VLA Survey Results

• B0031-07: HTML with images. (Also, plain text.) - Joe
• J0108-1431: HTML with images. (Also, plain text.) - Joe
• B0136+57: HTML with images. (Also, plain text.) - Joe
• B0138+59: HTML with images. (Also, plain text.) - Joe
• B0149-16: HTML with images. (Also, plain text.) -Walter
• B0450+55: HTML with images. (Also, plain text.)
• B0450-18: HTML with images. (Also, plain text.)
• B0525+21: HTML with images. (Also, plain text.)
• B0540+23: HTML with images. (Also, plain text.)
• B0609+37: HTML with images. (Also, plain text.)
• J0613-0200: HTML with images. (Also, plain text.)
• J0751+1807: HTML with images. (Also, plain text.) - Miller
• B0818-13: HTML with images. (Also, plain text.) - Miller
• B0834+06: HTML with images. (Also, plain text.) - Miller
• J1012+5307: HTML with images. (Also, plain text.) - Miller
• J1022+10: HTML with images. (Also, plain text.) - Miller
• B1039-19: HTML with images. (Also, plain text.) - Miller
• B1112+50: HTML with images. (Also, plain text.) - Miller
• J1643-1224: HTML with images. (Also, plain text.) - Miller
• B1508+55: HTML with images. (Also, plain text.) - Miller
• B1541+09: HTML with images. (Also, plain text.) - Miller
• B1604-00: HTML with images. (Also, plain text.) - Miller
• B1702-19: HTML with images. (Also, plain text.) - Miller
• B1706-16: HTML with images. (Also, plain text.) - Miller
• J1713+0747: HTML with images. (Also, plain text.) - Miller
• J1744-1134: HTML with images. (Also, plain text.) - Miller
• B1800-21: HTML with images. (Also, plain text.) - Joe
• B1804-08: HTML with images. (Also, plain text.) - Joe
• B1818-04: HTML with images. (Also, plain text.) - Joe
• B1821-19: HTML with images. (Also, plain text.)
• B1822-09: HTML with images. (Also, plain text.) - walter
• B1826-17: HTML with images. (Also, plain text.)
• B1829-08: HTML with images. (Also, plain text.) - Walter
• B1831-04: HTML with images. (Also, plain text.) - Joe
• B1834-10: HTML with images. (Also, plain text.)
• J1835-1106: HTML with images. (Also, plain text.)
• B1839+56: HTML with images. (Also, plain text.) - Joe
• B1839-04: HTML with images. (Also, plain text.) - Walter
• B1839+09: HTML with images. (Also, plain text.) - Joe
• B1844-04: HTML with images. (Also, plain text.) - Walter
• B1845-01: HTML with images. (Also, plain text.) - Joe
• B1855+09: HTML with images. (Also, plain text.) - Joe
• B1905+39: HTML with images. (Also, plain text.) - Mark
• B1911-04: HTML with images. (Also, plain text.) - Joe
• B1919+21: HTML with images. (Also, plain text.) - Mark
• B1933+16: HTML with images. (Also, plain text.) - Mark
• B1937+21: HTML with images. (Also, plain text.) - Mark
• B1944+17: HTML with images. (Also, plain text.) - Mark
• B1946+35: HTML with images. (Also, plain text.) - Mark
• B1953+50: HTML with images. (Also, plain text.) - Walter
• B2000+40: HTML with images. (Also, plain text.) - Walter
• B2011+38: HTML with images. (Also, plain text.) - Walter
• B2045-16: HTML with images. (Also, plain text.)
• B2053+36: HTML with images. (Also, plain text.)
• B2106+44: HTML with images. (Also, plain text.)
• B2111+46: HTML with images. (Also, plain text.)
• B2154+40: HTML with images. (Also, plain text.)
• B2255+58: HTML with images. (Also, plain text.) - Ed
• B2310+42: HTML with images. (Also, plain text.)
• B2319+60: HTML with images. (Also, plain text.) - Ed
• B2324+60: HTML with images. (Also, plain text.) - Ed
• B2351+61: HTML with images. (Also, plain text.) - Joe
• B2334+61: HTML with images. (Also, plain text.) - Joe

1. After VLA imaging, the output is a text file with information and an EPS image from KNTR + LWPLA. The pulsar should always be field 001 in the text listing. The text file format is:
   

   # Field name    RA              Dec             Flux    RMS     Comment
   B0450+55.001    04 54 07.75794  55 43 41.4416   11.57   0.15    Pulsar
   B0450+55.002    04 54 00.08356  55 36 45.3387   225.5   0.18    Core - jet
   

2. The RMS noise is from IMEAN's histogram estimate.
   Flux, RA and DEC estimates are from MAXFIT with PIXXY = the peak found by IMEAN.
   This is crude, but quick, and is sufficient for follow-up observations.

3. Inputs to KNTR:   docont 1; dogrey 0; ltype -3; cbplot 1;
     plev 10; levs -4,-2,-1,1,2,4,8,9.5;

4. Inputs to LWPLA:   dparm 0 0 0 0 1 5005 31 6 0 0;
     outfile 'FITS:'!!inname!!'.'!!inclass!!'.eps'

5. The web page is generated from the text results and EPS images in the aips FITS directory, using mkweb.pl, a Perl script. This also generates the required GIF images and calculates the angular separation (D) in arcmin.

6. The comment field has information about the compactness and suitability as an in-beam candidate.

• Aips scripts from Walter: usage notes to be added.
• mkweb.pl: to generate the pulsar web pages and gif images.
• anglsep.c: code to calculate angular separations between sources.
  Uses SLALIB and does it without kludges!
• HTML header and footer pages: these are not valid HTML pages on their own.

Shami Chatterjee shami@astro.cornell.edu Last modified: 2 Apr 2002