Zobrazeno 1 - 10
of 48
pro vyhledávání: '"Frank D. Ghigo"'
Autor:
Richard J. Wainscoat, Rob Landis, Robert Weryk, Detlef Koschny, M. J. Brucker, Alessandra Springmann, Hong Kyu Moon, K. E. Fast, Jon D. Giorgini, Olivier Hainaut, Boris M. Shustov, Viqar Abbasi, Frank D. Ghigo, Michael S. P. Kelley, Donovan Mathias, Davide Farnocchia, Cassandra Lejoly, Lorien Wheeler, Paul W. Chodas, Theodore Kareta, Annika Gustafsson, Myung-Jin Kim, Robert S. McMillan, William Ryan, Martin A. Slade, Vishnu Reddy, James Bauer, Ravi Teja Nallapu, David Polishook, Jessie L. Dotson, James V. Scotti, John Noonan, Joseph S. Jao, Clement G. Lee, Haris Khan Niazi, Eileen V. Ryan, J. A. Larsen, Makoto Yoshikawa, T. A. Lister, Nicolas Erasmus, Michael W. Busch, Shantanu P. Naidu, Lindley S. Johnson, David G. Gilbank, Lawrence G. Snedeker, Young-Jun Choi, Rachel B. Fernandes, Walter M. Harris, Denis G. Laurin, Amber Bonsall, David Trilling, Alberto Quijano Vodniza, Benjamin N. L. Sharkey, Amanda A. Sickafoose, Lauren Schatz, Michael Mommert, Lance A. M. Benner, Marc A. Silva, Zarah Brown, Joseph R. Masiero, Marco Micheli, E. A. Kramer, Schelte J. Bus, David J. Tholen, Marina Brozovic, Cristina A. Thomas, John P. Faucher, Lindsay R. Slick, Nicholas Moskovitz
Publikováno v:
Icarus. 326:133-150
著者人数: 69名 (所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 吉川, 真)
Number of authors: 69 (Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS): Yoshikaw
Number of authors: 69 (Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS): Yoshikaw
Autor:
P. T. Wallace, Frank D. Ghigo, Dennis Egan, J. Ray, J. J. Brandt, David T. Frayer, J. D. Nelson, Richard M. Prestage, E. White, Ronald J. Maddalena
With a 100mx110m off-axis paraboloid dish, the Green Bank Telescope (GBT) is the largest fully steerable radio telescope on Earth. A major challenge facing large ground-based radio telescopes is achieving sufficient pointing accuracy for observing at
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::93f4fa6a7beb55fb318c23dd340e2186
Autor:
Jamie McCallum, A. S. Andrianov, J. R. Rizzo, M. S. Burgin, C. García-Miró, Paweł Wolak, E. V. Kravchenko, Yu. A. Kovalev, M. V. Shatskaya, Tuomas Savolainen, James M. Anderson, Alexander B. Pushkarev, A. V. Kovalenko, G. Giovannini, N. N. Shakhvorostova, Marcello Giroletti, A. M. Kutkin, I. A. Rakhimov, Mikhail M. Lisakov, V. I. Kostenko, Norbert Bartel, Sándor Frey, I. N. Pashchenko, Magdalena Kunert-Bajraszewska, Zhi-Qiang Shen, Tapasi Ghosh, D. G. Nair, P. de Vicente, Ivan Litovchenko, Kirill Sokolovsky, J. A. Zensus, Philip G. Edwards, Antonis Polatidis, Shinji Horiuchi, Anastasios Melis, V. A. Zuga, Frank D. Ghigo, Jun Yi Koay, Tao An, P. A. Voitsik, S. F. Likhachev, J. F. H. Quick, I. A. Girin, Marcin P. Gawronski, David L. Jauncey, M. A. Kharinov, C. S. Reynolds, A. E. Melnikov, N. S. Kardashev, Simon Ellingsen, V. Yu. Avdeev, Hayley Bignall, D. V. Ivanov, R. C. Vermeulen, Leonid I. Gurvits, Chris Phillips, Yuri Y. Kovalev, M. A. Shchurov, Alexey Rudnitskiy, Carlo Migoni
Publikováno v:
Advances in Space Research
The largest Key Science Program of the RadioAstron space VLBI mission is a survey of active galactic nuclei (AGN). The main goal of the survey is to measure and study the brightness of AGN cores in order to better understand the physics of their emis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::772671b24e947bad6776e168efdff4be
https://aaltodoc.aalto.fi/handle/123456789/43103
https://aaltodoc.aalto.fi/handle/123456789/43103
Autor:
Aaron P. LaCluyze, J. B. Haislip, R. Egger, J. E. Reichart, J. R. Martin, J. P. Moore, M. Maples, N. D. Kumar, A. Foster, J. Stýblová, N. Frank, Daniel E. Reichart, A. S. Trotter, D. A. Moffett, Travis A. Berger, J. L. Stanley, Frank D. Ghigo, S. White, D. A. Dutton, Brad N. Barlow, M. L. Paggen, Sue Ann Heatherly, Vladimir Kouprianov
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 469:1299-1313
Based on five years of observations with the 40-foot telescope at Green Bank Observatory (GBO), Reichart & Stephens (2000) found that the radio source Cassiopeia A had either faded more slowly between the mid-1970s and late 1990s than Baars et al. (1
Autor:
