# VLA survey summary: see http://www.astro.cornell.edu/~shami/psrvlb/ # Best inbeam candidates # Pulsar position is from 1.4 GHz; Inbeam pos from 8.4 GHz A array # Note that inbeam L-band fluxes are underestimates (primary beam) # # Name Sub RA (J2000) Dec (J2000) D(') s1400 s8400 B0031-07 PSR 00 34 08.87043 -07 21 53.5632 0 12.6 0 # J0108-1431 PSR 01 08 08.04510 -14 31 53.9057 0 1.4 0 J0108-1431 006 01 07 48.27484 -14 13 45.3600 18.8 4.2 18.2 J0108-1431 002 01 09 38.70873 -14 42 35.2366 24.4 21.2 24.6 # B0136+57 PSR 01 39 19.74455 58 14 31.7186 0 4.6 0 # 009 is 1 mJy and close B0136+57 011 01 39 11.18090 58 35 42.9875 21.2 20.3 45.8 B0136+57 012 01 37 50.47629 58 14 11.2905 11.8 91.4 85.7 B0136+57 005 01 40 32.32726 58 11 35.3004 10.0 12.9 3.9 # B0138+59 PSR 01 41 39.93702 60 09 32.1320 0 5.3 0 B0138+59 016 01 40 56.30429 60 10 57.2533 5.6 10.4 4.9 B0138+59 010 01 40 12.44514 60 07 45.9803 11.0 5.3 1.8 # B0149-16 PSR 01 52 10.85610 -16 37 53.188 0 1.5 0 B0149-16 006 01 53 25.14799 -16 31 13.6879 19.0 2.9 26.9 B0149-16 018 01 51 43.63350 -16 26 37.7007 13.0 7.3 7.9 # B0450+55 PSR 04 54 07.75794 55 43 41.4416 0 11.6 0 # bright and close! B0450+55 002 04 54 00.06323 55 36 45.4060 7.0 225.5 120.7 # B0450-18 PSR 04 52 34.10961 -17 59 23.3871 0 154.2 0 B0450-18 002 04 52 11.97908 -18 16 41.9582 18.1 23.1 12.0 # B0525+21 PSR 05 28 52.26843 22 00 04.8078 0 18.2 0 # weak (2.4 mJy) but the only one! B0525+21 004 05 28 48.65463 21 42 30.1766 17.6 3.3 2.4 # B0540+23 PSR 05 43 09.67074 23 29 06.2776 0 8.7 0 # no X-band sources? # B0609+37 PSR 06 12 48.69831 37 21 37.3581 0 3.0 0 # great looking source! B0609+37 008 06 12 12.91365 37 25 38.3110 8.2 10.7 14.7 # J0613-0200 PSR 06 13 43.97930 -02 00 47.0600 0 1.8 0 J0613-0200 002 06 15 02.38012 -01 58 24.4205 19.7 13.3 12.3 J0613-0200 008 06 13 27.79276 -02 14 25.5430 14.2 4.6 2.1 # J0751+1807 PSR 07 51 09.15629 18 07 38.4174 0 9.0 0 # 024 is 22.5' away but 142 mJy J0751+1807 024 07 50 00.33469 18 23 11.2627 22.5 21.6 141.7 J0751+1807 020 07 50 20.38045 18 09 50.5743 11.8 4.9 3.7 J0751+1807 005 07 51 52.28710 17 54 31.5133 16.7 10.6 3.6 # B0818-13 PSR 08 20 26.38662 -13 50 55.7525 0 4.7 0 # 43 mJy, 4', 70.5mas B0818-13 002 08 20 11.43071 -13 49 12.8558 4.0 30.1 43.8 # B0834+06 PSR 08 37 05.63990 06 10 14.9220 0 3.7 0 # both sources weak, 10.6',13.9' away B0834+06 008 08 36 35.73231 06 02 43.3238 10.6 16.0 2.5 B0834+06 009 08 36 31.74770 05 59 10.8400 13.9 8.3 2.0 # J1012+5307 PSR 10 12 33.43151 53 07 02.4825 0 3.0 0 # all sources