Zobrazeno 1 - 10
of 3 319
pro vyhledávání: '"Cram, L."'
Autor:
Dietz, Karl-Josef
Publikováno v:
The New Phytologist, 1999 Dec 01. 144(3), 419-420.
Externí odkaz:
https://www.jstor.org/stable/2588876
Publikováno v:
Mon.Not.Roy.Astron.Soc.367:331-338,2006
We estimate the star-formation rates and the stellar masses of the Extremely Red objects (EROs) detected in a 180arcmin2 Ks-band survey (Ks~20mag). This sample is complemented by sensitive 1.4GHz radio observations (12micro-Jy; 1sigma rms) and multiw
Externí odkaz:
http://arxiv.org/abs/astro-ph/0512138
Publikováno v:
Astron.J.131:1216-1230,2006
We present optical and X-ray identifications for the sixty-four radio sources in the GOODS-S ACS field revealed in the ATCA 1.4 GHz survey of the Chandra Deep Field South. Optical identifications are made using the ACS images and catalogs, while the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0510774
Publikováno v:
Astrophys.J.620:584-594,2005
In this paper we explore the clustering properties and the environment of the Extremely Red Objects (EROs; I-K>4mag) detected in a ~180arcmin^2 deep (Ks~20mag) Ks-band survey of a region within the Phoenix Deep Survey, an on-going multiwavelength pro
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411572
Autor:
Afonso, J., Georgakakis, A., Almeida, C., Hopkins, A. M., Cram, L. E., Mobasher, B., Sullivan, M.
Publikováno v:
Astrophys.J.624:135-154,2005
The Phoenix Deep Survey is a multi-wavelength survey based on deep 1.4 GHz radio imaging, reaching well into the sub-100 microJy level. One of the aims of this survey is to characterize the sub-mJy radio population, exploring its nature and evolution
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411578
The radio properties of hard (2-8keV) X-ray selected sources are explored by combining a single 50ks XMM-Newton pointing with the ultra-deep and homogeneous Phoenix radio (1.4GHz) survey (Hopkins et al. 2003). A total of 43 sources are detected above
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407078
Insensitive to dust obscuration, radio wavelengths are ideal to study star-forming galaxies free of dust induced biases. Using data from the Phoenix Deep Survey, we have identified a sample of star-forming extremely red objects (EROs). Stacking of th
Externí odkaz:
http://arxiv.org/abs/astro-ph/0312117
The Phoenix Deep Survey (PDS) is a multiwavelength survey based on deep 1.4 GHz radio observations used to identify a large sample of star forming galaxies to z=1. Photometric redshifts are estimated for the optical counterparts to the radio-detected
Externí odkaz:
http://arxiv.org/abs/astro-ph/0312035
Autor:
Chan, B. H. P., Cram, L. E., Sadler, E. M., Killeen, N. E. B., Jackson, C. A., Mobasher, B., Ekers, R. D.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 352 (2004) 1245
The Australia Telescope Compact Array (ATCA) has been used to survey at 1.4GHz, a small region (< 3 sq deg) overlapping with the 2dF Galaxy Redshift Survey (Colless et al. 2001, MNRAS, 328, 1039). We surveyed with a varying radio sensitivity, ranging
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310315
The Phoenix Deep Survey (PDS) is a multiwavelength survey based on deep 1.4 GHz radio observations used to identify a large sample of star forming galaxies to z=1. Here we present an exploration of the evolutionary constraints on the star-forming pop
Externí odkaz:
http://arxiv.org/abs/astro-ph/0309147