===========================================================================
COSMOS VLA 90cm Data                                            Version 1.0
===========================================================================

The Cosmic Evolution Survey (COSMOS) is an HST Treasury Project to
survey a 2 square degree equatorial field, centered on RA=10:00:28.6
and DEC=+02:12:21.0, using the ACS camera. The project also
incorporates major commitments from other observatories around the
world, including the National Radio Astronomy Observatory's (NRAO)
Very Large Array (VLA) radio telescope.

These VLA data represent 7.3 hrs of 327 MHz (P band, 90cm) observations of the 
field in A-configuration taken in November 2008. The survey has reached a 
sensitivity of 0.56 rms mJy/beam over the central 2 square degrees.

The key characteristics of these data:

        Configuration:                VLA A-array
        Dates of observations:        November, 2008
        Observing time:                7.3h
        Frequency:                326 MHz ( P band, 90cm)
        Bandwidth:                75 MHz (Multi-channel continuum mode)
        Pointings:                1 
        Area:                        3.1 square degrees
        Resolution:                6.3"
        Sensitivity:                0.56 mJy/beam

Any paper using these data should includ: Vernesa Smolcic
<vs@astro.uni-bonn.de>
Send any questions to: Vernesa Smolcic (vs@astro.uni-bonn.de).


The data products available here include:

        (1) a source catalog to 5.5 sigma.
        (2) a flux calibrated, astrometrically correct image,
            in SIN projection 

Further information may be obtained from the VLA-COSMOS web page:

        http://www.mpia-hd.mpg.de/COSMOS

or the main COSMOS web page:

        http://cosmos.astro.caltech.edu/

The data reduction, image reconstruction, catalog construction and bandwidth 
correction is similar to the procedures for the large project described in:

"The VLA-COSMOS Survey: II. Source Catalog of the Large Project"
by Schinnerer et al. 2007, ApJS, COSMOS special issue, 172, 46

"The VLA-COSMOS Survey: III. Further Catalog Analysis and the Radio 
Source Counts"
by Bondi et al., 2008, ApJ, 681, 1129
COSMOS VLA 90cm Data                                            Version 1.0
===========================================================================

The Cosmic Evolution Survey (COSMOS) is an HST Treasury Project to
survey a 2 square degree equatorial field, centered on RA=10:00:28.6
and DEC=+02:12:21.0, using the ACS camera. The project also
incorporates major commitments from other observatories around the
world, including the National Radio Astronomy Observatory's (NRAO)
Very Large Array (VLA) radio telescope.

These VLA data represent xx hrs of 327 MHz (90cm) observations of the 
field in XXX-configuration taken in November 2008. The survey has reached a 
sensitivity of an rms of uJy/beam over the central xxx.

The key characteristics of these data:

	Configuration:		VLA XXX-array
	Dates of observations:	November, 2008
	Observing time:		
	Frequency:		326 MHz ( = P band, 90cm)
	Bandwidth:		75 MHz (Multi-channel continuum mode)
	Pointings:		1 
	Area:			
	Resolution:		"
	Sensitivity:		uJy/beam

Any paper using these data should includ: Vernesa Smolcic <vs@astro.uni-bonn.de>
Send any questions to: Vernesa Smolcic (vs@astro.uni-bonn.de).


The data products available here include:

	(1) a source catalog to 5.5 sigma.
	(2) a flux calibrated, astrometrically correct image,
	    in SIN projection 

Further information may be obtained from the VLA-COSMOS web page:

	http://www.mpia-hd.mpg.de/COSMOS

or the main COSMOS web page:

	http://cosmos.astro.caltech.edu/

The data reduction, image reconstruction, catalog construction and bandwidth 
correction is similar to the procedures for the large project described in:

"The VLA-COSMOS Survey: II. Source Catalog of the Large Project"
by Schinnerer et al. 2007, ApJS, COSMOS special issue, 172, 46

"The VLA-COSMOS Survey: III. Further Catalog Analysis and the Radio 
Source Counts"
by Bondi et al., 2008, ApJ, 681, 1129