Zobrazeno 1 - 10
of 95
pro vyhledávání: '"Maan, Yogesh"'
Repeating fast radio bursts can exhibit a wide range of burst repetition rates, from none to hundreds of bursts per hour. Here, we report the detection and characteristics of 57 bursts from the recently discovered FRB 20240114A, observed with GMRT in
Externí odkaz:
http://arxiv.org/abs/2406.12804
Autor:
Pastor-Marazuela, Inés, van Leeuwen, Joeri, Bilous, Anna, Connor, Liam, Maan, Yogesh, Oostrum, Leon, Petroff, Emily, Vohl, Dany, Hess, Kelley M., Orrù, Emanuela, Sclocco, Alessio, Wang, Yuyang
Understanding the origin of fast radio bursts (FRBs) has become the main science driver of recent dedicated FRB surveys. Between July 2019 and February 2022, we carried out ALERT, an FRB survey at 1370 MHz using the Apertif instrument installed at th
Externí odkaz:
http://arxiv.org/abs/2406.00482
Autor:
Paladi, Avinash Kumar, Dwivedi, Churchil, Rana, Prerna, K, Nobleson, Susobhanan, Abhimanyu, Joshi, Bhal Chandra, Tarafdar, Pratik, Deb, Debabrata, Arumugam, Swetha, Gopakumar, A, Krishnakumar, M A, Batra, Neelam Dhanda, Debnath, Jyotijwal, Kareem, Fazal, Arumugam, Paramasivan, Bagchi, Manjari, Bathula, Adarsh, Dandapat, Subhajit, Desai, Shantanu, Gupta, Yashwant, Hisano, Shinnosuke, Kharbanda, Divyansh, Kikunaga, Tomonosuke, Kolhe, Neel, Maan, Yogesh, Manoharan, P K, Singha, Jaikhomba, Srivastava, Aman, Surnis, Mayuresh, Takahashi, Keitaro
The wideband timing technique enables the high-precision simultaneous estimation of pulsar Times of Arrival (ToAs) and Dispersion Measures (DMs) while effectively modeling frequency-dependent profile evolution. We present two novel independent method
Externí odkaz:
http://arxiv.org/abs/2304.13072
Autor:
Srivastava, Aman, Desai, Shantanu, Kolhe, Neel, Surnis, Mayuresh, Joshi, Bhal Chandra, Susobhanan, Abhimanyu, Chalumeau, Aurélien, Hisano, Shinnosuke, K., Nobleson, Arumugam, Swetha, Kharbanda, Divyansh, Singha, Jaikhomba, Tarafdar, Pratik, Arumugam, P, Bagchi, Manjari, Bathula, Adarsh, Dandapat, Subhajit, Dey, Lankeswar, Dwivedi, Churchil, Girgaonkar, Raghav, Gopakumar, A., Gupta, Yashwant, Kikunaga, Tomonosuke, Krishnakumar, M. A., Liu, Kuo, Maan, Yogesh, Manoharan, P K, Paladi, Avinash Kumar, Rana, Prerna, Shaifullah, Golam M., Takahashi, Keitaro
The Indian Pulsar Timing Array (InPTA) collaboration has recently made its first official data release (DR1) for a sample of 14 pulsars using 3.5 years of uGMRT observations. We present the results of single-pulsar noise analysis for each of these 14
Externí odkaz:
http://arxiv.org/abs/2303.12105
Autor:
Joshi, Bhal Chandra, Gopakumar, Achamveedu, Pandian, Arul, Prabu, Thiagaraj, Dey, Lankeswar, Bagchi, Manjari, Desai, Shantanu, Tarafdar, Pratik, Rana, Prerna, Maan, Yogesh, Batra, Neelam Dhanda, Girgaonkar, Raghav, Agarwal, Nikita, Arumugam, Paramasivan, Banik, Sarmistha, Basu, Avishek, Bathula, Adarsh, Dandapat, Subhajit, Gupta, Yashwant, Hisano, Shinnosuke, Kato, Ryo, Kharbanda, Divyansh, Kikunaga, Tomonosuke, Kolhe, Neel, Krishnakumar, M. A., Manoharan, P. K., Marmat, Piyush, Naidu, Arun, Nobleson, K., Paladi, Avinash Kumar, Pathak, Dhruv, Singha, Jaikhomba, Srivastava, Aman, Surnis, Mayuresh, Susarla, Sai Chaitanya, Susobhanan, Abhimanyu, Takahashi, Keitaro
Decades long monitoring of millisecond pulsars, which exhibit highly stable rotational periods, in pulsar timing array experiments is on the threshold of discovering nanohertz stochastic gravitational wave background. This paper describes the Indian
Externí odkaz:
http://arxiv.org/abs/2207.06461
Autor:
