Zobrazeno 1 - 10
of 197
pro vyhledávání: '"David Pooley"'
Autor:
Missfelder, Jan-Friedrich
Publikováno v:
Jahrbuch für Kommunikationsgeschichte, 2019 Jan 01. 21, 187-188.
Externí odkaz:
https://www.jstor.org/stable/27012807
Autor:
Peter J. Brown, Macie Robertson, Yaswant Devarakonda, Emily Sarria, David Pooley, Maximilian D. Stritzinger
Publikováno v:
Universe, Vol 9, Iss 5, p 218 (2023)
The Neil Gehrels Swift Observatory has proven to be an extraordinary supernova (SN) observatory. The clearest application of Swift’s unique strengths is obtaining very early UV and X-ray data of young SNe, which enables robust constraints on their
Externí odkaz:
https://doaj.org/article/be46ddb065a64cd8b3f4f18e7058850b
Autor:
M. J. Bustamante-Rosell, Greg Zeimann, J. Craig Wheeler, Karl Gebhardt, Aaron Zimmerman, Chris Fryer, Oleg Korobkin, Richard Matzner, V. Ashley Villar, S. Karthik Yadavalli, Kaylee M. de Soto, Matthew Shetrone, Steven Janowiecki, Pawan Kumar, David Pooley, Benjamin P. Thomas, Hsin-Yu Chen, Lifan Wang, Jozsef Vinkó, David J. Sand, Ryan Wollaeger, Frederic V. Hessman, Kristen B. McQuinn
Publikováno v:
The Astrophysical Journal, Vol 954, Iss 1, p 102 (2023)
The LIGO HET Response (LIGHETR) project is an enterprise to follow up optical transients (OTs) discovered as gravitational-wave merger sources by the LIGO/Virgo collaboration (LVC). Early spectroscopy has the potential to constrain crucial parameters
Externí odkaz:
https://doaj.org/article/6b990931ef4a45b2b217161e468d585d
Autor:
Keiichi Maeda, Poonam Chandra, Takashi J. Moriya, Andrea Reguitti, Stuart Ryder, Tomoki Matsuoka, Tomonari Michiyama, Giuliano Pignata, Daichi Hiramatsu, K. Azalee Bostroem, Esha Kundu, Hanindyo Kuncarayakti, Melina C. Bersten, David Pooley, Shiu-Hang Lee, Daniel Patnaude, Ósmar Rodríguez, Gaston Folatelli
Publikováno v:
The Astrophysical Journal, Vol 942, Iss 1, p 17 (2022)
SN 2018ivc is an unusual Type II supernova (SN II). It is a variant of SNe IIL, which might represent a transitional case between SNe IIP with a massive H-rich envelope and SNe IIb with only a small amount of the H-rich envelope. However, SN 2018ivc
Externí odkaz:
https://doaj.org/article/ceaecfcefa524d6f8ae77a5381adb8a4
Autor:
Keiichi Maeda, Poonam Chandra, Takashi J. Moriya, Andrea Reguitti, Stuart Ryder, Tomoki Matsuoka, Tomonari Michiyama, Giuliano Pignata, Daichi Hiramatsu, K. Azalee Bostroem, Esha Kundu, Hanindyo Kuncarayakti, Melina C. Bersten, David Pooley, Shiu-Hang Lee, Daniel Patnaude, Ósmar Rodríguez, Gaston Folatelli
Publikováno v:
The Astrophysical Journal. 942(1)
SN 2018ivc is an unusual type II supernova (SN II). It is a variant of SNe IIL, which might represent a transitional case between SNe IIP with a massive H-rich envelope, and IIb with only a small amount of the H-rich envelope. However, SN 2018ivc sho
Autor:
T. W. S. Holoien, Robert L. Mutel, Christopher S. Kochanek, E. E. Falco, T. M. Reynolds, WeiKang Zheng, A. Fiore, Andrea Pastorello, Alexei V. Filippenko, Auni Somero, Benjamin J. Shappee, Naveen A. Reddy, T. G. Brink, Peter Lundqvist, Subo Dong, Katie Auchettl, Chris Ashall, K. Z. Stanek, M. Stritzinger, Dirk Grupe, Tuguldur Sukhbold, Seppo Mattila, S. Benetti, Subhash Bose, Steven Villanueva, David Pooley, J. S. Brown, R. S. Post, Junbo Zhang, J. L. Prieto, Todd A. Thompson, Ping Chen
Publikováno v:
Bose, S, Dong, S, Kochanek, C S, Stritzinger, M D, Ashall, C, Benetti, S, Falco, E, Filippenko, A V, Pastorello, A, Prieto, J L, Somero, A, Sukhbold, T, Zhang, J, Auchettl, K, Brink, T G, Brown, J S, Chen, P, Fiore, A, Grupe, D, Holoien, T W S, Lundqvist, P, Mattila, S, Mutel, R, Pooley, D, Post, R S, Reddy, N, Reynolds, T M, Shappee, B J, Stanek, K Z, Thompson, T A, Villanueva, S & Zheng, W K 2021, ' ASASSN-18am/SN 2018gk : An overluminous type IIb supernova from a massive progenitor ', Monthly Notices of the Royal Astronomical Society, vol. 503, no. 3, pp. 3472-3491 . https://doi.org/10.1093/mnras/stab629
