Zobrazeno 1 - 10
of 21
pro vyhledávání: '"M. C. B. Ashley"'
Publikováno v:
Earth System Science Data, Vol 12, Pp 3529-3544 (2020)
Dome A, the summit of the East Antarctic Ice Sheet, is an area challenging to access and is one of the harshest environments on Earth. Up until recently, long-term automated observations from Dome A (DA) were only possible with very low power instrum
Externí odkaz:
https://doaj.org/article/69c988fcebe14defb468c81de22c5cbc
PGIR 20eid (SN2020qmp): A Type IIP Supernova at 15.6 Mpc discovered by the Palomar Gattini-IR survey
Autor:
G. P. Srinivasaragavan, I. Sfaradi, J. Jencson, K. De, A. Horesh, M. M. Kasliwal, S. Tinyanont, M. Hankins, S. Schulze, M. C. B. Ashley, M. J. Graham, V. Karambelkar, R. Lau, A. A. Mahabal, A. M. Moore, E. O. Ofek, Y. Sharma, J. Sollerman, J. Soon, R. Soria, T. Travouillon, R. Walters
We present a detailed analysis of SN 2020qmp, a nearby type IIP core-collapse supernova (CCSN), discovered by the Palomar Gattini-IR (PGIR) survey in the galaxy UGC07125. We illustrate how the multiwavelength study of this event helps our general und
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d9f964fa4194ca34b1b77708dc5d0b52
http://arxiv.org/abs/2109.02159
http://arxiv.org/abs/2109.02159
Autor:
I. Andreoni, K. Ackley, J. Cooke, A. Acharyya, J. R. Allison, G. E. Anderson, M. C. B. Ashley, D. Baade, M. Bailes, K. Bannister, A. Beardsley, M. S. Bessell, F. Bian, P. A. Bland, M. Boer, T. Booler, A. Brandeker, I. S. Brown, D. A. H. Buckley, S.-W. Chang, D. M. Coward, S. Crawford, H. Crisp, B. Crosse, A. Cucchiara, M. Cupák, J. S. de Gois, A. Deller, H. A. R. Devillepoix, D. Dobie, E. Elmer, D. Emrich, W. Farah, T. J. Farrell, T. Franzen, B. M. Gaensler, D. K. Galloway, B. Gendre, T. Giblin, A. Goobar, J. Green, P. J. Hancock, B. A. D. Hartig, E. J. Howell, L. Horsley, A. Hotan, R. M. Howie, L. Hu, Y. Hu, C. W. James, S. Johnston, M. Johnston-Hollitt, D. L. Kaplan, M. Kasliwal, E. F. Keane, D. Kenney, A. Klotz, R. Lau, R. Laugier, E. Lenc, X. Li, E. Liang, C. Lidman, L. C. Luvaul, C. Lynch, B. Ma, D. Macpherson, J. Mao, D. E. McClelland, C. McCully, A. Möller, M. F. Morales, D. Morris, T. Murphy, K. Noysena, C. A. Onken, N. B. Orange, S. Osłowski, D. Pallot, J. Paxman, S. B. Potter, T. Pritchard, W. Raja, R. Ridden-Harper, E. Romero-Colmenero, E. M. Sadler, E. K. Sansom, R. A. Scalzo, B. P. Schmidt, S. M. Scott, N. Seghouani, Z. Shang, R. M. Shannon, L. Shao, M. M. Shara, R. Sharp, M. Sokolowski, J. Sollerman, J. Staff, K. Steele, T. Sun, N. B. Suntzeff, C. Tao, S. Tingay, M. C. Towner, P. Thierry, C. Trott, B. E. Tucker, P. Väisänen, V. Venkatraman Krishnan, M. Walker, L. Wang, X. Wang, R. Wayth, M. Whiting, A. Williams, T. Williams, C. Wolf, C. Wu, X. Wu, J. Yang, X. Yuan, H. Zhang, J. Zhou, H. Zovaro
Publikováno v:
Publ.Astron.Soc.Austral.
