Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Groth, E. J."'
Autor:
Faber, S. M., Willmer, C. N. A., Wolf, C., Koo, D. C., Weiner, B. J., Newman, J. A., Im, M., Coil, A. L., Conroy, C., Cooper, M. C., Davis, M., Finkbeiner, D. P., Gerke, B. F., Gebhardt, K., Groth, E. J., Guhathakurta, P., Harker, J., Kaiser, N., Kassin, S., Kleinheinrich, M., Konidaris, N. P., Lin, L., Luppino, G., Madgwick, D. S., Noeske, K. Meisenheimer K. G., Phillips, A. C., Sarajedini, V. L., Simard, L., Szalay, A. S., Vogt, N. P., Yan, R.
Publikováno v:
Astrophys.J.665:265-294,2007
The DEEP2 and COMBO-17 surveys are used to study the evolution of the luminosity function of red and blue galaxies to $z \sim 1$. Schechter function fits show that, since $z = 1$, $M^*_B$ dims by $\sim$ 1.3 mag per unit redshift for both color classe
Externí odkaz:
http://arxiv.org/abs/astro-ph/0506044
Publikováno v:
Astrophys.J.572:L131-L134,2002
Weak lensing by large-scale structure provides a direct measurement of matter fluctuations in the universe. We report a measurement of this `cosmic shear' based on 271 WFPC2 archival images from the Hubble Space Telescope Medium Deep Survey (MDS). Ou
Externí odkaz:
http://arxiv.org/abs/astro-ph/0203131
Weak lensing by large-scale structure provides a unique method to directly measure matter fluctuations in the universe, and has recently been detected from the ground. Here, we report the first detection of this `cosmic shear' based on space-based im
Externí odkaz:
http://arxiv.org/abs/astro-ph/0101213
Autor:
Groth, E. J., Kristian, Jerome A., Ewald, S. P., Hester, J. Jeff, Holtzman, Jon A., Lauer, Tod R., Light, Robert M., Shaya, Edward J., Baum, William A., Campbell, Bel, Code, Arthur, Currie, Douglas G., Danielson, G. Edward, Faber, S. M., Hoessel, John G., Hunter, Deidre, Kelsall, T., Lynds, Roger, Mackie, Glen, Monet, David G., O'Neill, Earl J., Jr., Schneider, Donald P., Seidelmann, P. Kenneth, Smith, Brad, Westphal, James A.
The data are three exposures in PC6 through F785LP obtained on March 3, 1991. The exposure times are 120, 400, and 400 seconds. The data are reduced with the "standard" WFPC reduction scheme: A-to-D correction, DC bias subtraction, AC bias subtractio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od________38::71de2c835cf1d1ab4c79e8e8b9e142d2
https://resolver.caltech.edu/CaltechAUTHORS:20141126-105710198
https://resolver.caltech.edu/CaltechAUTHORS:20141126-105710198
Akademický článek
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Autor:
Faber, S. M., Willmer, C. N. A., Wolf, C., Koo, D. C., Weiner, B. J., Newman, J. A., Im, M., Coil, A. L., Conroy, C., Cooper, M. C., Davis, M., Finkbeiner, D. P., Gerke, B. F., Gebhardt, K., Groth, E. J., Guhathakurta, P., Harker, J., Kaiser, N., Kassin, S., Kleinheinrich, M.
Publikováno v:
Astrophysical Journal; 8/10/2007, Vol. 665 Issue 1, p265-294, 30p
Autor:
Groth, E. J.
Publikováno v:
Annals of the New York Academy of Sciences; 1973, Vol. 224 Issue 1, p184-189, 6p