Zobrazeno 1 - 10
of 908
pro vyhledávání: '"L. Piro"'
Autor:
E. Troja, G. Ryan, L. Piro, H. van Eerten, S. B. Cenko, Y. Yoon, S.-K. Lee, M. Im, T. Sakamoto, P. Gatkine, A. Kutyrev, S. Veilleux
Publikováno v:
Nature Communications, Vol 9, Iss 1, Pp 1-10 (2018)
A faint gamma-ray burst (GRB 170817A) has been recently detected in coincidence with the gravitational wave (GW) event GW 170817. Here, the authors report that another faint short GRB at a cosmological distance (GRB150101B) and its late time emission
Externí odkaz:
https://doaj.org/article/2ad8bfb3c4ea49f0b49edc6395fbb505
Autor:
J M DerKacy, S Paugh, E Baron, P J Brown, C Ashall, C R Burns, E Y Hsiao, S Kumar, J Lu, N Morrell, M M Phillips, M Shahbandeh, B J Shappee, M D Stritzinger, M A Tucker, Z Yarbrough, K Boutsia, P Hoeflich, L Wang, L Galbany, E Karamehmetoglu, K Krisciunas, P Mazzali, A L Piro, N B Suntzeff, A Fiore, C P Gutiérrez, P Lundqvist, A Reguitti
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522:3481-3505
We present ultraviolet (UV) to near-infrared (NIR) observations and analysis of the nearby Type Ia supernova SN 2021fxy. Our observations include UV photometry from Swift/UVOT, UV spectroscopy from HST/STIS, and high-cadence optical photometry with t
Autor:
L Piro, M Colpi, J Aird, A Mangiagli, A C Fabian, M Guainazzi, S Marsat, A Sesana, P McNamara, M Bonetti, E M Rossi, N R Tanvir, J G Baker, G Belanger, T Dal Canton, O Jennrich, M L Katz, N Luetzgendorf
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2023, 521 (2), pp.2577-2592. ⟨10.1093/mnras/stad659⟩
Monthly Notices of the Royal Astronomical Society, 2023, 521 (2), pp.2577-2592. ⟨10.1093/mnras/stad659⟩
The European Space Agency is studying two large-class missions bound to operate in the decade of the 30s, and aiming at investigating the most energetic and violent phenomena in the Universe. $Athena$ is poised to study the physical conditions of bar
Autor:
M. D’Andrea, K. Ravensberg, A. Argan, D. Brienza, S. Lotti, C. Macculi, G. Minervini, L. Piro, G. Torrioli, F. Chiarello, L. Ferrari Barusso, M. Biasotti, G. Gallucci, F. Gatti, M. Rigano, H. Akamatsu, J. Dercksen, L. Gottardi, F. de Groote, R. den Hartog, J.-W. den Herder, R. Hoogeveen, B. Jackson, A. McCalden, S. Rosman, E. Taralli, D. Vaccaro, M. de Wit, J. Chervenak, S. Smith, N. Wakeham
Publikováno v:
Journal of Low Temperature Physics. 209:433-440
The X-IFU is the cryogenic spectrometer onboard the future ATHENA X-ray observatory. It is based on a large array of TES microcalorimeters, which works in combination with a Cryogenic AntiCoincidence detector (CryoAC). This is necessary to reduce the
Autor:
Bas Dorsman, Geert Raaijmakers, S. Bradley Cenko, Samaya Nissanke, Leo P. Singer, Mansi M. Kasliwal, Anthony L. Piro, Eric C. Bellm, Dieter H. Hartmann, Kenta Hotokezaka, Kamilė Lukošiūtė
Publikováno v:
The Astrophysical Journal
The detection of gravitational waves from binary neuron star merger GW170817 and electromagnetic counterparts GRB170817 and AT2017gfo kick-started the field of gravitational wave multimessenger astronomy. The optically red to near infra-red emission
