Zobrazeno 1 - 10
of 227
pro vyhledávání: '"Unwin S"'
Autor:
Moullet, A., Kataria, T., Lis, D., Unwin, S., Hasegawa, Y., Mills, E., Battersby, C., Roc, A., Meixner, M.
PRIMA (The PRobe for-Infrared Mission for Astrophysics) is a concept for a far-infrared (IR) observatory. PRIMA features a cryogenically cooled 1.8 m diameter telescope and is designed to carry two science instruments enabling ultra-high sensitivity
Externí odkaz:
http://arxiv.org/abs/2310.20572
Publikováno v:
In Journal of Infection November 2024 89(5)
Autor:
Danchi, W. C., Barry, R. K., Lopez, B., Rinehart, S., Absil, O., Augereau, J. -C., Beust, H., Bonfils, X., Borde, P., Defrere, Denis, Kern, Pierre, Lawson, P., Leger, A., Monin, J. -L., Mourard, D., Ollivier, M., Petrov, R., Traub, W., Unwin, S., Vakili, F.
The Fourier-Kelvin Stellar Interferometer (FKSI) is a mission concept for a nulling interferometer for the near-to-mid-infrared spectral region. FKSI is conceived as a mid-sized strategic or Probe class mission. FKSI has been endorsed by the Exoplane
Externí odkaz:
http://arxiv.org/abs/0912.2672
Autor:
Kasting, J., Traub, W., Roberge, A., Leger, A., Schwartz, A., Wooten, A., Vosteen, A., Lo, A., Brack, A., Tanner, A., Coustenis, A., Lane, B., Oppenheimer, B., Mennesson, B., Lopez, B., Grillmair, C., Beichman, C., Cockell, C., Hanot, C., McCarthy, C., Stark, C., Marois, C., Aime, C., Angerhausen, D., Montes, D., Wilner, D., Defrere, D., Mourard, D., Lin, D., Kite, E., Chassefiere, E., Malbet, F., Tian, F., Westall, F., Illingworth, G., Vasisht, G., Serabyn, G., Marcy, G., Bryden, G., White, G., Laughlin, G., Torres, G., Hammel, H., Ferguson, H., Shibai, H., Rottgering, H., Surdej, J., Wiseman, J., Ge, J., Bally, J., Krist, J., Monnier, J., Trauger, J., Horner, J., Catanzarite, J., Harrington, J., Nishikawa, J., Stapelfeldt, K., von Braun, K., Biazzo, K., Carpenter, K., Balasubramanian, K., Kaltenegger, L., Postman, M., Spaans, M., Turnbull, M., Levine, M., Burchell, M., Ealey, M., Kuchner, M., Marley, M., Dominik, M., Mountain, M., Kenworthy, M., Muterspaugh, M., Shao, M., Zhao, M., Tamura, M., Kasdin, N., Haghighipour, N., Kiang, N., Elias, N., Woolf, N., Mason, N., Absil, O., Guyon, O., Lay, O., Borde, P., Fouque, P., Kalas, P., Lowrance, P., Plavchan, P., Hinz, P., Kervella, P., Chen, P., Akeson, R., Soummer, R., Waters, R., Barry, R., Kendrick, R., Brown, R., Vanderbei, R., Woodruff, R., Danner, R., Allen, R., Polidan, R., Seager, S., MacPhee, S., Hosseini, S., Metchev, S., Kafka, S., Ridgway, S., Rinehart, S., Unwin, S., Shaklan, S., Brummelaar, T. ten, Mazeh, T., Meadows, V., Weiss, W., Danchi, W., Ip, W., Rabbia, Y.
Over 300 extrasolar planets (exoplanets) have been detected orbiting nearby stars. We now hope to conduct a census of all planets around nearby stars and to characterize their atmospheres and surfaces with spectroscopy. Rocky planets within their sta
Externí odkaz:
http://arxiv.org/abs/0911.2936
Autor:
Shao, M., Marcy, G., Unwin, S., Allen, R., Beichman, C., Catanzarite, J., Chaboyer, B., Ciardi, D., Edberg, S. J., Gallagher, D., Gould, A., Henry, T., Johnston, K., Kulkarni, S., Law, N., Majewski, S., Marr, J., Pan, X., Shaklan, S., Shaya, E., Tanner, A., Tomsick, J., Wehrle, A., Worthey, G.
