CYBERSKA
A Cyberinfrastructure platform to meet the needs of data intensive radio astronomy on route to the SKA |
Automated Source Finding - SAD
...ked at the C-field 13 Jul 2010 Release with Duchamp and encountering a few issues I thought it would be prudent to run a similar analysis with the AIPS implemenation of SAD. In the...4295 days ago
3951 days ago
EN1 GMRT Stokes I mosaic - version 2
...probability function is now best fit with an rms of 10.3 microJy instead of 10.7 for version 1. The source list for this file created using AIPS SAD contains 2800 sources....2174 days ago
Preliminary 5 GHz source counts
...elimary sources counts at 5 GHz from ten-pointing mosaic C-array image. The rms noise is 1.9 μJy. These counts are made from an aips sad source list with a 5&sigm...3475 days ago
Automated Source Finding - SAD
Having looked at the C-field 13 Jul 2010 Release with Duchamp and encountering a few issues I thought it would be prudent to run a similar analysis with the AIPS implemenation of SAD. In the Stokes I image, some 489 sources were found down to a detection threshold of 1K (as with Duchamp a numbe...Tags: galfacts, cfield, igalfa, sources, source finding, nvss, gb6, sad, aips
4295 days ago
Comment on "Fractional polarization versus offset"
>I guess the other difference between your result and mine is that you processed in aips and I processed in casa. Wouldn't expect that to make a difference in the best of all possible worlds.... I've taken a look at Jamie's M51 data with casa in the past and I saw the same issues.3735 days ago
Comment on "Fractional polarization versus offset"
...ination pattern and dish shape, as you point out in your memo). I guess the other difference between your result and mine is that you processed in aips and I processed in casa. &nbs...3737 days ago