Zobrazeno 1 - 10
of 40
pro vyhledávání: '"R. M. Quimby"'
Autor:
M. R. Siebert, C. DeCoursey, D. A. Coulter, M. Engesser, J. D. R. Pierel, A. Rest, E. Egami, M. Shahbandeh, W. Chen, O. D. Fox, Y. Zenati, T. J. Moriya, A. J. Bunker, P. A. Cargile, M. Curti, D. J. Eisenstein, S. Gezari, S. Gomez, M. Guolo, B. D. Johnson, B. A. Joshi, M. Karmen, R. Maiolino, R. M. Quimby, B. Robertson, L. G. Strolger, F. Sun, Q. Wang, T. Wevers
Publikováno v:
The Astrophysical Journal Letters, Vol 972, Iss 1, p L13 (2024)
We present James Webb Space Telescope (JWST) NIRCam and NIRSpec observations of a Type Ic supernova (SN Ic) and its host galaxy (JADES-GS+53.13533-27.81457) at z = 2.83. This SN (named SN 2023adta) was identified in deep JWST/NIRCam imaging from the
Externí odkaz:
https://doaj.org/article/20ed11d80e6e42e59c4bd4a45523741a
Autor:
J. D. R. Pierel, M. Engesser, D. A. Coulter, C. DeCoursey, M. R. Siebert, A. Rest, E. Egami, W. Chen, O. D. Fox, D. O. Jones, B. A. Joshi, T. J. Moriya, Y. Zenati, A. J. Bunker, P. A. Cargile, M. Curti, D. J. Eisenstein, S. Gezari, S. Gomez, M. Guolo, B. D. Johnson, M. Karmen, R. Maiolino, R. M. Quimby, B. Robertson, M. Shahbandeh, L. G. Strolger, F. Sun, Q. Wang, T. Wevers
Publikováno v:
The Astrophysical Journal Letters, Vol 971, Iss 2, p L32 (2024)
We present the James Webb Space Telescope (JWST) discovery of SN 2023adsy, a transient object located in a host galaxy JADES-GS+53.13485−27.82088 with a host spectroscopic redshift of 2.903 ± 0.007. The transient was identified in deep (JWST)/NIRC
Externí odkaz:
https://doaj.org/article/8ca2b65a0aea4db4b417e86a75a2d60d
Autor:
G. Dhungana, R. Kehoe, R. Staten, J. Vinko, J. C. Wheeler, C. Akerlof, D. Doss, F. V. Ferrante, C. A. Gibson, J. Lasker, G. H. Marion, S. B. Pandey, R. M. Quimby, E. Rykoff, D. Smith, F. Yuan, W. Zheng
Publikováno v:
The Astrophysical Journal, Vol 962, Iss 1, p 60 (2024)
We present cosmological analysis of 12 nearby ( z < 0.06) Type IIP supernovae (SNe IIP) observed with the ROTSE-IIIb telescope. To achieve precise photometry, we present a new image-differencing technique that is implemented for the first time on the
Externí odkaz:
https://doaj.org/article/8ee3feef6ab64b728fe4175feaf50262
Autor:
K V Sokolovsky, T J Johnson, S Buson, P Jean, C C Cheung, K Mukai, L Chomiuk, E Aydi, B Molina, A Kawash, J D Linford, A J Mioduszewski, M P Rupen, J L Sokoloski, M N Williams, E Steinberg, I Vurm, B D Metzger, K L Page, M Orio, R M Quimby, A W Shafter, H Corbett, S Bolzoni, J DeYoung, K Menzies, F D Romanov, M Richmond, J Ulowetz, T Vanmunster, G Williamson, D J Lane, M Bartnik, M Bellaver, E Bruinsma, E Dugan, J Fedewa, C Gerhard, S Painter, D-M Peterson, J E Rodriguez, C Smith, H Sullivan, S Watson
Classical novae are shock-powered multi-wavelength transients triggered by a thermonuclear runaway on an accreting white dwarf. V1674 Her is the fastest nova ever recorded (time to declined by two magnitudes is t_2=1.1 d) that challenges our understa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9da3ef0202cf77632a25421fdfd4af80
http://arxiv.org/abs/2302.03043
http://arxiv.org/abs/2302.03043
Publikováno v:
Research Notes of the AAS. 5:160
We report high-cadence photometry of the ultra-fast (t 2 ∼ 1.2 days) nova V1674 Her during its rise to maximum light (V ∼ 6.3) and the beginning of its subsequent decline. These observations from Evryscope and the Mount Laguna Observatory All-Sky
M31N 2008-12a - the remarkable recurrent nova in M31:Pan-Chromatic observations of the 2015 eruption