weak J1012+5307 017 10 13 07.29382 53 12 34.3308 7.5 20.2 3.5 J1012+5307 014 10 12 30.55368 52 58 25.5316 8.6 6.5 2.6 J1012+5307 018 10 13 07.35425 53 04 22.8756 5.7 4.1 2.3 # J1022+10 PSR 10 22 58.00254 10 01 52.8084 0 5.1 0 # 010 is by far the best J1022+10 010 10 23 10.90487 10 01 26.9064 3.2 28.1 17.8 J1022+10 006 10 24 18.69204 09 55 46.9418 20.8 4.9 5.0 J1022+10 005 10 23 26.59566 09 57 21.9062 8.4 4.4 3.1 # B1039-19 PSR 10 41 36.17974 -19 42 13.3545 0 1.4 0 # this is a weak 1.7 mJy candidate B1039-19 002 10 41 17.81292 -19 52 40.3647 11.3 6.7 1.7 # B1112+50 PSR 11 15 38.48073 50 30 25.6351 0 31.5 0 # 021 is 1.7 mJy @ X-band B1112+50 003 11 16 51.18705 50 36 01.9199 12.8 5.4 5.7 B1112+50 021 11 14 50.06499 50 29 17.3066 7.8 5.7 1.7 # B1508+55 PSR 15 09 25.63048 55 31 32.3289 0 1.4 0 # very compact, 25.8 mJy, 22.6' away B1508+55 006 15 11 48.06076 55 41 56.2876 22.6 7.1 25.8 # B1541+09 PSR 15 43 38.82788 09 29 16.3742 0 4.1 0 # great! 31.1 mJy, 13.3' away compact B1541+09 008 15 43 03.70214 09 19 09.7845 13.3 150.5 31.1 # B1604-00 PSR 16 07 12.07792 -00 32 41.1643 0 2.0 0 # 1.4 mJy, 9.1' B1604-00 011 16 06 35.55558 -00 32 38.1375 9.1 4.9 1.4 # J1643-1224 PSR 16 43 38.16396 -12 24 58.7005 0 3.8 0 # 6.6' away 14.7 mJy J1643-1224 007 16 43 19.43821 -12 20 15.6969 6.6 10.1 14.7 # B1702-19 PSR 17 05 36.05144 -19 06 39.2201 0 20.8 0 # 007 is 4.3mJy, 2.0' away, compact B1702-19 007 17 05 45.70871 -19 04 40.4153 3.0 2.0 4.3 B1702-19 013 17 04 41.58672 -18 58 07.3331 15.4 2.0 31.3 B1702-19 012 17 04 29.16675 -19 03 35.9759 16.1 17.7 16.4 B1702-19 002 17 06 07.40406 -19 00 57.0999 9.3 5.8 3.3 # B1706-16 PSR 17 09 26.44344 -16 40 58.1108 0 1.5 0 # 2.2mJy, 4.8' away, weak pulsar B1706-16 013 17 09 40.55787 -16 37 35.3791 4.8 3.6 2.2 # J1713+0747 PSR 17 13 49.54882 07 47 37.3229 0 0.5 0 J1713+0747 008 17 13 27.09521 07 30 18.9931 18.2 7.0 17.1 # J1744-1134 PSR 17 44 29.41892 -11 34 54.8889 0 7.3 0 J1744-1134 015 17 43 25.18090 -11 17 56.0366 23.2 7.3 10.9 # B1800-21 PSR 18 03 51.42154 -21 37 07.3780 0 14.6 0 # 5.0mJy, 3.3mJy, bright pulsar B1800-21 006 18 03 38.65393 -21 22 37.3251 14.8 26.4 5.0 B1800-21 003 18 04 20.40030 -21 31 58.6359 8.5 9.3 3.3 # B1804-08 PSR 18 07 38.01128 -08 47 43.1881 0 10.6 0 B1804-08 005 18 07 26.04776 -09 05 47.1812 18.3 3.7 11.3 B1804-08 003 18 08 17.68320 -08 52 38.9134 11.0 8.9 6.7 # B1818-04 PSR 18 20 52.57449 -04 27 37.1120 0 6.4 0 B1818-04 006 18 20 43.39607 -04 24 12.4164 4.1 69.6 82.6 B1818-04 005 18 21 03.91950 -04 26 33.7892 3.0 52.4 3.4 # B1821-19 PSR 18 24 00.47617 -19 45 52.1887 0 7.0 0 # 007 is 2.2 mJy, compact B1821-19 011 18 24 22.00871 -19 52 34.8565 8.4 6.7 9.9 B1821-19 016 18 22 58.41138 -19 30 02.1595 21.6 10.8 10.8 B1821-19 007 18 24 29.58179 -19 36 44.6407 11.4 8.4 2.2 # B1822-09 PSR 18 25 30.62923 -09 35 23.0109 0 5.6 0 # 20.7' away, otherwise great B1822-09 008 18 24 32.56566 -09 50 17.6804 20.7 5.8 39.5 # B1826-17 PSR 18 29 43.16222 -17 51 04.5352 0 9.5 0 # B1829-08 PSR 18 32 37.00140 -08 27 03.3100 0 4.2 0 B1829-08 005 18 32 27.48135 -08 37 18.2364 10.5 6.7 4.3 B1829-08 004 18 32 32.29644 -08 38 53.5006 11.9 58.0 11.3 # B1831-04 PSR 18 34 25.59887 -04 26 16.1950 0 11.1 0 # B1834-10 PSR 18 36 53.90734 -10 08 09.1132 0 3.1 0 # What, no X-band? # J1835-1106 PSR 18 35 18.35003 -11 06 16.8556 0 2.7 0 J1835-1106 004 18 35 19.57533 -11 15 59.2894 9.7 66.4 62.3 J1835-1106 012 18 35 25.24992 -11 08 37.0745 2.9 9.3 3.4 # B1839+09 PSR 18 41 55.95619 09 12 07.2456 0 4.7 0 B1839+09 009 18 41 50.02858 08 57 19.6383 14.9 8.4 18.1 B1839+09 007 18 42 23.59912 09 27 17.8759 16.6 3.0 5.5 # B1839+56 PSR 18 40 44.59000 56 40 55.3500 0 3.0 0 # Great source B1839+56 013 18 41 09.02612 56 38 15.2841 4.3 3.4 8.9 # B1839-04 PSR 18 42 26.45062 -03 59 59.1501 0 7.1 0 # Great source B1839-04 007 18 41 27.31380 -03 48 44.3345 18.6 15.2 118.5 # B1844-04 PSR 18 47 22.82291 -04 02 14.1341 0 3.1 0 # 008 is 1.8 mJy but only 3.5' away B1844-04 017 18 46 26.90112 -04 08 52.2038 15.4 12.5 3.7 B1844-04 008 18 47 25.32509 -04 05 39.6409 3.5 7.1 1.8 # B1845-01 PSR 18 48 23.60004 -01 23 58.3755 0 11.4 0 B1845-01 003 18 48 51.74008 -01 40 18.0075 17.8 7.7 14.2 B1845-01 004B 18 48 40.14273 -01 45 23.2494 21.8 7.7 6.8 # B1855+09 PSR 18 57 36.68518 09 43 22.8402 0 0.9 0 # 20.1' away, 13.7mJy B1855+09 006 18 57 24.77888 09 23 32.3191 20.1 3.6 13.7 # B1905+39 PSR 19 07 34.65479 40 02 05.8611 0 1.8 0 B1905+39 019 19 06 11.42710 39 56 10.0581 17.0 60.7 103.3 B1905+39 017 19 06 55.76275 39 53 27.1839 11.4 18.3 5.0 # B1911-04 PSR 19 13 54.18819 -04 40 48.1731 0 4.8 0 B1911-04 009 19 13 21.79431 -04 32 54.0058 11.3 5.8 6.9 B1911-04 005 19 14 11.14288 -04 58 44.4379 18.4 4.5 10.0 B1911-04 002 19 15 22.12592 -04 34 36.8014 22.8 8.2 13.1 # B1919+21 PSR 19 21 44.85040 21 53 02.1962 0 1.0 0 # Its 1.3 mJy for a 1.0 mJy PSR # B1933+16 PSR 19 35 47.83002 16 16 40.0501 0 58.9 0 # both are weak, but psr is strong B1933+16 010 19 35 55.52636 16 17 00.6849 1.9 11.6 2.8 B1933+16 007 19 36 00.87528 15 56 46.3356 20.1 4.1 2.5 # B1937+21 PSR 19 39 