Luisa F. Zambrano-Marin, Tarik Zegmott, Ellen S. Howell, Alan Fitzsimmons, Frank D. Ghigo, Joseph S. Jao, Michael D. Hicks, Marina Brozovic, W. D. Smythe, Benjamin Rozitis, Colin Snodgrass, Shantanu P. Naidu, Paul R. Weissman, Lance A. M. Benner, Michael C. Nolan, Patrick A. Taylor, Stephen C. Lowry, Simon F. Green, Anne Virkki, Linda A. Rodriguez-Ford, Edgard G. Rivera-Valentin, Agata Rozek, Jon D. Giorgini, L. G. Snedeker, Betzaida Aponte-Hernandez
Publikováno v:
Rozek, A, Lowry, S C, Nolan, M C, Taylor, P A, Benner, L A M, Fitzsimmons, A, Zegmott, T J, Weissman, P R, Green, S F, Rozitis, B, Snodgrass, C, Smythe, W D, Hicks, M D, Howell, E S, Virkki, A K, Aponte-Hernandez, B, Rivera-Valentin, E G, Rodriguez-Ford, L A, Zambrano-Marin, L F, Brozovic, M, Naidu, S P, Giorgini, J D, Snedeker, L G, Jao, J S & Ghigo, F D 2019, ' Shape model and spin-state analysis of PHA contact binary (85990) 1999 JV6 from combined radar and optical observations ', Astronomy & Astrophysics, vol. 631, A149 . https://doi.org/10.1051/0004-6361/201936302
Context.The potentially hazardous asteroid (85990) 1999 JV6 has been a target of previously published thermal-infrared observations and optical photometry. It has been identified as a promising candidate for possible Yarkovsky-O’Keefe-Radzievskii-P
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6bea8c04bbe5a9e47007bf5cafed2852
http://oro.open.ac.uk/68266/7/68266.pdf
http://oro.open.ac.uk/68266/7/68266.pdf
Autor:
R. L. Gao, J. B. Haislip, Stephen White, M. L. Paggen, G. I. Langston, J. B. Karlik, J. Harvey, L. M. Barnes, J. E. Reichart, A. Foster, C. P. Salemi, Daniel E. Reichart, O. H. Shaban, Frank D. Ghigo, J. R. Martin, Travis A. Berger, J. A. Duncan, S. Mazlin, M. Maples, E. M. Johnson, A. S. Trotter, D. A. Dutton, S. Bussa, Sue Ann Heatherly, Vladimir Kouprianov
Publikováno v:
The Astrophysical Journal Supplement Series. 240:12
We present a single-dish mapping algorithm with a number of advantages over traditional techniques. (1) Our algorithm makes use of weighted modeling, instead of weighted averaging, to interpolate between signal measurements. This smooths the data, bu
Autor:
Yuri Y. Kovalev, M. V. Popov, Frank D. Ghigo, V. I. Zhuravlev, Norbert Bartel, V. A. Soglasnov, V. I. Kondrat’ev
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 430:2815-2821
We have studied the statistical and polarization properties of giant pulses (GPs) emitted by the millisecond pulsar B1937+21, with high sensitivity and time resolution. The observations were made in June 2005 with the 100-m Robert C. Byrd Green Bank
Autor:
Andrei Lobanov, Kirill Sokolovsky, J. A. Zensus, J. M. Anderson, P. A. Voitsik, L. Yu. Petrov, Tapasi Ghosh, Chris Salter, Frank D. Ghigo, Alex Kraus, Jonathan D. Romney, U. Bach, Michael D. Johnson, Mikhail M. Lisakov, Yuri Y. Kovalev, Leonid I. Gurvits, Yu. A. Kovalev, David L. Jauncey, N. S. Kardashev, K. I. Kellermann
Publikováno v:
The Astrophysical Journal Letters
Inverse Compton cooling limits the brightness temperature of the radiating plasma to a maximum of $10^{11.5}$ K. Relativistic boosting can increase its observed value, but apparent brightness temperatures much in excess of $10^{13}$ K are inaccessibl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d16f05fe87887b1d7084cf0ba277ce04
http://gfzpublic.gfz-potsdam.de/pubman/item/escidoc:1586891
http://gfzpublic.gfz-potsdam.de/pubman/item/escidoc:1586891
Autor:
Brian Mason, Richard M. Prestage, Jason Ray, Kim T. Constantikes, J. Brandt, Todd R. Hunter, Frederic R. Schwab, Paul Ries, Frank D. Ghigo
Publikováno v:
Publications of the Astronomical Society of the Pacific. 123:682-691
Wind-induced pointing errors are a serious concern for large-aperture high-frequency radio telescopes. In this paper, we describe the implementation of an optical quadrant detector instrument that can detect and provide a correction signal for wind-i
Publikováno v:
Symposium - International Astronomical Union. 219:181-186
Periodicities of radio flaring activity from the Algol systems β Per and δ Lib and the RS CVn systems V711 Tau and UX Ari were determined from a continuous 5-year survey. The radio continuum fluxes at 2.3 GHz and 8.3 GHz were monitored with the NRA