Zobrazeno 1 - 10
of 39
pro vyhledávání: '"Eales, Stephen"'
Autor:
Aretxaga, Itziar, Hughes, David H., Coppin, Kristen, Mortier, Angela M. J., Wagg, Jeff, Dunlop, James S., Chapin, Edward L., Eales, Stephen A., Gaztanaga, Enrique, Halpern, Mark, Ivison, Rob J., van Kampen, Eelco, Scott, Douglas, Serjeant, Stephen, Smail, Ian, Babbedge, Thomas, Benson, Andrew J., Chapman, Scott, Clements, David L., Dunne, Loretta, Dye, Simon, Farrah, Duncan, Jarvis, Matthew J., Mann, Robert G., Pope, Alexandra, Priddey, Robert, Rawlings, Steve, Seigar, Marc, Silva, Laura, Simpson, Chris, Vaccari, Mattia
Publikováno v:
Mon.Not.Roy.Astron.Soc.379:1571-1588,2007
We present the redshift distribution of the SHADES galaxy population based on the rest-frame radio-mm-FIR colours of 120 robustly detected 850um sources in the Lockman Hole East (LH) and Subaru XMM-Newton Deep Field (SXDF). The redshift distribution
Externí odkaz:
http://arxiv.org/abs/astro-ph/0702503
Publikováno v:
Mon.Not.Roy.Astron.Soc.379:1042-1048,2007
We use the results of the SCUBA Local Universe Galaxy Survey, a submillimetre survey of galaxies in the nearby Universe, to investigate the relationship between the far-infrared--submillimetre and radio emission of galaxies at both low and high redsh
Externí odkaz:
http://arxiv.org/abs/astro-ph/0609198
Publikováno v:
Mon.Not.Roy.Astron.Soc.364:1253-1285,2005
We present new results from the SCUBA Local Universe Galaxy Survey (SLUGS), the first large systematic submillimetre survey of the local Universe. Since our initial survey of a sample of 104 IRAS-selected galaxies we have now completed a survey of a
Externí odkaz:
http://arxiv.org/abs/astro-ph/0510768
We present new results from the SCUBA Local Universe Galaxy Survey, the first large statistical submillimetre survey of the local Universe. Following our initial survey of a sample of 104 IRAS-selected galaxies we now present the results of a sample
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411067
We discuss the progress of the SCUBA Local Universe Galaxy Survey (SLUGS), the first large, statistical sub-mm survey of the local universe. Since our original survey of a sample of 104 IRAS-selected galaxies we have recently completed a sample of 78
Externí odkaz:
http://arxiv.org/abs/astro-ph/0408466
Publikováno v:
Nature 424:285-287,2003
Large amounts of dust have recently been discovered in high-z galaxies and QSOs. The stellar winds produced by AGB stars are thought to be the main source of dust in galaxies, but they cannot produce that dust on a short enough timescale (<1 Gyr) to
Externí odkaz:
http://arxiv.org/abs/astro-ph/0307320
Autor:
Waskett, Timothy J., Eales, Stephen A., Gear, Walter K., Puchnarewicz, Elizabeth M., Lilly, Simon, Flores, Hector, Webb, Tracy, Clements, David, Stevens, Jason A., Thuan, Trinh X.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 341 (2003) 1217
First results from XMM-Newton observations of the Canada France Redshift Survey (CFRS) 3hr, 10hr and 14hr fields are presented. Limited regions of two of the XMM surveys (3 and 14hr) are compared to the Canada UK Deep sub-mm Surveys (CUDSS) undertake
Externí odkaz:
http://arxiv.org/abs/astro-ph/0301610
Autor:
Dunne, Loretta, Eales, Stephen
Publikováno v:
Mon.Not.Roy.Astron.Soc. 327 (2001) 697
This is the second in a series of papers presenting results from the SCUBA Local Universe Galaxy Survey. In our first paper we provided 850 micron flux densities for 104 galaxies selected from the IRAS Bright Galaxy Sample and we found that the 60, 1
Externí odkaz:
http://arxiv.org/abs/astro-ph/0106362
Publikováno v:
Mon.Not.Roy.Astron.Soc.322:536-552,2001
We measure the radio luminosity function (RLF) of steep-spectrum radio sources using three redshift surveys of flux-limited samples selected at low (151 & 178 MHz) radio frequency, low-frequency source counts and the local RLF. The redshift surveys u
Externí odkaz:
http://arxiv.org/abs/astro-ph/0010419
Autor:
Eales, Stephen, Lilly, Simon, Webb, Tracy, Dunne, Loretta, Gear, Walter, Clements, David, Yun, Min
We have used SCUBA to survey an area of 50 square arcmin, detecting 19 sources down to a 3sigma sensitivity limit of 3.5 mJy at 850 microns. We have used Monte-Carlo simulations to assess the effect of source confusion and noise on the SCUBA fluxes a
Externí odkaz:
http://arxiv.org/abs/astro-ph/0009154