Zobrazeno 1 - 10
of 62
pro vyhledávání: '"E. S. Phinney"'
Autor:
Kevin B. Burdge, Thomas R. Marsh, Jim Fuller, Eric C. Bellm, Ilaria Caiazzo, Deepto Chakrabarty, Michael W. Coughlin, Kishalay De, V. S. Dhillon, Matthew J. Graham, Pablo Rodríguez-Gil, Amruta D. Jaodand, David L. Kaplan, Erin Kara, Albert K. H. Kong, S. R. Kulkarni, Kwan-Lok Li, S. P. Littlefair, Walid A. Majid, Przemek Mróz, Aaron B. Pearlman, E. S. Phinney, Jan van Roestel, Robert A. Simcoe, Igor Andreoni, Andrew J. Drake, Richard G. Dekany, Dmitry A. Duev, Erik C. Kool, Ashish A. Mahabal, Michael S. Medford, Reed Riddle, Thomas A. Prince
Over a dozen millisecond pulsars are ablating low-mass companions in close binary systems. In the original "black widow", the 8-hour orbital period eclipsing pulsar PSR J1959+2048 (PSR B1957+20), high energy emission originating from the pulsar is ir
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a602a3542eed06c32003c95c04150397
https://resolver.caltech.edu/CaltechAUTHORS:20220505-812251500
https://resolver.caltech.edu/CaltechAUTHORS:20220505-812251500
Autor:
Thomas Kupfer, Zhuyun Zhuang, S. P. Littlefair, E. S. Phinney, Boris Gaensicke, Thomas A. Prince, David L. Kaplan, Reed Riddle, Tom Marsh, Matthew J. Graham, Stephen Kaye, Jan van Roestel, Przemek Mróz, Dmitry A. Duev, Maayane T. Soumagnac, Michael W. Coughlin, George Helou, Andrew J. Drake, Ashish Mahabal, Pier-Emmanuel Tremblay, Pablo Rodríguez-Gil, Frank J. Masci, Jim Fuller, Roger Smith, David Hale, Ilaria Caiazzo, Michael Feeney, V. S. Dhillon, Shrinivas R. Kulkarni, Kevin B. Burdge, Richard Dekany, Yuhan Yao, Eric C. Bellm, J. J. Hermes
Publikováno v:
The Astrophysical Journal
Using photometry collected with the Zwicky Transient Facility (ZTF), we are conducting an ongoing survey for binary systems with short orbital periods ($P_{\rm b}
32 pages, 12 figures, 7 tables, submitted to ApJ
32 pages, 12 figures, 7 tables, submitted to ApJ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d2f2db5fcbc4899300fb45f24ae073dc
https://resolver.caltech.edu/CaltechAUTHORS:20200916-113006965
https://resolver.caltech.edu/CaltechAUTHORS:20200916-113006965
Autor:
R. R. Laher, A. A. Mahabal, Y.-L. Kim, Adam A. Miller, M. Rigault, Jesper Sollerman, Tassilo Schweyer, Frank J. Masci, Ariel Goobar, M. Kromer, M. R. Magee, Stephen Kaye, Reed Riddle, E. Zimmerman, Eran O. Ofek, E. S. Phinney, Abigail Polin, Suhail Dhawan, P. E. Nugent, Maayane T. Soumagnac, Kate Maguire, David L. Shupe, Alexandre Delacroix, S. J. Prentice, David Goldstein, Avishay Gal-Yam, Robert J. Walters, Daniel A. Perley, I. Andreoni, I. Irani, Matthew J. Graham, C. Fremling, B. Rusholme, Steve Schulze, Lin Yan, V. Z. Golkhou, Shrinivas R. Kulkarni, M. M. Kasliwal, Giacomo Terreran, Mattia Bulla, K. de, R. Dekany, Yuhan Yao, Eric C. Bellm, J. Zolkower
Publikováno v:
Astrophysical Journal, vol 898, iss 1
Astrophys.J.
Astrophys.J., 2020, 898 (1), pp.56. ⟨10.3847/1538-4357/ab9e05⟩
The Astrophysical Journal
Astrophys.J.
Astrophys.J., 2020, 898 (1), pp.56. ⟨10.3847/1538-4357/ab9e05⟩
The Astrophysical Journal
Early observations of Type Ia supernovae (SNe$\,$Ia) provide essential clues for understanding the progenitor system that gave rise to the terminal thermonuclear explosion. We present exquisite observations of SN$\,$2019yvq, the second observed SN$\,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b6e7fc0f7a547442b16c88c4c18e3fc6
https://escholarship.org/uc/item/0558g06b
https://escholarship.org/uc/item/0558g06b
Autor:
David R. Williams, B. Rusholme, E. C. Kool, Michael Porter, Lin Yan, Jesper Sollerman, Melissa L. Graham, V. Z. Golkhou, Daniel J. Reiley, David A. Green, Yashvi Sharma, Hector P. Rodriguez, Jakob Nordin, Stephen Kaye, Itai Sfaradi, Dmitry A. Duev, Leonardo Tartaglia, E. S. Phinney, Cristina Barbarino, Y.-L. Kim, Frank J. Masci, Kaushik De, Emir Karamehmetoglu, Ragnhild Lunnan, Daniel A. Perley, J. van Roestel, Maayane T. Soumagnac, T. M. Reynolds, Eric C. Bellm, Assaf Horesh, Steve Schulze, Kirsty Taggart, Christoffer Fremling, Russ R. Laher
Publikováno v:
Astron.Astrophys.