38.58406 21 34 58.7684 0 2.5 0 # both are very extended # B1944+17 PSR 19 46 53.06633 18 05 41.3134 0 9.9 0 # 016 is 23.1' away B1944+17 016 19 46 20.93679 18 27 32.7358 23.1 41.1 27.1 B1944+17 013 19 45 45.54691 18 15 14.5061 18.7 8.8 3.9 # B1946+35 PSR 19 48 24.99891 35 40 11.0109 0 7.4 0 # 300 mJy, 16.7' away B1946+35 010 19 48 04.51924 35 56 20.6653 16.7 159.7 303.2 # B1953+50 PSR 19 55 18.73691 50 59 55.6642 0 7.9 0 # 22.4' away B1953+50 021 19 53 58.92013 51 18 33.1225 22.4 8.2 11.3 # B2000+40 PSR 20 02 44.03296 40 50 53.6628 0 5.8 0 B2000+40 004 20 03 06.77628 40 29 01.1660 22.3 10.0 27.3 # B2011+38 PSR 20 13 10.35260 38 45 42.9143 0 6.8 0 B2011+38 002 20 13 59.27394 38 28 51.9562 19.4 20.0 81.0 B2011+38 008 20 13 39.98681 38 37 34.5442 10.0 3.6 4.5 # B2045-16 PSR 20 48 35.60161 -16 16 44.5919 0 4.8 0 B2045-16 011 20 48 36.69994 -16 09 45.4394 7.0 19.0 10.0 B2045-16 008 20 48 49.57191 -16 00 13.9195 16.8 21.7 83.4 B2045-16 009 20 48 08.93113 -16 01 45.2250 16.3 3.4 3.4 # B2053+36 PSR 20 55 31.35433 36 30 21.7039 0 2.3 0 B2053+36 011 20 55 12.22739 36 34 22.6929 5.6 15.6 17.9 B2053+36 013 20 55 32.58045 36 37 53.6296 7.5 19.2 6.7 B2053+36 019 20 54 14.10850 36 40 30.8534 18.5 4.3 4.5 # B2106+44 PSR 21 08 20.48337 44 41 48.9434 0 4.6 0 B2106+44 016 21 08 06.77400 44 56 16.9776 14.7 5.4 13.6 # B2111+46 PSR 21 13 24.31688 46 44 08.7343 0 22.8 0 # 011 is only 2.1mJy but 1.8' away B2111+46 011 21 13 14.25888 46 43 41.4909 1.8 3.3 2.1 B2111+46 005 21 14 32.87532 46 34 39.2864 15.1 21.9 170.3 B2111+46 019 21 11 52.13387 46 44 53.5221 15.8 3.3 3.8 # B2154+40 PSR 21 57 01.84110 40 17 46.0682 0 12.4 0 B2154+40 003 21 57 54.02421 40 04 54.6025 16.3 45.6 23.8 B2154+40 011 21 57 17.80378 40 12 25.4848 6.2 6.6 2.4 # B2255+58 PSR 22 57 57.75737 59 09 14.7361 0 5.9 0 B2255+58 003 22 59 56.64761 59 11 47.1650 15.4 9.5 30.8 B2255+58 014 22 57 46.82558 59 24 32.4757 15.4 6.3 24.9 B2255+58 004 22 58 01.90675 58 59 15.6779 10.0 86.4 11.8 # B2310+42 PSR 23 13 08.61386 42 53 12.9910 0 15.8 0 B2310+42 014 23 12 13.49560 42 39 32.3585 17.0 8.7 18.1 # B2319+60 PSR 23 21 55.21478 60 24 30.5935 0 15.2 0 # 2.5mJy (psr is 15.2) B2319+60 009 23 19 58.01254 60 26 29.5762 14.6 3.6 2.5 # B2324+60 PSR 23 26 58.68797 61 13 36.2702 0 3.3 0 # Its a longshot at 1.5 mJy B2324+60 003 23 26 32.88767 60 59 31.7402 14.4 6.1 1.5 # B2334+61 PSR 23 37 05.79901 61 51 01.4063 0 3.7 0 # 2.6 mJy, resolved # B2351+61 PSR 23 54 04.75021 61 55 46.6533 0 0.9 0 B2351+61 008 23 54 40.72504 61 37 36.1130 18.7 16.9 36.8 #