabata, Miho, Taguchi, Kenta, Teja, Rishabh Singh, Nakaoka, Tatsuya, Maeda, Keiichi, Kawabata, Koji S., Nagao, Takashi, Moriya, Takashi J., Sahu, D. K., Anupama, G. C., Tominaga, Nozomu, Morokuma, Tomoki, Imazawa, Ryo, Inutsuka, Satoko, Isogai, Keisuke, Kasuga, Toshihiro, Kobayashi, Naoto, Kondo, Sohei, Maehara, Hiroyuki, Mori, Yuki, Niino, Yuu, Ogawa, Mao, Ohsawa, Ryou, Okumura, Shin-ichiro, Saito, Sei, Sako, Shigeyuki, Takahashi, Hidenori, Uno, Kohki, Yamanaka, Masayuki
We present photometric, spectroscopic and polarimetric observations of the intermediate-luminosity Type IIP supernova (SN) 2021gmj from 1 to 386 days after the explosion. The peak absolute V-band magnitude of SN 2021gmj is -15.5 mag, which is fainter
Externí odkaz:
http://arxiv.org/abs/2401.05837