Astron.Astrophys., 2021, 652, pp.A136. ⟨10.1051/0004-6361/202039137⟩
Astron.Astrophys., 2021, 652, pp.A136. ⟨10.1051/0004-6361/202039137⟩
Context: Type Ibn supernovae are a rare class of stripped envelope supernovae interacting with a helium-rich CSM. The majority of the SNe Ibn reported display a surprising homogeneity in their fast lightcurves and starforming hosts. Aims: We present
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::334bcfa3a3c4246792f2294fba596058
Autor:
Stephen Bourke, E. S. Phinney, Marin M. Anderson, Kunal Mooley, D. Dong, S. T. Myers, Dale A. Frail, Gregg Hallinan, Shrinivas R. Kulkarni, Assaf Horesh, S. B. Cenko
We present the discovery of a nuclear transient with the Caltech-NRAO Stripe 82 Survey (CNSS), a dedicated radio transient survey carried out with the Karl G. Jansky Very Large Array (VLA). This transient, CNSS J001947.3+003527, exhibited a turn-on o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d00b834aa75d0c1fd674804ec2dc383f
http://arxiv.org/abs/1910.11912
http://arxiv.org/abs/1910.11912
Autor:
Daniel J. Reiley, Ashish Mahabal, Paula Szkody, Tom Marsh, Ulrich Heber, Dmitry A. Duev, S. P. Littlefair, Kevin B. Burdge, Ben Rusholme, Michael Porter, Hector P. Rodriguez, Maayane T. Soumagnac, Thomas Kupfer, David L. Shupe, Jim Fuller, Gabriel Murawski, V. S. Dhillon, Russ R. Laher, Andrew J. Drake, Lars Bildsten, J. J. Hermes, Jan van Roestel, Shrinivas R. Kulkarni, Thomas A. Prince, Yuhan Yao, Eric C. Bellm, D. Schneider, Andreas Irrgang, Matthew J. Graham, Evan B. Bauer, Frank J. Masci, E. S. Phinney, Michael Feeney
Publikováno v:
The Astrophysical Journal. 898:L25
We present the discovery of the second binary with a Roche lobe-filling hot subdwarf transferring mass to a white dwarf (WD) companion. This 56 minute binary was discovered using data from the Zwicky Transient Facility. Spectroscopic observations rev
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::73def2809671054c9294a677caba5e6c
https://doi.org/10.3847/2041-8213/aba3c2
https://doi.org/10.3847/2041-8213/aba3c2
Publikováno v:
The Astrophysical Journal, 817, 69
The Astrophysical Journal, 817, 1-7
The Astrophysical Journal, 817, 1, pp. 1-7
The Astrophysical Journal, 817, 1-7
The Astrophysical Journal, 817, 1, pp. 1-7
The theoretical and observed populations of pre-cataclysmic variables (pre-CVs) are dominated by systems with low-mass white dwarfs (WDs), while the WD masses in CVs are typically high. In addition, the space density of CVs is found to be significant
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::189fb3bcc4ad0bd711c22bc5b70d6dd7
http://hdl.handle.net/1887/47261
http://hdl.handle.net/1887/47261
Autor:
E. S. Phinney, Alison J. Farmer
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 346:1197-1214
We use a population synthesis approach to characterise, as a function of cosmic time, the extragalactic close binary population descended from stars of low to intermediate initial mass. The unresolved gravitational wave (GW) background due to these s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::17cbbecabae87d81c75796c49576f678
https://doi.org/10.1111/j.1365-2966.2003.07176.x
https://doi.org/10.1111/j.1365-2966.2003.07176.x
Autor:
E. S. Phinney, Andrew Melatos
Publikováno v:
Publications of the Astronomical Society of Australia. 18:421-430
The hydromagnetic structure of a neutron star accreting symmetrically at both magnetic poles is calculated as a function of accreted mass, Ma, starting from a polytropic sphere plus central magnetic dipole (Ma =0) and evolving the configuration throu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::64f2ec98c134e38ca826623b2d57a3a1
https://doi.org/10.1071/as01056
https://doi.org/10.1071/as01056
Autor:
R. M. Wark, Shri Kulkarni, Dale A. Frail, E. S. Phinney, Mark H. Wieringa, James L. Higdon, Joshua S. Bloom, Elaine M. Sadler, Ron Ekers
Publikováno v:
Nature. 395:663-669
Data accumulated over the past year strongly favour the idea that γ-ray bursts lie at cosmological distances, although the nature of the power source remains unclear. Here we report radio observations of the supernova SN1998bw, which exploded at abo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e942b4dd307f911716496fae3ae36ee7
https://doi.org/10.1038/27139
https://doi.org/10.1038/27139