Publ.Astron.Soc.Austral., 2017, 34, pp.e069. ⟨10.1017/pasa.2017.65⟩
Publ.Astron.Soc.Austral., 2017, 34, pp.e069. 〈10.1017/pasa.2017.65〉
NASA Astrophysics Data System
Publ.Astron.Soc.Austral., 2017, 34, pp.e069. ⟨10.1017/pasa.2017.65⟩
Publ.Astron.Soc.Austral., 2017, 34, pp.e069. 〈10.1017/pasa.2017.65〉
NASA Astrophysics Data System
The discovery of the first electromagnetic counterpart to a gravitational wave signal has generated follow-up observations by over 50 facilities world-wide, ushering in the new era of multi-messenger astronomy. In this paper, we present follow-up obs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aae2ca7b815db596d403a51785846758
https://hal.science/hal-01704750
https://hal.science/hal-01704750
Autor:
John W. V. Storey, Takashi Ichikawa, C. S. Bonner, M. C. B. Ashley, Naruhisa Takato, Hirofumi Okita
Publikováno v:
Proceedings of the International Astronomical Union. 8:25-28
We carried out the first seeing measurements at Dome Fuji in the 2010–2011 austral summer. From these observations, we found that the summer seeing at Dome Fuji was 1.2″ (mean), 1.1″ (median), 0.83″ (25th percentile) and 1.5″ (75th percenti
Autor:
E. S. Rykoff, V. Mangano, S. A. Yost, R. Sari, F. Aharonian, C. W. Akerlof, M. C. B. Ashley, S. D. Barthelmy, D. N. Burrows, N. Gehrels, E. Gögüş, T. Güver, D. Horns, Ü. Kiıziıloglu, H. A. Krimm, T. A. McKay, M. Özel, A. Phillips, R. M. Quimby, G. Rowell, W. Rujopakarn, B. E. Schaefer, D. A. Smith, H. F. Swan, W. T. Vestrand, J. C. Wheeler, J. Wren, F. Yuan
Publikováno v:
The Astrophysical Journal. 638:L5-L8
The ROTSE-IIIc telescope at the H.E.S.S. site, Namibia, obtained the earliest detection of optical emission from a Gamma-Ray Burst (GRB), beginning only 21.8 s from the onset of Swift GRB 050801. The optical lightcurve does not fade or brighten signi
Autor:
E. S. Rykoff, S. A. Yost, H. A. Krimm, F. Aharonian, C. W. Akerlof, K. Alatalo, M. C. B. Ashley, S. D. Barthelmy, N. Gehrels, E. Gögüş, T. Güver, D. Horns, Ü. Kıizıiloglu, T. A. McKay, M. Özel, A. Phillips, R. M. Quimby, W. Rujopakarn, B. E. Schaefer, D. A. Smith, H. F. Swan, W. T. Vestrand, J. C. Wheeler, J. Wren
Publikováno v:
The Astrophysical Journal. 631:L121-L124
The ROTSE-IIIa telescope at Siding Spring Observatory, Australia, detected prompt optical emission from Swift GRB 050401. In this letter, we present observations of the early optical afterglow, first detected by the ROTSE-IIIa telescope 33 s after th
Context. Dome Fuji, the second highest region on the Antarctic plateau, is expected to have some of the best astronomical seeing on Earth. However, site testing at Dome Fuji is still in its very early stages. Aims. To investigate the astronomical see
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4b7c1841777155fee1af812c84bf4020
Publikováno v:
Symposium - International Astronomical Union. 213:77-79
The presence of an extrasolar planet can be revealed when it passes in front of its host star, reducing the star's apparent brightness by ∼ 1%. We are monitoring a large sample (of order 104) of stars using our own 0.5 m telescope at Siding Spring
Autor:
Zhen-Hui Lin, Qizhou Zhang, X. B. Li, Ji Yang, Zhaohui Shang, Hiroshi Matsuo, M. C. B. Ashley, Sheng-Cai Shi, Zhongwen Hu, Qijun Yao, Wen-Ying Duan, Scott Paine
Publikováno v:
2012 37th International Conference on Infrared, Millimeter, and Terahertz Waves.
China is planing to construct a 5-m THz telescope (DATE5) at Dome A, Antarctic, which is the best site on the earth for astronomical observations in the THz regime. To evaluate the atmospheric transmission at Dome A, we have developed a broadband Fou
Autor:
F. Yuan, E. S. Rykoff, B. E. Schaefer, W. Rujopakarn, T. Güver, F. Aharonian, C. W. Akerlof, M. C. B. Ashley, S. D. Barthelmy, N. Gehrels, E. Gögăüş, D. Horns, Ü. Kiziloǧlu, H. A. Krimm, T. A. Mckay, M. Özel, A. Phillips, R. M. Quimby, G. Rowell, H. F. Swan, W. T. Vestrand, J. C. Wheeler, J. Wren, Yong-Feng Huang, Zi-Gao Dai, Bing Zhang
Publikováno v:
AIP Conference Proceedings.
We report on the results of rapid responses to GRB 080330 and GRB 080413A by the ROTSE-IIIb and ROTSE-IIIc telecopes. In both cases, optical follow-up started during the prompt emission phase and recorded optical flares peaking at similar times as th