Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Christopher Bilinski"'
Autor:
David J. Sand, Chengyuan Xu, Ken'ichi Nomoto, Iair Arcavi, Koichi Itagaki, Y. Dong, Gagandeep S. Anand, Takashi J. Moriya, T. Noguchi, Jamison Burke, Alexei V. Filippenko, Jennifer E. Andrews, D. Andrew Howell, Gastón Folatelli, Keiichi Maeda, Curtis McCully, Daichi Hiramatsu, Melina C. Bersten, G. Grant Williams, Stefano Valenti, Nozomu Tominaga, Schuyler D. Van Dyk, Peter J. Brown, Patrick L. Kelly, Jared A. Goldberg, Nathan Smith, Griffin Hosseinzadeh, Paul S. Smith, Christopher Bilinski, K. Azalee Bostroem
In the transitional mass range (~8–10 solar masses) between white dwarf formation and iron core-collapse supernovae, stars are expected to produce an electron-capture supernova. Theoretically, these progenitors are thought to be super-asymptotic gi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c5f50e0dafdc37a66b8b17e0d2c11cef
https://resolver.caltech.edu/CaltechAUTHORS:20210202-095214084
https://resolver.caltech.edu/CaltechAUTHORS:20210202-095214084
Autor:
Paul S. Smith, Jennifer Andrews, Douglas C. Leonard, Kelsey I. Clubb, Patrick L. Kelly, Samantha Cargill, Nathan Smith, WeiKang Zheng, Christopher Bilinski, D. Andrew Howell, Alexei V. Filippenko, Kenia Pina, H. Yuk, Griffin Hosseinzadeh, O. D. Fox, D. J. Sand, Haejung Kim, Goni Halevy, Jennifer L. Hoffman, Chadwick Casper, Sahana Kumar, Peter Milne, G. Grant Williams
We present photometry, spectra, and spectropolarimetry of supernova (SN) 2014ab, obtained through $\sim 200$ days after peak brightness. SN 2014ab was a luminous Type IIn SN ($M_V < -19.14$ mag) discovered after peak brightness near the nucleus of it
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::97fac7ebc807a95d9ff9881194831d7c
http://arxiv.org/abs/2007.12134
http://arxiv.org/abs/2007.12134
Autor:
Jeffrey M. Silverman, Maxwell Moe, Mansi M. Kasliwal, Wen-fai Fong, Alexei V. Filippenko, Carles Badenes, Nathan Smith, Charles D. Kilpatrick, Christopher Bilinski, Jennifer E. Andrews, Peter Milne
MCA-1B (also called UIT003) is a luminous hot star in the western outskirts of M33, classified over 20yr ago with a spectral type of Ofpe/WN9 and identified then as a candidate luminous blue variable (LBV). Palomar Transient Factory data reveal that
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::846fd6318e51e14744e6835c54f9687e
https://resolver.caltech.edu/CaltechAUTHORS:20200326-132640739
https://resolver.caltech.edu/CaltechAUTHORS:20200326-132640739
Autor:
Jennifer E. Andrews, G. Grant Williams, Wei Kang Zheng, S. Bradley Cenko, Kelsey I. Clubb, Charles D. Kilpatrick, Patrick L. Kelly, Alexei V. Filippenko, Wen-fai Fong, Peter Milne, Christopher Bilinski, Jon C. Mauerhan, Christopher Bullivant, O. D. Fox, Nathan Smith
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 476:1497-1518
We present photometry and spectroscopy of SN2013fs and SN2013fr in the first 100 days post-explosion. Both objects showed transient, relatively narrow H$\alpha$ emission lines characteristic of SNeIIn, but later resembled normal SNeII-P or SNeII-L, i
Autor:
Jennifer L. Hoffman, Jon C. Mauerhan, Douglas C. Leonard, Luc Dessart, Amber L. Porter, Paul S. Smith, Christopher Bilinski, Nathan Smith, Leah Huk, G. Grant Williams, Peter Milne
Publikováno v:
Proceedings of the International Astronomical Union. 12:54-58
Because polarization encodes geometrical information about unresolved scattering regions, it provides a unique tool for analyzing the 3-D structures of supernovae (SNe) and their surroundings. SNe of all types exhibit time-dependent spectropolarimetr
Autor:
