Zobrazeno 1 - 10
of 84
pro vyhledávání: '"Odewahn, S. C."'
Autor:
Verley, S., Leon, S., Verdes-Montenegro, L., Combes, F., Sabater, J., Sulentic, J., Bergond, G., Espada, D., Lisenfeld, U., Odewahn, S. C.
The role of the environment on galaxy evolution is still not fully understood. In order to quantify and set limits on the role of nurture one must identify and study a sample of isolated galaxies. The AMIGA project "Analysis of the Interstellar Mediu
Externí odkaz:
http://arxiv.org/abs/0909.1511
Autor:
Verley, S., Leon, S., Verdes-Montenegro, L., Combes, F., Sabater, J., Sulentic, J., Bergond, G., Espada, D., Garcia, E., Lisenfeld, U., Odewahn, S. C.
The AMIGA project aims to build a well defined and statistically significant reference sample of isolated galaxies in order to estimate the environmental effects on the formation and evolution of galaxies. The goal of this paper is to provide a measu
Externí odkaz:
http://arxiv.org/abs/0706.2555
Autor:
Verley, S., Odewahn, S. C., Verdes-Montenegro, L., Leon, S., Combes, F., Sulentic, J., Bergond, G., Espada, D., Garcia, E., Lisenfeld, U., Sabater, J.
Studies of the effects of environment on galaxy properties and evolution require well defined control samples. Such isolated galaxy samples have up to now been small or poorly defined. The AMIGA project (Analysis of the interstellar Medium of Isolate
Externí odkaz:
http://arxiv.org/abs/0705.0479
Autor:
Lopes, P. A. A., de Carvalho, R. R., Capelato, H. V., Gal, R. R., Djorgovski, S. G., Brunner, R. J., Odewahn, S. C., Mahabal, A. A.
Publikováno v:
Astrophys.J.648:209-229,2006
We present a comparison of optical and X-ray properties of galaxy clusters in the northern sky. We determine the recovery rate of X-ray detected clusters in the optical as a function of richness, redshift and X-ray luminosity, showing that the missed
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605292
Autor:
Lopes, P. A. A., de Carvalho, R. R., Gal, R. R., Djorgovski, S. G., Odewahn, S. C., Mahabal, A. A., Brunner, R. J.
Publikováno v:
Astron.J.128:1017-1045, 2004
We present an optically selected galaxy cluster catalog from ~ 2,700 square degrees of the Digitized Second Palomar Observatory Sky Survey (DPOSS), spanning the redshift range 0.1 < z < 0.5, providing an intermediate redshift supplement to the previo
Externí odkaz:
http://arxiv.org/abs/astro-ph/0406123
Autor:
Brunner, Robert J., Hall, Patrick B., Djorgovski, S. George, Gal, R. R., Mahabal, A. A., Lopes, P. A. A., de Carvalho, R. R., Odewahn, S. C., Castro, S., Thompson, D., Chaffee, F., Darling, J., Desai, V.
Publikováno v:
Astron.J. 126 (2003) 53
With the recent release of large (i.e., > hundred million objects), well-calibrated photometric surveys, such as DPOSS, 2MASS, and SDSS, spectroscopic identification of important targets is no longer a simple issue. In order to enhance the returns fr
Externí odkaz:
http://arxiv.org/abs/astro-ph/0304166
Autor:
Gal, R. R., de Carvalho, R. R., Lopes, P. A. A., Djorgovski, S. G., Brunner, R. J., Mahabal, A. A., Odewahn, S. C.
We present a new, objectively defined catalog of candidate galaxy clusters based on the galaxy catalogs from the Digitized Second Palomar Observatory Sky Survey (DPOSS). This cluster catalog, derived from the best calibrated plates in the high latitu
Externí odkaz:
http://arxiv.org/abs/astro-ph/0301274
Autor:
Gal, R. R., de Carvalho, R. R., Odewahn, S. C., Djorgovski, S. G., Mahabal, A. A., Brunner, R. J., Lopes, P. A. A.
We present the photometric calibration technique for the Digitized Second Palomar Observatory Sky Survey (DPOSS), used to create seamless catalogs of calibrated objects over large sky areas. After applying a correction for telescope vignetting, the e
Externí odkaz:
http://arxiv.org/abs/astro-ph/0210298
Autor:
Windhorst, R. A., Taylor, V. A., Jansen, R. A., Odewahn, S. C., Chiarenza, C. A. T., Conselice, C. J., de Grijs, R., de Jong, R. S., MacKenty, J. W., Eskridge, P. B., Frogel, J. A., Gallagher III, J. S ., Hibbard, J. E., Matthews, L. D., O'Connell, R. W.
Publikováno v:
Astrophys.J.Suppl. 143 (2002) 113-158
(Abbreviated) We present an imaging survey of 37 nearby galaxies observed with HST/WFPC2 in the mid-UV F300W filter and in F814W. 11 galaxies were also imaged in F255W. These galaxies were selected to be detectable with WFPC2 in one orbit, and cover
Externí odkaz:
http://arxiv.org/abs/astro-ph/0204398
We use automated surface photometry and pattern classification techniques to morphologically classify galaxies. The two-dimensional light distribution of a galaxy is reconstructed using Fourier series fits to azimuthal profiles computed in concentric
Externí odkaz:
http://arxiv.org/abs/astro-ph/0110275