Autor:
Makoto Watanabe, Pablo Rodríguez-Gil, Iair Arcavi, A. W. Shafter, Amanpreet Kaur, P. Boumis, Iain A. Steele, N. Gehrels, J. U. Ness, F. Kabashima, K. Nishiyama, Izumi Hachisu, J. A. Kennea, Edward M. Sion, Tim O'Brien, M. F. Bode, Hiroyuki Maehara, B. F. Williams, K. Nakajima, M. J. Darnley, N. Kawai, Kamil Hornoch, X. Gao, Michael M. Shara, K. L. Page, Steven Williams, H. Naito, Valério A. R. M. Ribeiro, Griffin Hosseinzadeh, Z. Xu, P. Godon, Y. Sano, J. Chuck Horst, J. P. Osborne, V. P. Goranskij, E. A. Barsukova, D. J. Harman, K. Itagaki, A. F. Valeev, Martin Henze, R. M. Quimby, Rebekah Hounsell, Hana Kučáková, Mariko Kato, D. H. Hartmann, J. Figueira, Gloria Sala, Akira Arai, Tianran Chen, F. Watanabe, Jordi José, K. M. Lau, M. Hernanz, S. Kiyota, S. N. Fabrika
Publikováno v:
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
SCOPUS0004637X-2016-833-2-SID85007524590
Darnley, M J, Henze, M, Bode, M F, Hachisu, I, Hernanz, M, Hornoch, K, Hounsell, R, Kato, M, Ness, J U, Osborne, J P, Page, K L, Ribeiro, V A R M, Rodríguez-Gil, P, Shafter, A W, Shara, M M, Steele, I A, Williams, S C, Arai, A, Arcavi, I, Barsukova, E A, Boumis, P, Chen, T, Fabrika, S, Figueira, J, Gao, X, Gehrels, N, Godon, P, Goranskij, V P, Harman, D J, Hartmann, D H, Hosseinzadeh, G, Horst, J C, Itagaki, K, José, J, Kabashima, F, Kaur, A, Kawai, N, Kennea, J A, Kiyota, S, Kučáková, H, Lau, K M, Maehara, H, Naito, H, Nakajima, K, Nishiyama, K, O'Brien, T J, Quimby, R, Sala, G, Sano, Y, Sion, E M, Valeev, A F, Watanabe, F, Watanabe, M, Williams, B F & Xu, Z 2016, ' M31N 2008-12a-The REMARKABLE RECURRENT NOVA in M31 : PANCHROMATIC OBSERVATIONS of the 2015 ERUPTION ', Astrophysical Journal, vol. 833, no. 2, 149 . https://doi.org/10.3847/1538-4357/833/2/149
The Astrophysical Journal, 833, 2, pp. 1-38
Recercat. Dipósit de la Recerca de Catalunya
instname
The Astrophysical Journal, 833, 1-38
NASA Astrophysics Data System
Universitat Politècnica de Catalunya (UPC)
SCOPUS0004637X-2016-833-2-SID85007524590
Darnley, M J, Henze, M, Bode, M F, Hachisu, I, Hernanz, M, Hornoch, K, Hounsell, R, Kato, M, Ness, J U, Osborne, J P, Page, K L, Ribeiro, V A R M, Rodríguez-Gil, P, Shafter, A W, Shara, M M, Steele, I A, Williams, S C, Arai, A, Arcavi, I, Barsukova, E A, Boumis, P, Chen, T, Fabrika, S, Figueira, J, Gao, X, Gehrels, N, Godon, P, Goranskij, V P, Harman, D J, Hartmann, D H, Hosseinzadeh, G, Horst, J C, Itagaki, K, José, J, Kabashima, F, Kaur, A, Kawai, N, Kennea, J A, Kiyota, S, Kučáková, H, Lau, K M, Maehara, H, Naito, H, Nakajima, K, Nishiyama, K, O'Brien, T J, Quimby, R, Sala, G, Sano, Y, Sion, E M, Valeev, A F, Watanabe, F, Watanabe, M, Williams, B F & Xu, Z 2016, ' M31N 2008-12a-The REMARKABLE RECURRENT NOVA in M31 : PANCHROMATIC OBSERVATIONS of the 2015 ERUPTION ', Astrophysical Journal, vol. 833, no. 2, 149 . https://doi.org/10.3847/1538-4357/833/2/149
The Astrophysical Journal, 833, 2, pp. 1-38
Recercat. Dipósit de la Recerca de Catalunya
instname
The Astrophysical Journal, 833, 1-38
NASA Astrophysics Data System
The Andromeda Galaxy recurrent nova M31N 2008-12a had been observed in eruption ten times, including yearly eruptions from 2008-2014. With a measured recurrence period of $P_\mathrm{rec}=351\pm13$ days (we believe the true value to be half of this) a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8e50a254b58aabe93dd2a543a78625c8
https://doi.org/10.3847/1538-4357/833/2/149
https://doi.org/10.3847/1538-4357/833/2/149
