Zobrazeno 1 - 10
of 15
pro vyhledávání: '"J S Bright"'
Autor:
Giulia Migliori, R. Margutti, B. D. Metzger, R. Chornock, C. Vignali, D. Brethauer, D. L. Coppejans, T. Maccarone, L. Rivera Sandoval, J. S. Bright, T. Laskar, D. Milisavljevic, E. Berger, A. J. Nayana
Publikováno v:
The Astrophysical Journal Letters, Vol 963, Iss 1, p L24 (2024)
We present the first deep X-ray observations of luminous fast blue optical transient (LFBOT) AT 2018cow at ∼3.7 yr since discovery, together with the reanalysis of the observation at δ t ∼ 220 days. X-ray emission is significantly detected at a
Externí odkaz:
https://doaj.org/article/00f566ea293e46778ab2f4f352b06703
Autor:
Raffaella Margutti, J. S. Bright, D. J. Matthews, D. L. Coppejans, K. D. Alexander, E. Berger, M. Bietenholz, R. Chornock, L. DeMarchi, M. R. Drout, T. Eftekhari, W. V. Jacobson-Galán, T. Laskar, D. Milisavljevic, K. Murase, M. Nicholl, C. M. B. Omand, M. Stroh, G. Terreran, B. A. VanderLey
Publikováno v:
The Astrophysical Journal Letters, Vol 954, Iss 2, p L45 (2023)
We present the results from a multiyear radio campaign of the superluminous supernova (SLSN) SN 2017ens, which yielded the earliest radio detection of an SLSN to date at the age of ∼3.3 yr after explosion. SN 2017ens was not detected at radio frequ
Externí odkaz:
https://doaj.org/article/f7f078ac73cf4ef9a83c614548219151
Autor:
C. D. Tremblay, S. S. Varghese, J. Hickish, P. B. Demorest, C. Ng, A. P. V. Siemion, D. Czech, R. A. Donnachie, W. Farah, V. Gajjar, M. Lebofsky, D. H. E. MacMahon, T. Myburgh, M. Ruzindana, J. S. Bright, A. Erickson, K. Lacker
Publikováno v:
The Astronomical Journal, Vol 167, Iss 1, p 35 (2023)
The primary goal of the search for extraterrestrial intelligence is to gain an understanding of the prevalence of technologically advanced beings (organic or inorganic) in the Galaxy. One way to approach this is to look for technosignatures: remotely
Externí odkaz:
https://doaj.org/article/b3191100ad2141fcb20e678e4eb2336c
Autor:
R P Fender, K P Mooley, S E Motta, J S Bright, D R A Williams, A P Rushton, R J Beswick, J C A Miller-Jones, M Kimura, K Isogai, T Kato
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 518:1243-1259
We present analysis of comprehensive radio observations of the black hole V404 Cyg during its 2015 outburst. These data represent the best ever coverage of jet production and particle acceleration from any black hole. We report for the first time a c
Autor:
L Rhodes, J S Bright, R Fender, I Sfaradi, D A Green, A Horesh, K Mooley, D Pasham, S Smartt, D J Titterington, A J van der Horst, D R A Williams
Publikováno v:
Rhodes, L, Bright, J S, Fender, R, Sfaradi, I, Green, D A, Horesh, A, Mooley, K, Pasham, D, Smartt, S, Titterington, D J, van der Horst, A J & Williams, D R A 2023, ' Day-time-scale variability in the radio light curve of the Tidal Disruption Event AT2022cmc: confirmation of a highly relativistic outflow ', Monthly Notices of the Royal Astronomical Society, vol. 521, no. 1, pp. 389–395 . https://doi.org/10.1093/mnras/stad344
Rhodes, L, Bright, J S, Fender, R, Sfaradi, I, Green, D A, Horesh, A, Mooley, K, Pasham, D, Smartt, S, Titterington, D J, van der Horst, A J & Williams, D R A 2023, ' Day-time-scale variability in the radio light curve of the Tidal Disruption Event AT2022cmc: confirmation of a highly relativistic outflow ', Monthly Notices of the Royal Astronomical Society, vol. 521, no. 1, pp. 389-395 . https://doi.org/10.1093/mnras/stad344
