Zobrazeno 1 - 10
of 66
pro vyhledávání: '"Monet, D. G."'
Autor:
Ivezić, Ž., Axelrod, T., Brandt, W. N., Burke, D. L., Claver, C. F., Connolly, A., Cook, K. H., Gee, P., Gilmore, D. K., Jacoby, S. H., Jones, R. L., Kahn, S. M., Kantor, J. P.;, Krabbendam, V., Lupton, R. H., Monet, D. G., Pinto, P. A., Saha, A., Schalk, T. L., Schneider, D. P., Strauss, M. A., Stubbs, C. W., Sweeney, D., Szalay, A., Thaler, J. J., Tyson, J. A.
Publikováno v:
Serbian Astronomical Journal, Vol 176, Pp 1-13 (2008)
In the history of astronomy, major advances in our understanding of the Universe have come from dramatic improvements in our ability to accurately measure astronomical quantities. Aided by rapid progress in information technology, current sky surveys
Externí odkaz:
https://doaj.org/article/426fa780b14e47bca161122d32383e1a
Autor:
Chambers, K. C., Magnier, E. A., Metcalfe, N., Flewelling, H. A., Huber, M. E., Waters, C. Z., Denneau, L., Draper, P. W., Farrow, D., Finkbeiner, D. P., Holmberg, C., Koppenhoefer, J., Price, P. A., Rest, A., Saglia, R. P., Schlafly, E. F., Smartt, S. J., Sweeney, W., Wainscoat, R. J., Burgett, W. S., Chastel, S., Grav, T., Heasley, J. N., Hodapp, K. W., Jedicke, R., Kaiser, N., Kudritzki, R. -P., Luppino, G. A., Lupton, R. H., Monet, D. G., Morgan, J. S., Onaka, P. M., Shiao, B., Stubbs, C. W., Tonry, J. L., White, R., Bañados, E., Bell, E. F., Bender, R., Bernard, E. J., Boegner, M., Boffi, F., Botticella, M. T., Calamida, A., Casertano, S., Chen, W. -P., Chen, X., Cole, S., Deacon, N., Frenk, C., Fitzsimmons, A., Gezari, S., Gibbs, V., Goessl, C., Goggia, T., Gourgue, R., Goldman, B., Grant, P., Grebel, E. K., Hambly, N. C., Hasinger, G., Heavens, A. F., Heckman, T. M., Henderson, R., Henning, T., Holman, M., Hopp, U., Ip, W. -H., Isani, S., Jackson, M., Keyes, C. D., Koekemoer, A. M., Kotak, R., Le, D., Liska, D., Long, K. S., Lucey, J. R., Liu, M., Martin, N. F., Masci, G., McLean, B., Mindel, E., Misra, P., Morganson, E., Murphy, D. N. A., Obaika, A., Narayan, G., Nieto-Santisteban, M. A., Norberg, P., Peacock, J. A., Pier, E. A., Postman, M., Primak, N., Rae, C., Rai, A., Riess, A., Riffeser, A., Rix, H. W., Röser, S., Russel, R., Rutz, L., Schilbach, E., Schultz, A. S. B., Scolnic, D., Strolger, L., Szalay, A., Seitz, S., Small, E., Smith, K. W., Soderblom, D. R., Taylor, P., Thomson, R., Taylor, A. N., Thakar, A. R., Thiel, J., Thilker, D., Unger, D., Urata, Y., Valenti, J., Wagner, J., Walder, T., Walter, F., Watters, S. P., Werner, S., Wood-Vasey, W. M., Wyse, R.
Pan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the $3\pi$ Steradian Survey and the Medium Deep Survey in 5 bands ($grizy_{P1}$). The mean 5$\sigma$ point source limiting sensitivities in the stacked 3$\pi$ Sterad
Externí odkaz:
http://arxiv.org/abs/1612.05560
Publikováno v:
Steward Observatory Parker Library SO QB 4 .S752 ARCH
Externí odkaz:
http://hdl.handle.net/10150/623908
http://arizona.openrepository.com/arizona/handle/10150/623908
http://arizona.openrepository.com/arizona/handle/10150/623908
Autor:
Wang, P. F., Chen, W. P., Lin, C. C., Pandey, A. K., Huang, C. K., Panwar, N., Lee, C. H., Tsai, M. F., Tang, C. -H., Goldman, B., Burgett, W. S., Chambers, K. C., Draper, P. W., Flewelling, H., Grav, T., Heasley, J. N., Hodapp, K. W., Huber, M. E., Jedicke, R., Kaiser, N., Kudritzki, R. -P., Luppino, G. A., Lupton, R. H., Magnier, E. A., Metcalfe, N., Monet, D. G., Morgan, J. S., Onaka, P. M., Price, P. A., Stubbs, C. W., Sweeney, W., Tonry, J. L., Wainscoat, R. J., Waters, C.
Membership identification is the first step to determine the properties of a star cluster. Low-mass members in particular could be used to trace the dynamical history, such as mass segregation, stellar evaporation, or tidal stripping, of a star clust
Externí odkaz:
http://arxiv.org/abs/1401.7424
Autor:
Sanders, Nathan E., Soderberg, A. M., Valenti, S., Foley, R. J., Chornock, R., Chomiuk, L., Berger, E., Smartt, S., Hurley, K., Barthelmy, S. D., Levesque, E. M., Narayan, G., Kirshner, R. P., Botticella, M. T., Briggs, M. S., Connaughton, V., Terada, Y., Gehrels, N., Golenetskii, S., Mazets, E., Cline, T., von Kienlin, A., Boynton, W., Chambers, K. C., Grav, T., Heasley, J. N., Hodapp, K. W., Jedicke, R., Kaiser, N., Kudritzki, R. -P., Luppino, G. A., Lupton, R. H., Magnier, E. A., Monet, D. G., Morgan, J. S., Onaka, P. M., Price, P. A., Stubbs, C. W., Tonry, J. L., Wainscoat, R. J., Waterson, M. F.