The past two Decadal Surveys in Astronomy and Astrophysics recommended the completion of a space-based interferometry mission, known today as SIM PlanetQuest, for its unique ability to detect and characterize nearby rocky planets (Bahcall 1991, McKee
Externí odkaz:
http://arxiv.org/abs/0704.0952
Autor:
Millan-Gabet, R., Monnier, J. D., Akeson, R. L., Hartmann, L., Berger, J. -P., Tannirkulam, A., Melnikov, S., Billmeier, R., Calvet, N., D'Alessio, P., Hillenbrand, L. A., Kuchner, M., Traub, W. A., Tuthill, P. G., Beichman, C., Boden, A., Booth, A., Colavita, M., Creech-Eakman, M., Gathright, J., Hrynevych, M., Koresko, C., Mignant, D. Le, Ligon, R., Mennesson, B., Neyman, C., Sargent, A., Shao, M., Swain, M., Thompson, R., Unwin, S., van Belle, G., Vasisht, G., Wizinowich, P.
Publikováno v:
Astrophys.J.641:547-555,2006
We present new K-band long baseline interferometer observations of three young stellar objects of the FU Orionis class, V1057 Cyg, V1515 Cyg and Z CMa-SE, obtained at the Keck Interferometer during its commissioning science period. The interferometer
Externí odkaz:
http://arxiv.org/abs/astro-ph/0512230
Autor:
Swain, M., Vasisht, G., Akeson, R., Monnier, J., Millan-Gabet, R., Serabyn, E., Creech-Eakman, M., van Belle, G., Beletic, J., Beichman, C., Boden, A., Booth, A., Colavita, M., Gathright, J., Hrynevych, M., Koresko, C., Mignant, D. Le, Ligon, R., Mennesson, B., Neyman, C., Sargent, A., Shao, M., Thompson, R., Unwin, S., Wizinowich, P.
Publikováno v:
Astrophys.J.596:L163-L166,2003
We report novel, high-angular resolution interferometric measurements that imply the near-infrared nuclear emission in NGC 4151 is unexpectedly compact. We have observed the nucleus of NGC 4151 at 2.2 microns using the two 10-meter Keck telescopes as
Externí odkaz:
http://arxiv.org/abs/astro-ph/0308513
Autor:
Leisawitz, D., Armstrong, T., Benford, D., Blain, A., Danchi, K. Borne W., Evans, N., Gardner, J., Gezari, D., Harwit, M., Kashlinsky, A., Langer, W., Lawrence, C., Lawson, P., Lester, D., Mather, J., Moseley, S. H., Mundy, L., Rieke, G., Rinehart, S., Shao, M., Silverberg, R., Spergel, D., Staguhn, J., Swain, M., Traub, W., Unwin, S., Wright, E., Yorke, H.
The question "How did we get here and what will the future bring?" captures the human imagination and the attention of the National Academy of Science's Astronomy and Astrophysics Survey Commitee (AASC). Fulfillment of this "fundamental goal" require
Externí odkaz:
http://arxiv.org/abs/astro-ph/0202085
Autor:
Walker, R. C., Benson, J. M., Unwin, S. C., Lystrup, M. B., Hunter, T. R., Pilbratt, G., Hardee, P. E.
Results are presented from long term VLBI monitoring of the parsec-scale radio jet in 3C120, primarily at 5 and 1.7 GHz. Numerous superluminal features are followed, some over large fractional distances from the core. The speeds of the features are n
Externí odkaz:
http://arxiv.org/abs/astro-ph/0103379
Autor:
Wehrle, A. E., Piner, B. G., Unwin, S. C., Zook, A. C., Xu, W., Marscher, A. P., Terasranta, H., Valtaoja, E.
Publikováno v:
Astrophys.J.Suppl.133:297-320,2001
We present results of long-term high-frequency VLBI monitoring of the relativistic jet in 3C279, consisting of 18 epochs at 22 GHz from 1991 to 1997 and 10 epochs at 43 GHz from 1995 to 1997. Three major results of this study are: apparent speeds mea
Externí odkaz:
http://arxiv.org/abs/astro-ph/0008458