Rhodes, L, Bright, J S, Fender, R, Sfaradi, I, Green, D A, Horesh, A, Mooley, K, Pasham, D, Smartt, S, Titterington, D J, van der Horst, A J & Williams, D R A 2023, ' Day-time-scale variability in the radio light curve of the Tidal Disruption Event AT2022cmc: confirmation of a highly relativistic outflow ', Monthly Notices of the Royal Astronomical Society, vol. 521, no. 1, pp. 389-395 . https://doi.org/10.1093/mnras/stad344
Tidal disruption events (TDEs) are transient, multi-wavelength events in which a star is ripped apart by a supermassive black hole. Observations show that in a small fraction of TDEs, a short-lived, synchrotron emitting jet is produced. We observed t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7afa3e0960f414be63992046d010b551
https://www.repository.cam.ac.uk/handle/1810/346015
https://www.repository.cam.ac.uk/handle/1810/346015
Autor:
W. V. Jacobson-Galán, P. Venkatraman, R. Margutti, D. Khatami, G. Terreran, R. J. Foley, R. Angulo, C. R. Angus, K. Auchettl, P. K. Blanchard, A. Bobrick, J. S. Bright, D. Brout, K. C. Chambers, C. D. Couch, D. A. Coulter, K. Clever, K. W. Davis, T. J. L. de Boer, L. DeMarchi, S. A. Dodd, D. O. Jones, J. Johnson, C. D. Kilpatrick, N. Khetan, Z. Lai, D. Langeroodi, C.-C. Lin, E. A. Magnier, D. Milisavljevic, H. B. Perets, J. D. R. Pierel, J. Raymond, S. Rest, A. Rest, R. Ridden-Harper, K. J. Shen, M. R. Siebert, C. Smith, K. Taggart, S. Tinyanont, F. Valdes, V. A. Villar, Q. Wang, S. K. Yadavalli, Y. Zenati, A. Zenteno
Publikováno v:
Jacobson-Galan, W V, Venkatraman, P, Margutti, R, Khatami, D, Terreran, G, Foley, R J, Angulo, R, Angus, C R, Auchettl, K, Blanchard, P K, Bobrick, A, Bright, J S, Brout, D, Chambers, K C, Couch, C D, Coulter, D A, Clever, K, Davis, K W, de Boer, T J L, DeMarchi, L, Dodd, S A, Jones, D O, Johnson, J, Kilpatrick, C D, Khetan, N, Lai, Z, Langeroodi, D, Lin, C-C, Magnier, E A, Milisavljevic, D, Perets, H B, Pierel, J D R, Raymond, J, Rest, S, Rest, A, Ridden-Harper, R, Shen, K J, Siebert, M R, Smith, C, Taggart, K, Tinyanont, S, Valdes, F, Villar, V A, Wang, Q, Yadavalli, S K, Zenati, Y & Zenteno, A 2022, ' The Circumstellar Environments of Double-peaked, Calcium-strong Transients 2021gno and 2021inl ', Astrophysical Journal, vol. 932, no. 1, 58 . https://doi.org/10.3847/1538-4357/ac67dc
We present panchromatic observations and modeling of calcium-strong supernovae (SNe) 2021gno in the star-forming host-galaxy NGC 4165 and 2021inl in the outskirts of elliptical galaxy NGC 4923, both monitored through the Young Supernova Experiment tr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ba22b71685953059d46ebd8b20f5d94b
https://curis.ku.dk/ws/files/315472935/Jacobson_Gal_n_2022_ApJ_932_58.pdf
https://curis.ku.dk/ws/files/315472935/Jacobson_Gal_n_2022_ApJ_932_58.pdf
Autor:
L Rhodes, A J van der Horst, R Fender, D R Aguilera-Dena, J S Bright, S Vergani, D R A Williams
Publikováno v:
Rhodes, L, van der Horst, A J, Fender, R, Aguilera-Dena, D R, Bright, J S, Vergani, S & Williams, D R A 2022, ' Jet-cocoon geometry in the optically dark, very high energy gamma-ray burst 201216C ', Monthly Notices of the Royal Astronomical Society, vol. 513, no. 2, pp. 1895-1909 . https://doi.org/10.1093/mnras/stac1057
We present the results of a radio observing campaign on GRB 201216C, combined with publicly available optical and X-ray data. The detection of very high energy (VHE, >100GeV) emission by MAGIC makes this the fifth VHE GRB at time of publication. Comp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ddb1f6b9c16685770b879e303947be0
