Zobrazeno 1 - 10
of 1 515
pro vyhledávání: '"Ingalls, J"'
Autor:
Ducrot, Elsa, Gillon, M., Delrez, L., Agol, E., Rimmer, P., Turbet, M., Günther, M. N., Demory, B-O., Triaud, A. H. M. J., Bolmont, E., Burgasser, A., Carey, S. J., Ingalls, J. G., Jehin, E., Leconte, J., Lederer, S. M., Queloz, D., Raymond, S. N., Selsis, F., Van Grootel, V., de Wit, J.
Publikováno v:
A&A 640, A112 (2020)
With more than 1000 hours of observation from Feb 2016 to Oct 2019, the Spitzer Exploration Program Red Worlds (ID: 13067, 13175 and 14223) exclusively targeted TRAPPIST-1, a nearby (12pc) ultracool dwarf star orbited by seven transiting Earth-sized
Externí odkaz:
http://arxiv.org/abs/2006.13826
Autor:
Fazio, G. G., Hora, J. L., Witzel, G., Willner, S. P., Ashby, M. L. N., Baganoff, F., Becklin, E., Carey, S., Haggard, D., Gammie, C., Ghez, A., Gurwell, M. A., Ingalls, J., Marrone, D., Morris, M. R., Smith, H. A.
Sgr A*, the supermassive black hole (SMBH) at the center of our Milky Way Galaxy, is known to be a variable source of X-ray, near-infrared (NIR), and submillimeter (submm) radiation and therefore a prime candidate to study the electromagnetic radiati
Externí odkaz:
http://arxiv.org/abs/1807.07599
Autor:
Witzel, G., Martinez, G., Hora, J., Willner, S. P., Morris, M. R., Gammie, C., Becklin, E. E., Ashby, M. L. N., Baganoff, F., Carey, S., Do, T., Fazio, G. G., Ghez, A., Glaccum, W. J., Haggard, D., Herrero-Illana, R., Ingalls, J., Narayan, R., Smith, H. A.
Sagittarius A* (Sgr A*) is the variable radio, near-infrared (NIR), and X-ray source associated with accretion onto the Galactic center black hole. We present an analysis of the most comprehensive NIR variability dataset of Sgr A* to date: eight 24-h
Externí odkaz:
http://arxiv.org/abs/1806.00479
Autor:
Stauffer, J. R., Marley, M. S., Gizis, J. E., Rebull, L. M., Carey, S. J., Krick, J., Ingalls, J. G., Lowrance, P., Glaccum, W., Kirkpatrick, J. D., Simon, A. A., Wong, M. H.
We have used the Spitzer Space Telescope in February 2016 to obtain high cadence, high signal-to-noise, 17-hour duration light curves of Neptune at 3.6 and 4.5 $\mu$m. The light curve duration was chosen to correspond to the rotation period of Neptun
Externí odkaz:
http://arxiv.org/abs/1608.07198
Autor:
Krick, J. E., Ingalls, J., Carey, S., von Braun, K., Kane, S. R., Ciardi, D., Plavchan, P., Wong, I., Lowrance, P.
Motivated by a high Spitzer IRAC oversubscription rate, we present a new technique of randomly and sparsely sampling phase curves of hot Jupiters. Snapshot phase curves are enabled by technical advances in precision pointing as well as careful charac
Externí odkaz:
http://arxiv.org/abs/1603.03383
Autor:
Hora, J. L., Witzel, G., Ashby, M. L. N., Becklin, E. E., Carey, S., Fazio, G. G., Ghez, A., Ingalls, J., Meyer, L., Morris, M. R., Smith, H. A., Willner, S. P.
We present the first detection from the Spitzer Space Telescope of 4.5 micron variability from Sgr A*, the emitting source associated with the Milky Way's central black hole. The >23 hour continuous light curve was obtained with the IRAC instrument i
Externí odkaz:
http://arxiv.org/abs/1408.1951
Autor:
Lisse, C. M., VanCleve, J., Adams, A. C., Fernández, Y. R., Farnham, T. L., Armus, L., Grillmair, C. J., Ingalls, J., Belton, M. J. S., Groussin, O., McFadden, L. A., Meech, K. J., Schultz, P. H., Clark, B. C., Feaga, L. M., Sunshine, J. M.
Publikováno v:
Science, 2006 Aug 01. 313(5787), 635-640.
Externí odkaz:
https://www.jstor.org/stable/3846742
Autor:
Carey, S. J., Noriega-Crespo, A., Mizuno, D. R., Shenoy, S., Paladini, R., Kraemer, K. E., Price, S. D., Flagey, N., Ryan, E., Ingalls, J. G., Kuchar, T. A., Pinheiro Gonçalves, Daniela, Indebetouw, R., Billot, N., Marleau, F. R., Padgett, D. L., Rebull, L. M., Bressert, E., Ali, Babar, Molinari, S., Martin, P. G., Berriman, G. B., Boulanger, F., Latter, W. B., Miville-Deschenes, M. A., Shipman, R., Testi, L.
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2009 01. 121(875), 76-97.
Externí odkaz:
https://www.jstor.org/stable/10.1086/596581
Autor:
Mennesson, B., Bailey, V. P., Zellem, R., Hildebrandt, S., Ygouf, M., Rhodes, J., Zimmerman, N., Kasdin, J., Macintosh, B., Turnbull, M., Douglas, E., Mandell, A., Maier, E. R., Nemati, B., Gonzalez, G., Cady, E., Kern, B., Krist, J., Heydorff, K., Luchik, T., Mok, F., Morrissey, P., Pobereszhskiy, I., Riggs, A. J., Shi, F., Zhao, F., Akeson, R., Armus, L., Ingalls, J., Lowrance, P., Meshkat, T.
Publikováno v:
Techniques and Instrumentation for Detection of Exoplanets X.
The Nancy Grace Roman Space Telescope (formally WFIRST) will be launched in the mid-2020’s with an onboard coronagraph instrument which will serve as a technology demonstrator for exoplanet direct imaging. The Roman Coronagraph will be capable of d
Autor:
Coyle, Laura E., Matsuura, Shuji, Perrin, Marshall D., Mennesson, B., Bailey, V. P., Zellem, R., Hildebrandt, S., Ygouf, M., Rhodes, J., Zimmerman, N., Nemati, B., Gonzalez, G., Cady, E., Kern, B., Koch, T., Krist, J., Heydorff, K., Luchik, T., Mok, F., Morrissey, P., Poberezhskiy, I., Riggs, A. J., Shi, F., Zhao, F., Akeson, R., Armus, L., Greenbaum, A., Ingalls, J., Lowrance, P.
Publikováno v:
Proceedings of SPIE; August 2022, Vol. 12180 Issue: 1 p121801W-121801W-13, 12058313p