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::adc82b8989b272f947e4e3c26b28165d
https://resolver.caltech.edu/CaltechAUTHORS:20230314-845495900.47
https://resolver.caltech.edu/CaltechAUTHORS:20230314-845495900.47
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
M. D. Fulton, S. J. Smartt, L. Rhodes, M. E. Huber, V. A. Villar, T. Moore, S. Srivastav, A. S. B. Schultz, K. C. Chambers, L. Izzo, J. Hjorth, T.-W. Chen, M. Nicholl, R. J. Foley, A. Rest, K. W. Smith, D. R. Young, S. A. Sim, J. Bright, Y. Zenati, T. de Boer, J. Bulger, J. Fairlamb, H. Gao, C.-C. Lin, T. Lowe, E. A. Magnier, I. A. Smith, R. Wainscoat, D. A. Coulter, D. O. Jones, C. D. Kilpatrick, P. McGill, E. Ramirez-Ruiz, K.-S. Lee, G. Narayan, V. Ramakrishnan, R. Ridden-Harper, A. Singh, Q. Wang, A. K. H. Kong, C.-C. Ngeow, Y.-C. Pan, S. Yang, K. W. Davis, A. L. Piro, C. Rojas-Bravo, J. Sommer, S. K. Yadavalli
Publikováno v:
Fulton, M D, Smartt, S J, Rhodes, L, Huber, M E, Villar, V A, Moore, T, Srivastav, S, Schultz, A S B, Chambers, K C, Izzo, L, Hjorth, J, Chen, T-W, Nicholl, M, Foley, R J, Rest, A, Smith, K W, Young, D R, Sim, S A, Bright, J, Zenati, Y, Boer, T D, Bulger, J, Fairlamb, J, Gao, H, Lin, C-C, Lowe, T, Magnier, E A, Smith, I A, Wainscoat, R, Coulter, D A, Jones, D O, Kilpatrick, C D, McGill, P, Ramirez-Ruiz, E, Lee, K-S, Narayan, G, Ramakrishnan, V, Ridden-Harper, R, Singh, A, Wang, Q, Kong, A K H, Ngeow, C-C, Pan, Y-C, Yang, S, Davis, K W, Piro, A L, Rojas-Bravo, C, Sommer, J & Yadavalli, S K 2023, ' The optical light curve of GRB 221009A: the afterglow and the emerging supernova ', The Astrophysical Journal Letters, vol. 946, no. 1, L22 . https://doi.org/10.3847/2041-8213/acc101
We present extensive optical photometry of the afterglow of GRB~221009A. Our data cover $0.9 - 59.9$\,days from the time of \textit{Swift} and \textit{Fermi} GRB detections. Photometry in $rizy$-band filters was collected primarily with Pan-STARRS an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8862e25fa7866ff766df72e4ccfaf526
Autor:
Mi Lai, Stacey E. Alexeeff, Hannes L. Röst, Ziyi Zhang, Michael B. Wheeler, Feihan F. Dai, Amina Allalou, Erica P. Gunderson, Anthony L. Piro
Publikováno v:
BMC Medicine, Vol 19, Iss 1, Pp 1-21 (2021)
BMC Medicine
BMC Medicine
BackgroundWomen with a history of gestational diabetes mellitus (GDM) have a 7-fold higher risk of developing type 2 diabetes (T2D). It is estimated that 20-50% of women with GDM history will progress to T2D within 10 years after delivery. Intensive
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Hydrodynamics of Collisions and Close Encounters between Stellar Black Holes and Main-sequence Stars
Recent analyses have shown that close encounters between stars and stellar black holes occur frequently in dense star clusters. Depending upon the distance at closest approach, these interactions can lead to dissipating encounters such as tidal captu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::efdee63ad74d6b9df1ebb8ba6601ec4a
https://resolver.caltech.edu/CaltechAUTHORS:20220517-214238256
https://resolver.caltech.edu/CaltechAUTHORS:20220517-214238256