Autor:
E. Aydi, K. V. Sokolovsky, J. S. Bright, E. Tremou, M. M. Nyamai, A. Evans, J. Strader, L. Chomiuk, G. Myers, F-J. Hambsch, K. L. Page, D. A. H. Buckley, C. E. Woodward, F. M. Walter, P. Mróz, P. J. Vallely, T. R. Geballe, D. P. K. Banerjee, R. D. Gehrz, R. P. Fender, M. Gromadzki, A. Kawash, C. Knigge, K. Mukai, U. Munari, M. Orio, V. A. R. M. Ribeiro, J. L. Sokoloski, S. Starrfield, A. Udalski, P. A. Woudt
We present a detailed study of the 2019 outburst of the cataclysmic variable V1047~Cen, which hosted a classical nova eruption in 2005. The peculiar outburst occurred 14 years after the classical nova event and lasted for more than 400 days, reaching
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e32bd2c37f5f238b5c05bf4de0f453f3
Autor:
A. Hajela, R. Margutti, J. S. Bright, K. D. Alexander, B. D. Metzger, V. Nedora, A. Kathirgamaraju, B. Margalit, D. Radice, C. Guidorzi, E. Berger, A. MacFadyen, D. Giannios, R. Chornock, I. Heywood, L. Sironi, O. Gottlieb, D. Coppejans, T. Laskar, Y. Cendes, R. Barniol Duran, T. Eftekhari, W. Fong, A. McDowell, M. Nicholl, X. Xie, J. Zrake, S. Bernuzzi, F. S. Broekgaarden, C. D. Kilpatrick, G. Terreran, V. A. Villar, P. K. Blanchard, S. Gomez, G. Hosseinzadeh, D. J. Matthews, J. C. Rastinejad
Publikováno v:
The Astrophysical Journal Letters
Astrophysical Journal Letters, 927, 1-23
Astrophysical Journal Letters, 927, 1, pp. 1-23
Astrophysical Journal Letters, 927, 1-23
Astrophysical Journal Letters, 927, 1, pp. 1-23
For the first $\sim3$ years after the binary neutron star merger event GW 170817 the radio and X-ray radiation has been dominated by emission from a structured relativistic off-axis jet propagating into a low-density medium with n $< 0.01\,\rm{cm^{-3
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa9ddf2b1829cdcd4ea1d69bb59c3da2
Autor:
K. W. Smith, Enrico Ramirez-Ruiz, S. J. Smartt, Q. Wang, P. K. Blanchard, Claudio Grillo, Z. Ansari, Tiara Hung, E. A. Magnier, Georgios Dimitriadis, Andrew Engel, Sofia Rest, Hugo Pfister, Armin Rest, R. J. Wainscoat, Charles D. Kilpatrick, Daniel Muthukrishna, N. Arendse, J. S. Brown, César Rojas-Bravo, Konstantin Malanchev, Katie Auchettl, Christa Gall, J. R. Fairlamb, D. Brethauer, Lindsay DeMarchi, D. A. Coulter, David O. Jones, S. H. Bruun, M. E. Huber, Adriano Agnello, Matthew R. Siebert, Ryan J. Foley, David Matthews, A. Sarangi, S. L. Schr der, C. R. Angus, Maria R. Drout, A. N. Kolborg, Deanne L. Coppejans, Heidi Korhonen, Sierra A. Dodd, Vivienne Baldassare, C. Hede, Candice Stauffer, M. C. Stroh, Kate D. Alexander, D. K. Ramanah, Y. C. Pan, T. J. L. de Boer, Jamie Law-Smith, Alexander Gagliano, Giacomo Terreran, Deep Chatterjee, S. Tinyanont, Kirsty Taggart, K. C. Chambers, Radosław Wojtak, A. Hajela, J. S. Bright, Wynn V. Jacobson-Galán, Gautham Narayan, C. C. Lin, Raffaella Margutti, P. Aleo, A. Baldeschi, Jens Hjorth, S. I. Raimundo, Brenna Mockler, Luca Izzo, K. D. French
Time domain science has undergone a revolution over the past decade, with tens of thousands of new supernovae (SNe) discovered each year. However, several observational domains, including SNe within days or hours of explosion and faint, red transient
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ef68b7f54be9e802ed82d05d4f73c737
https://doi.org/10.48550/arxiv.2010.09724
https://doi.org/10.48550/arxiv.2010.09724