Tarafdar, Pratik, K., Nobleson, Rana, Prerna, Singha, Jaikhomba, Krishnakumar, M. A., Joshi, Bhal Chandra, Paladi, Avinash Kumar, Kolhe, Neel, Batra, Neelam Dhanda, Agarwal, Nikita, Bathula, Adarsh, Dandapat, Subhajit, Desai, Shantanu, Dey, Lankeswar, Hisano, Shinnosuke, Ingale, Prathamesh, Kato, Ryo, Kharbanda, Divyansh, Kikunaga, Tomonosuke, Marmat, Piyush, Pandian, B. Arul, Prabu, T., Srivastava, Aman, Surnis, Mayuresh, Susarla, Sai Chaitanya, Susobhanan, Abhimanyu, Takahashi, Keitaro, Arumugam, P., Bagchi, Manjari, Banik, Sarmistha, De, Kishalay, Girgaonkar, Raghav, Gopakumar, A., Gupta, Yashwant, Maan, Yogesh, Manoharan, P. K., Naidu, Arun, Pathak, Dhruv
Publikováno v:
Publications of the Astronomical Society of Australia, Volume 39, 2022, e053
We present the pulse arrival times and high-precision dispersion measure estimates for 14 millisecond pulsars observed simultaneously in the 300-500 MHz and 1260-1460 MHz frequency bands using the upgraded Giant Metrewave Radio Telescope (uGMRT). The
Externí odkaz:
http://arxiv.org/abs/2206.09289
Autor:
Szary, Andrzej, van Leeuwen, Joeri, Wright, Geoff, Weltevrede, Patrick, Agar, Crispin H., Tiburzi, Caterina, Maan, Yogesh, Keith, Michael J.
We present an analysis of the subpulse drift in PSR J1750-3503, which is characterized by abrupt transitions of drift direction. As the pulsar does not exhibit other mode changes or clear nulling, it is an ideal candidate system for studying the phen
Externí odkaz:
http://arxiv.org/abs/2206.02382
Autor:
van Leeuwen, Joeri, Kooistra, Eric, Oostrum, Leon, Connor, Liam, Hargreaves, J. E., Maan, Yogesh, Pastor-Marazuela, Inés, Petroff, Emily, van der Schuur, Daniel, Sclocco, Alessio, Straal, Samayra M., Vohl, Dany, Wijnholds, Stefan J., Adams, Elizabeth A. K., Adebahr, Björn, Attema, Jisk, Bassa, Cees, Bast, Jeanette E., Bilous, Anna, de Blok, W. J. G., Boersma, Oliver M., van Cappellen, Wim A., Coolen, Arthur H. W. M., Damstra, Sieds, Dénes, Helga, van Diepen, Ger N. J., Gardenier, David W., Grange, Yan G., Gunst, André W., Hess, Kelley M., Holties, Hanno, van der Hulst, Thijs, Hut, Boudewijn, Kutkin, Alexander, Loose, G. Marcel, Lucero, Danielle M., Mika, Ágnes, Mikhailov, Klim, Morganti, Raffaella, Moss, Vanessa A., Mulder, Henk, Norden, Menno J., Oosterloo, Tom A., Orrú, Emaneula, Paragi, Zsolt, de Reijer, Jan-Pieter R., Schoenmakers, Arno P., Stuurwold, Klaas J. C., ter Veen, Sander, Wang, Yu-Yang, Zanting, Alwin W., Ziemke, Jacob
Publikováno v:
A&A 672, A117 (2023)
Fast Radio Bursts must be powered by uniquely energetic emission mechanisms. This requirement has eliminated a number of possible source types, but several remain. Identifying the physical nature of Fast Radio Burst (FRB) emitters arguably requires g
Externí odkaz:
http://arxiv.org/abs/2205.12362
Autor:
Pastor-Marazuela, Inés, van Leeuwen, Joeri, Bilous, Anna, Connor, Liam, Maan, Yogesh, Oostrum, Leon, Petroff, Emily, Straal, Samayra, Vohl, Dany, Adams, E. A. K., Adebahr, B., Attema, Jisk, Boersma, Oliver M., Brink, R. van den, van Cappellen, W. A., Coolen, A. H. W. M., Damstra, S., Dénes, H., Hess, K. M., van der Hulst, J. M., Hut, B., Kutkin, A., Loose, G. Marcel, Lucero, D. M., Mika, Á., Moss, V. A., Mulder, H., Norden, M. J., Oosterloo, T. A., Rajwade, Kaustubh, van der Schuur, D., Sclocco, A., Smits, R., Ziemke, J.
Publikováno v:
A&A 678, A149 (2023)
Fast radio bursts (FRBs) are extragalactic radio transients of extraordinary luminosity. Studying the diverse temporal and spectral behaviour recently observed in a number of FRBs may help determine the nature of the entire class. For example, a fast
Externí odkaz:
http://arxiv.org/abs/2202.08002
We present the long-term spectro-temporal evolution of the average radio emission properties of the magnetar XTE J1810-197 (PSR J1809-1943) following its most recent outburst in late 2018. We report the results from two and a half years of monitoring
Externí odkaz:
http://arxiv.org/abs/2201.13006