Jakob Nordin, D. Bersier, Gautham Narayan, Dan Kasen, Zhihao Chen, R. S. Post, B. Cseh, J. Van Cleve, James M. DerKacy, L. Denneau, Lluís Galbany, M. Redick, A. Rest, Krisztián Sárneczky, Subhash Bose, Curtis McCully, Hanna Sai, B. C. Kaiser, E. Baron, C. A. Peterson, J. Vinicius de Miranda Cardoso, Jeffrey L. Coughlin, A. Razza, M. Packard, Steven Williams, G. Beerman, M. Muszynski, Cs. Kalup, B. Elsaesser, O. Hanyecz, G. Csörnyei, Iair Arcavi, J. Moffatt, Isobel Hook, Wenxiong Li, A. Villar, J. Kampmeier, Robert L. Mutel, César Rojas-Bravo, K. A. Larson, Liming Rui, R. Gangopadhyay, B. Csák, S. Margheim, Peter A. Milne, Cosimo Inserra, Subo Dong, Thomas W.-S. Holoien, Jennifer E. Andrews, J. Burke, Han Lin, Jun Mo, Jessie L. Dotson, Kaicheng Zhang, John C Wheeler, J. Palmerio, J. S. Brown, R. M. Larsen, Kate Maguire, H. Flewelling, Katie Auchettl, Danfeng Xiang, K. C. Chambers, Ori D. Fox, Attila Bódi, S. Holmbo, András Pál, C. McGinn, Edward J. Shaya, John L. Tonry, Xulin Zhao, Xiaojia Zhang, E. A. Magnier, M. Hanley, Yen-Chen Pan, Bernadett Ignácz, B. Stalder, R. Szabó, K. M. McCalmont-Everton, G. Zsidi, Joshua S. Reding, J. A. Muñoz, Geert Barentsen, Daichi Hiramatsu, K. Steward, Brad E. Tucker, J. Brimacombe, K. W. Smith, A. Zenteno, R. J. Foley, J. V. Shields, I. Rajmon, Jozsef Vinko, Xiaofeng Wang, Charles D. Kilpatrick, Steven Villanueva, A. Wheaton, B. Spencer, Ann Marie Cody, Peter J. Brown, T. Weschler, L. Migliorini, Xue Li, Claudia P. Gutiérrez, Fang Huang, Saurabh Jha, R. Bjella, C. Labonde, Benjamin J. Shappee, Mark Willman, D. Tallon, V. Nystrom, Tianmeng Zhang, Griffin Hosseinzadeh, S. Flynn, Long Wang, David A. Coulter, David J. Sand, Georgios Dimitriadis, D. O. Jones, J. J. Hermes, Thomas Barclay, Christopher Bilinski, H. Weiland, Réka Könyves-Tóth, Régis Cartier, Steve B. Howell, Peter M. Garnavich, Kim Griest, J. L. Prieto, S. E. Ross, Mark E. Huber, Zs. Bognár, Róbert Szakáts, R. Kloetzel, Krzysztof Z. Stanek, Christopher S. Kochanek, Stefano Valenti, Christina Hedges, G. Castillo, Todd A. Thompson, Ping Chen, C. Z. Waters, L. Kohnert, Adam G. Riess, Nathan Smith, T. B. Lowe, Anthony L. Piro, L. H. Reedy, Levente Kriskovics, Linyi Li, Maria R. Drout, Dale Andrew Howell, A. N. Heinze, A. Ordasi, Stephen J. Smartt, Patrick J. Vallely, A. S. B. Schultz, Joanna Bulger, Michael Gully-Santiago, Jujia Zhang, Ádám Sódor, D. Osborne
Publikováno v:
Astrophys.J.
Astrophys.J., 2019, 870 (1), pp.12. ⟨10.3847/1538-4357/aaec74⟩
Li, W, Wang, X, Vinko, J, Mo, J, Hosseinzadeh, G, Sand, D J, Zhang, J, Lin, H, Zhang, T, Wang, L, Zhang, J, Chen, Z, Xiang, D, Rui, L, Huang, F, Li, X, Zhang, X, Li, L, Baron, E, Derkacy, J M, Zhao, X, Sai, H, Zhang, K, Wang, L, Howell, D A, McCully, C, Arcavi, I, Valenti, S, Hiramatsu, D, Burke, J, Rest, A, Garnavich, P, Tucker, B E, Narayan, G, Shaya, E, Margheim, S, Zenteno, A, Villar, A, Dimitriadis, G, Foley, R J, Pan, Y-C, Coulter, D A, Fox, O D, Jha, S W, Jones, D O, Kasen, D N, Kilpatrick, C D, Piro, A L, Riess, A G, Holmbo, S, PTSS TNTS, LCO, KEGS, UCSC, ASAS-SN, Pan-STARRS, Swift, ePESSTO, ATLAS, K2 Mission Team & Kepler Spacecraft Team 2019, ' Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the Kepler 2 Observations ', Astrophysical Journal, vol. 870, no. 1, 12 . https://doi.org/10.3847/1538-4357/aaec74
The Astrophysical Journal
Astrophys.J., 2019, 870 (1), pp.12. ⟨10.3847/1538-4357/aaec74⟩