Autor:
I. M. Hook, Jeff Cooke, P. Podsiadlowski, Avishay Gal-Yam, Iair Arcavi, D. A. Howell, Paolo A. Mazzali, Lars Bildsten, R. C. Thomas, Dovi Poznanski, J. S. Bloom, Nicholas M. Law, M. M. Kasliwal, P. E. Nugent, Eran O. Ofek, S. B. Cenko, S. R. Kulkarni, R. M. Quimby, S. Blake, Mark Sullivan
PTF09dav is a peculiar subluminous type Ia supernova (SN) discovered by the Palomar Transient Factory (PTF). Spectroscopically, it appears superficially similar to the class of subluminous SN1991bg-like SNe, but it has several unusual features which
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aebcaf83f290f9dd4a045a9bb99b99da
https://ora.ox.ac.uk/objects/uuid:69f3a204-d971-464c-80c9-1ed180c64107
https://ora.ox.ac.uk/objects/uuid:69f3a204-d971-464c-80c9-1ed180c64107
Autor:
John C Wheeler, Ersin Gogus, Felix Aharonian, Hans A. Krimm, S. A. Yost, Timothy A. McKay, Wiphu Rujopakarn, David Smith, B. E. Schaefer, R. M. Quimby, Michael C. B. Ashley, U. Kiziloglu, Tolga Guver, Jim Wren, Fang Yuan, Eli S. Rykoff, N. Gehrels, M. Özel, H. Flewelling, W. T. Vestrand, Carl W. Akerlof, Gavin Rowell, Scott Barthelmy, A. Phillips
Publikováno v:
The Astrophysical Journal. 702:489-505
WOS: 000269244500040
We report on a complete set of early optical afterglows of gamma-ray bursts (GRBs) obtained with the Robotic Optical Transient Search Experiment (ROTSE-III) telescope network from 2005 March through 2007 June. This set is co
We report on a complete set of early optical afterglows of gamma-ray bursts (GRBs) obtained with the Robotic Optical Transient Search Experiment (ROTSE-III) telescope network from 2005 March through 2007 June. This set is co
Autor:
J. Gorosabel, P. M. Vreeswijk, D. Bersier, C. Ledoux, Eleonora Troja, D. Malesani, R. L. C. Starling, Pall Jakobsson, H. A. Krimm, Jesper Sollerman, Ersin Gogus, Ralph A. M. J. Wijers, A. J. Levan, Yuji Urata, Tolga Guver, Carl W. Akerlof, P. T. O'Brien, Ü. Kızıloǧlu, B. Milvang-Jensen, Nial R. Tanvir, Chryssa Kouveliotou, Dieter Horns, E. S. Rykoff, H. F. Swan, M. Özel, S. A. Yost, Michael C. B. Ashley, Jens Hjorth, J. Wren, Meng Zhai, Fang Yuan, A. E. Ruiz-Velasco, A. Melandri, John C Wheeler, B. L. Jensen, Johan P. U. Fynbo, A. J. Castro-Tirado, Wiphu Rujopakarn, S. D. Barthelmy, Carole Mundell, B. E. Schaefer, Dong Xu, Felix Aharonian, J. M. Castro Cerón, Christina C. Thöne, W. K. Zheng, N. Gehrels, T. R. Marsh, K. Y. Huang, W. T. Vestrand, R. M. Quimby, Michael I. Andersen, Darach Watson, C. Guidorzi, Gavin Rowell, Timothy A. McKay, Andrew C. Phillips
Publikováno v:
Astrophysical Journal, 669(1), 1-9. IOP Publishing Ltd.
We report on follow-up observations of the GRB 060927 using the ROTSE-IIIa telescope and a suite of larger aperture ground-based telescopes. An optical afterglow was detected 20 s after the burst, the earliest rest-frame detection of optical emission
Autor:
R. M. Quimby, E. Goegues, Timothy A. McKay, Michael C. B. Ashley, David Smith, Dieter Horns, Andrew C. Phillips, Ue. Kiziloglu, John C Wheeler, Katherine Alatalo, T. Guever, S. A. Yost, W. T. Vestrand, H. F. Swan, B. E. Schaefer, M. Oezel, Carl W. Akerlof, Robert Kehoe, Felix Aharonian, J. Wren, E. S. Rykoff
Publikováno v:
The Astrophysical Journal. 640:402-406
We present the unfiltered ROTSE-III light curve of the optical transient associated with GRB 050319 beginning 4 s after the cessation of gamma-ray activity. We fit a power-law function to the data using the revised trigger time given by Chincarini et