WSRT Virgo HI filament survey (Popping+, 2011)

Details WSRT Virgo HI filament survey (Popping+, 2011) WSRT Virgo HI filament survey (Popping+, 2011)

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35279090p&link_type=abstract

VizieR On-line Data Catalog: J/A+A/527/A90. Originally published in: 2011A&A...527A..90P

Physics

Surveys, Clusters: Galaxy, Galaxies: Radio, H I Data

Scientific paper

To obtain the highest possible brightness sensitivity in cross-correlations, the WSRT (Westerbork Synthesis Radio Telescope) was configured to simulate a large filled aperture in projection. Twelve of the 14 WSRT 25m telescopes were positioned at regular intervals of 144m.
A deep fully-sampled survey of the galaxy filament joining the Local Group to the Virgo Cluster has been undertaken, extending from 8 to 17h in RA and from -1 to +10 degrees in declination and covering 40MHz of bandwidth with 8km/s resolution.
(3 data files).

Affiliated with

Also associated with

No associations

Rating

WSRT Virgo HI filament survey (Popping+, 2011) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with WSRT Virgo HI filament survey (Popping+, 2011), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and WSRT Virgo HI filament survey (Popping+, 2011) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1003925