Li, W, Wang, X, Vinko, J, Mo, J, Hosseinzadeh, G, Sand, D J, Zhang, J, Lin, H, Zhang, T, Wang, L, Zhang, J, Chen, Z, Xiang, D, Rui, L, Huang, F, Li, X, Zhang, X, Li, L, Baron, E, Derkacy, J M, Zhao, X, Sai, H, Zhang, K, Wang, L, Howell, D A, McCully, C, Arcavi, I, Valenti, S, Hiramatsu, D, Burke, J, Rest, A, Garnavich, P, Tucker, B E, Narayan, G, Shaya, E, Margheim, S, Zenteno, A, Villar, A, Dimitriadis, G, Foley, R J, Pan, Y-C, Coulter, D A, Fox, O D, Jha, S W, Jones, D O, Kasen, D N, Kilpatrick, C D, Piro, A L, Riess, A G, Holmbo, S, PTSS TNTS, LCO, KEGS, UCSC, ASAS-SN, Pan-STARRS, Swift, ePESSTO, ATLAS, K2 Mission Team & Kepler Spacecraft Team 2019, ' Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the Kepler 2 Observations ', Astrophysical Journal, vol. 870, no. 1, 12 . https://doi.org/10.3847/1538-4357/aaec74
The Astrophysical Journal
Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically-confirmed type Ia supernova (SN Ia) observed in the $Kepler$ field. The $Kepler$ data revealed an excess emission in its early light curve, allowing to place interesting constraints o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::55e9e5cf46dafad065d3e32cbff5c492
https://hal.archives-ouvertes.fr/hal-01990737
https://hal.archives-ouvertes.fr/hal-01990737
Autor:
Subo Dong, Boaz Katz, S. Benetti, Nathan Smith, Christopher Bilinski, A. Morales-Garoffolo, L. Tomasella, Ping Chen, Thomas W.-S. Holoien, Barry F. Madore, Peter Milne, Jeffrey A. Rich, Jennifer E. Andrews, Stephan Frank, J. A. Kollmeier, Subhash Bose, Benjamin J. Shappee, Andrea Pastorello, J. L. Prieto, Leonardo Tartaglia, D. Bersier, Seiichiro Kiyota, Nancy Elias-Rosa, Christopher S. Kochanek, Krzysztof Z. Stanek, Enrico Cappellaro, Charles D. Kilpatrick, Joseph Brimacombe
Publikováno v:
Astrophysical Journal
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
We report a luminous Type II supernova, ASASSN-15nx, with a peak luminosity of M_V=-20 mag, that is between typical core-collapse supernovae and super-luminous supernovae. The post-peak optical light curves show a long, linear decline with a steep sl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6a8df66c73346bf7dcaf75883f2a014f
http://arxiv.org/abs/1804.00025
http://arxiv.org/abs/1804.00025
Autor:
Melissa L. Graham, J. Craig Wheeler, Jennifer L. Hoffman, Douglas C. Leonard, George H Marion, Emmanouil Chatzopoulos, Jon C. Mauerhan, Robert M. Quimby, Christopher Bilinski, Carl W. Akerlof, Alexei V. Filippenko, G. Grant Williams, Peter Milne, Jeffrey M. Silverman, Leah Huk, Nathan Smith, Jennifer E. Andrews, Jozsef Vinko, Paul S. Smith, Wei Kang Zheng, Fang Yuan
Publikováno v:
NASA Astrophysics Data System
We present photometry, spectra, and spectropolarimetry of supernova (SN) 2012ab, mostly obtained over the course of $\sim 300$ days after discovery. SN 2012ab was a Type IIn (SN IIn) event discovered near the nucleus of spiral galaxy 2MASXJ12224762+0
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d2e2134136415567590be9260043ce88
http://arxiv.org/abs/1712.03370
http://arxiv.org/abs/1712.03370
Autor:
Nathan Smith, G. Grant Williams, Jennifer L. Hoffman, Leah Huk, Amber L. Porter, Mark D. Leising, Paul S. Smith, Christopher Bilinski, Peter A. Milne, Douglas C. Leonard
We present spectropolarimetric observations of the nearby Type Ia SN 2014J in M82 over six epochs: +0, +7, +23, +51, +77, +109, and +111 days with respect to B-band maximum. The strong continuum polarization, which is constant with time, shows a wave
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2bd6f0fd2ba33ef2ead017d7bb33b434
Autor:
Weidong Li, Alexei V. Filippenko, Christopher Bilinski, G. Grant Williams, Nathan Smith, Wei Kang Zheng
We searched through roughly 12 years of archival survey data acquired by the Katzman Automatic Imaging Telescope (KAIT) as part of the Lick Observatory Supernova Search (LOSS) in order to detect or place limits on possible progenitor outbursts of Typ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1220ec35e69de95ff491f2494b0a3819
http://arxiv.org/abs/1503.04252
http://arxiv.org/abs/1503.04252