========================================================================== J/A+AS/136/571 Pulsars identified from the NRAO VLA Sky Survey (Han+ 1999) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table1.dat table2.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/cgi-bin/VizieR?-source=J/A+AS/136/571 ==========================================================================
drwxr-xr-x 26 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:56 [TAR file] -rw-r--r-- 1 cats archive 480 May 14 1999 .message -r--r--r-- 1 cats archive 6203 May 14 1999 ReadMe -rw-r--r-- 1 cats archive 420 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 3565 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 15707 Mar 9 1999 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 658 Mar 8 1999 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+AS/136/571 Pulsars identified from the NRAO VLA Sky Survey (Han+ 1999) ================================================================================ Pulsars identified from the NRAO VLA Sky Survey Han J.L., Tian W.W. <Astron. Astrophys. Suppl. Ser. 136, 571 (1999)> =1999A&AS..136..571H (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Pulsars ; Polarization ; Radio sources Keywords: pulsars: general - polarization - surveys Description: Table1 gives the NVSS radio sources around the positions of all known pulsars. This table was generated by searching NVSS catalog, and each row gives the closest source around one pulsar. However, not all of them are pulsars, as we discussed in our paper. If there is "?" in the Notes, we had more considerations to identify the source as a pulsar. If there is nothing or just "*" in Notes, the source is believed to be the pulsar. Table 2 lists 14 strong pulsars not detected by the NVSS, or more exactly saying, not listed in the NVSS catalog. By the courtesy of Jim Condon, we found some of these pulsars are confused by nearby strong radio sources, and most of them were really scintillating during the NVSS.
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