========================================================================== J/A+A/508/117 Spitzer selected starbursts at z 2 (Fiolet+, 2009) The following files can be converted to FITS (extension .fit or fit.gz) table1.dat table4.dat table5.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/508/117 ==========================================================================
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Beginning of ReadMe : J/A+A/508/117 Spitzer selected starbursts at z 2 (Fiolet+, 2009) ================================================================================ Multi-wavelength properties of Spitzer selected starbursts at z 2. Fiolet N., Omont A., Polletta M., Owen F., Berta S., Shupe D., Siana B., Lonsdale C., Strazzullo V., Pannella M., Baker A.J., Beelen A., Biggs A., De Breuck C., Farrah D., Ivison R., Lagache G., Lutz D., Tacconi L.J., Zylka R. <Astron. Astrophys., 508, 117-132 (2009)> =2009A&A...508..117F ================================================================================ ADC_Keywords: Galaxies, radio ; Galaxies, IR ; Redshifts ; Photometry, SDSS ; Photometry, infrared Keywords: galaxies: high-redshift - galaxies: starburst - galaxies: active - infrared: galaxies - submillimeter - radio continuum: galaxies Abstract: Wide-field Spitzer surveys allow identification of thousands of potentially high-z submillimeter galaxies (SMGs) through their bright 24um emission and their mid-IR colors. We want to determine the average properties of such z 2 Spitzer-selected SMGs by combining millimeter, radio, and infrared photometry for a representative IR-flux (lambda_rest_ 8um) limited sample of SMG candidates. A complete sample of 33 sources believed to be starbursts (5.8um-peakers) was selected in the (0.5deg^2^) J1046+56 field with selection criteria F_24um>400uJy, the presence of a redshifted stellar emission peak at 5.8um, and r'_Vega_>23. The field, part of the SWIRE Lockman Hole field, benefits from very deep VLA/GMRT 20cm, 50cm, and 90cm radio data (all 33 sources are detected at 50cm), and deep 160um and 70um Spitzer data. The 33 sources, with photometric redshifts 1.5-2.5, were observed at 1.2mm with IRAM-30m/MAMBO to an rms 0.7-0.8mJy in most cases. Their millimeter, radio, 7-band Spitzer, and near-IR properties were jointly analyzed. Description: Observations were made during the winter 2006/2007 MAMBO observing pool between December 2006 and March 2007 at the IRAM 30m telescope, located at Pico Veleta, Spain, using the 117-element version of the MAMBO array operating at 1.2mm (250GHz).