Publikováno v:
Astrophysical Journal 756 (2012) 184S
We report on our serendipitous pre-discovery detection and detailed follow-up of the broad-lined Type Ic supernova (SN) 2010ay at z = 0.067 imaged by the Pan-STARRS1 3pi survey just ~4 days after explosion. The SN had a peak luminosity, M_R ~ -20.2 m
Externí odkaz:
http://arxiv.org/abs/1110.2363
Autor:
Girard, T. M., van Altena, W. F., Zacharias, N., Vieira, K., Casetti-Dinescu, D. I., Castillo, D., Herrera, D., Lee, Y. S., Beers, T. C., Monet, D. G., Lopez, C. E.
We present the fourth installment of the Yale/San Juan Southern Proper Motion Catalog, SPM4. The SPM4 contains absolute proper motions, celestial coordinates, and (B,V) photometry for over 103 million stars and galaxies between the south celestial po
Externí odkaz:
http://arxiv.org/abs/1104.5708
Autor:
Pastorello, A., Smartt, S. J., Botticella, M. T., Maguire, K., Fraser, M., Smith, K., Kotak, R., Magill, L., Valenti, S., Young, D. R., Gezari, S., Bresolin, F., Kudritzki, R., Howell, D. A., Rest, A., Metcalfe, N., Mattila, S., Kankare, E., Huang, K. Y., Urata, Y., Burgett, W. S., Chambers, K. C., Dombeck, T., Flewelling, T., Grav, T., Heasley, J. N., Hodapp, K. W., Kaiser, N., Luppino, G. A., Lupton, R. H., Magnier, E. A., Monet, D. G., Morgan, J. S., Onaka, P. M., Price, P. A., Rhoads, P. H., Siegmund, W. A., Stubbs, C. W., Sweeney, W. E., Tonry, J. L., Wainscoat, R. J., Waterson, M. F., Waters, C., Wynn-Williams, C. G.
Recent searches by unbiased, wide-field surveys have uncovered a group of extremely luminous optical transients. The initial discoveries of SN 2005ap by the Texas Supernova Search and SCP-06F6 in a deep Hubble pencil beam survey were followed by the
Externí odkaz:
http://arxiv.org/abs/1008.2674
Autor:
Gezari, S., Rest, A., Huber, M. E., Narayan, G., Forster, K., Neill, J. D., Martin, D. C., Valenti, S., Smartt, S. J., Chornock, R., Berger, E., Soderberg, A. M., Mattila, S., Kankare, E., Burgett, W. S., Chambers, K. C., Dombeck, T., Grav, T., Heasley, J. N., Hodapp, K. W., Jedicke, R., Kaiser, N., Kudritzki, R., Luppino, G., Lupton, R. H., Magnier, E. A., Monet, D. G., Morgan, J. S., Onaka, P. M., Price, P. A., Rhoads, P. H., Siegmund, W. A., Stubbs, C. W., Tonry, J. L., Wainscoat, R. J., Waterson, M. F., Wynn-Williams, C. G.
Publikováno v:
Astrophys.J. 720 (2010) L77-L81
We present the early UV and optical light curve of Type IIP supernova (SN) 2010aq at z=0.0862, and compare it to analytical models for thermal emission following SN shock breakout in a red supergiant star. SN 2010aq was discovered in joint monitoring
Externí odkaz:
http://arxiv.org/abs/1007.4551
Autor:
Botticella, M. T., Trundle, C., Pastorello, A., Rodney, S., Rest, A., Gezari, S., Smartt, S. J., Narayan, G., Huber, M. E., Tonry, J. L., Young, D., Smith, K., Bresolin, F., Valenti, S., Kotak, R., Mattila, S., Kankare, E., Wood-Vasey, W. M., Riess, A., Neill, J. D., Forster, K., Martin, D. C., Stubbs, C. W., Burgett, W. S., Chambers, K. C., Dombeck, T., Flewelling, H., Grav, T., Heasley, J. N., Hodapp, K. W., Kaiser, N., Kudritzki, R., Luppino, G., Lupton, R. H., Magnier, E. A., Monet, D. G., Morgan, J. S., Onaka, P. M., Price, P. A., Rhoads, P. H., Siegmund, W. A., Sweeney, W. E., Wainscoat, R. J., Waters, C., Waterson, M. F., Wynn-Williams, C. G.
We present photometric and spectroscopic observations of a luminous type IIP Supernova 2009kf discovered by the Pan-STARRS 1 (PS1) survey and detected also by GALEX. The SN shows a plateau in its optical and bolometric light curves, lasting approxima
Externí odkaz:
http://arxiv.org/abs/1001.5427
Autor:
Batalha, N. M., Borucki, W. J., Koch, D. G., Bryson, S. T., Haas, M. R., Brown, T. M., Caldwell, D. A., Gilliland, R. L., Latham, D. W., Meibom, S., Monet, D. G.
The Kepler Mission began its 3.5-year photometric monitoring campaign in May 2009 on a select group of approximately 150,000 stars. The stars were chosen from the ~half million in the field of view that are brighter than 16th magnitude. The selection
Externí odkaz:
http://arxiv.org/abs/1001.0349