Bose, S, Dong, S, Kochanek, C S, Stritzinger, M D, Ashall, C, Benetti, S, Falco, E, Filippenko, A, Pastorello, A, Prieto, J L, Somero, A, Sukhbold, T, Zhang, J, Auchettl, K, Brink, T G, Brown, J S, Chen, P, Fiore, A, Grupe, D, Holoien, T W S, Lundqvist, P, Mattila, S, Mutel, R, Pooley, D, Post, R S, Reddy, N, Reynolds, T M, Shappee, B J, Stanek, K Z, Thompson, T A, Villanueva, S JR & Zheng, W 2021, ' ASASSN-18am/SN 2018gk : an overluminous Type IIb supernova from a massive progenitor ', Monthly Notices of the Royal Astronomical Society, vol. 503, no. 3, pp. 3472-3491 . https://doi.org/10.1093/mnras/stab629
Bose, S, Dong, S, Kochanek, C S, Stritzinger, M D, Ashall, C, Benetti, S, Falco, E, Filippenko, A, Pastorello, A, Prieto, J L, Somero, A, Sukhbold, T, Zhang, J, Auchettl, K, Brink, T G, Brown, J S, Chen, P, Fiore, A, Grupe, D, Holoien, T W S, Lundqvist, P, Mattila, S, Mutel, R, Pooley, D, Post, R S, Reddy, N, Reynolds, T M, Shappee, B J, Stanek, K Z, Thompson, T A, Villanueva, S JR & Zheng, W 2021, ' ASASSN-18am/SN 2018gk : an overluminous Type IIb supernova from a massive progenitor ', Monthly Notices of the Royal Astronomical Society, vol. 503, no. 3, pp. 3472-3491 . https://doi.org/10.1093/mnras/stab629
ASASSN-18am/SN 2018gk is a newly discovered member of the rare group of luminous, hydrogen-rich supernovae (SNe) with a peak absolute magnitude of MV ≈ −20 mag that is in between normal core-collapse SNe and superluminous SNe. These SNe show no p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f75e874078cb06bc427969f5c3a6422
https://pure.au.dk/portal/da/publications/asassn18amsn-2018gk(7cd63507-3294-4d0e-9b96-8329fdb63c90).html
https://pure.au.dk/portal/da/publications/asassn18amsn-2018gk(7cd63507-3294-4d0e-9b96-8329fdb63c90).html
Autor:
Benjamin P. Thomas, J. Craig Wheeler, Vikram V. Dwarkadas, Christopher Stockdale, Jozsef Vinkó, David Pooley, Yerong Xu, Greg Zeimann, Phillip MacQueen
Publikováno v:
The Astrophysical Journal. 930:57
SN 2014C was originally classified as a Type Ib supernova, but at phase {\phi} = 127 d post-explosion strong H{\alpha} emission was observed. SN 2014C has since been observed in radio, infrared, optical and X-ray bands. Here we present new optical sp
Autor:
Arash Bahramian, James Miller-Jones, Craig O. Heinke, Jay Strader, Gregory R. Sivakoff, Vlad Tudor, Evangelia Tremou, Yue Zhao, K. L. Li, David Pooley, Thomas J. Maccarone, Laura Chomiuk, Johannes Buchner, Laura Shishkovsky
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2020, 901 (1), pp.57. ⟨10.3847/1538-4357/aba51d⟩
The Astrophysical Journal, American Astronomical Society, 2020, 901 (1), pp.57. ⟨10.3847/1538-4357/aba51d⟩
Globular clusters host a variety of lower-luminosity ($L_X 10^{33}$ erg s$^{-1}$. Among these moderately bright systems, we discover a new source in NGC 6539 that may be a candidate accreting stellar-mass black hole or a transitional millisecond puls
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::697fb47b15fac35f9ba7e9b10a3bc68c
https://hal.archives-ouvertes.fr/hal-02908362
https://hal.archives-ouvertes.fr/hal-02908362
Autor:
Alessandra Corsi, L. E. Rivera Sandoval, Peter J. Brown, J. C. Wheeler, David Pooley, Thomas J. Maccarone
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 480:L146-L150
Supernova (SN) 2018cow (or AT2018cow) is an optical transient detected in the galaxy CGCG 137-068. It has been classified as a SN due to various characteristics in its optical spectra. The transient is also a bright X-ray source. We present results o
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 474:933-946
WD 1145+017 was observed from 2016 November through 2017 June for the purpose of further characterizing the transit behavior of the dusty debris clouds orbiting this white dwarf. The optical observations were carried out with a small ground-based tel