Search for Very High-Energy Emission from the millisecond pulsar PSR J0218+4232

Autor: Acciari, V. A., Ansoldi, S., Antonelli, L. A., Engels, A. Arbet, Artero, M., Asano, K., Baack, D., Babić, A., Baquero, A., de Almeida, U. Barres, Barrio, J. A., Batković, I., González, J. Becerra, Bednarek, W., Bellizzi, L., Bernardini, E., Bernardos, M., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Biland, A., Blanch, O., Bonnoli, G., Bošnjak, Ž., Busetto, G., Carosi, R., Ceribella, G., Cerruti, M., Chai, Y., Chilingarian, A., Cikota, S., Colak, S. M., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., D'Amico, G., D'Elia, V., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Delfino, M., Delgado, J., Mendez, C. Delgado, Depaoli, D., Di Pierro, F., Di Venere, L., Espiñeira, E. Do Souto, Prester, D. Dominis, Donini, A., Dorner, D., Doro, M., Elsaesser, D., Ramazani, V. Fallah, Fattorini, A., Ferrara, G., Fonseca, M. V., Font, L., Fruck, C., Fukami, S., López, R. J. García, Garczarczyk, M., Gasparyan, S., Gaug, M., Giglietto, N., Giordano, F., Gliwny, P., Godinović, N., Green, J. G., Green, D., Hadasch, D., Hahn, A., Heckmann, L., Herrera, J., Hoang, J., Hrupec, D., Hütten, M., Inada, T., Inoue, S., Ishio, K., Iwamura, Y., Jiménez, I., Jormanainen, J., Jouvin, L., Kajiwara, Y., Karjalainen, M., Kerszberg, D., Kobayashi, Y., Kubo, H., Kushida, J., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Lombardi, S., Longo, F., López-Coto, R., López-Moya, M., López-Oramas, A., Loporchio, S., Fraga, B. Machado de Oliveira, Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Mariotti, M., Martínez, M., Mazin, D., Menchiari, S., Mender, S., Mićanović, S., Miceli, D., Miener, T., Minev, M., Miranda, J. M., Mirzoyan, R., Molina, E., Moralejo, A., Morcuende, D., Moreno, V., Moretti, E., Neustroev, V., Nigro, C., Nilsson, K., Nishijima, K., Noda, K., Nozaki, S., Ohtani, Y., Oka, T., Santos, J. Otero, Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Pavletić, L., Peñil, P., Perennes, C., Persic, M., Moroni, P. G. Prada, Prandini, E., Priyadarshi, C., Puljak, I., Rhode, W., Ribó, M., Rico, J., Righi, C., Rugliancich, A., Saha, L., Sahakyan, N., Saito, T., Sakurai, S., Satalecka, K., Saturni, F. G., Schleicher, B., Schmidt, K., Schweizer, T., Sitarek, J., Šnidarić, I., Sobczynska, D., Spolon, A., Stamerra, A., Strom, D., Strzys, M., Suda, Y., Surić, T., Takahashi, M., Tavecchio, F., Temnikov, P., Terzić, T., Teshima, M., Tosti, L., Truzzi, S., Tutone, A., Ubach, S., van Scherpenberg, J., Vanzo, G., Acosta, M. Vazquez, Ventura, S., Verguilov, V., Vigorito, C. F., Vitale, V., Vovk, I., Will, M., Wunderlich, C., Zarić, D., Caraveo, P. A., Cognard, I., Guillemot, L., Harding, A. K., Li, J., Limyansky, B., Ng, C. Y., Torres, D. F., Parkinson, P. M. Saz

PSR J0218+4232 is one of the most energetic millisecond pulsars known and has long been considered as one of the best candidates for very high-energy (VHE; >100 GeV) gamma-ray emission. Using 11.5 years of Fermi Large Area Telescope (LAT) data betwee

Externí odkaz: http://arxiv.org/abs/2108.11373

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Proper motion, spectra, and timing of PSR J1813–1749 using Chandra and NICER.

Autor: Ho, Wynn C G, Guillot, Sebastien, Saz Parkinson, P M, Limyansky, B, Ng, C-Y, Bejger, Michał, Espinoza, Cristóbal M, Haskell, B, Jaisawal, Gaurava K, Malacaria, C

Publikováno v: Monthly Notices of the Royal Astronomical Society; Nov2020, Vol. 498 Issue 3, p4396-4403, 8p

Gamma Ray Pulsars and Opportunities for the MACE Telescope.

Autor: Pathania, Atul, Singh, Krishna Kumar, Yadav, Kuldeep Kumar

Publikováno v: Galaxies (2075-4434); Aug2023, Vol. 11 Issue 4, p91, 18p

Proper motion, spectra, and timing of PSR J1813–1749 using Chandra and NICER

Autor: C. Malacaria, P. M. Saz Parkinson, Sebastien Guillot, Cristobal M. Espinoza, Wynn C. G. Ho, Brynmor Haskell, Gaurava K. Jaisawal, B. Limyansky, Micha l. Bejger, Chi-Yung Ng

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 498 (3), pp.4396-4403. ⟨10.1093/mnras/staa2653⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 498 (3), pp.4396-4403. ⟨10.1093/mnras/staa2653⟩
Mon Not R Astron Soc
Ho, W C G, Guillot, S, Parkinson, P M S, Limyansky, B, Ng, C-Y, Bejger, M, Espinoza, C M, Haskell, B, Jaisawal, G K & Malacaria, C 2020, ' Proper motion, spectra, and timing of PSR J1813−1749 using Chandra and NICER ', Monthly Notices of the Royal Astronomical Society, vol. 498, pp. 4396–4403 . https://doi.org/10.1093/mnras/staa2653

PSR J1813-1749 is one of the most energetic rotation-powered pulsars known, producing a pulsar wind nebula (PWN) and gamma-ray and TeV emission, but whose spin period is only measurable in X-ray. We present analysis of two Chandra datasets that are s

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4799cd60249affc1a6c41841da84b079
https://hal.science/hal-02955775/document