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G89.0+4.7
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G89.0+4.7.htmlReferences:. Hirabayashi & Takahashi 1972, PASJ, 24, 231. 30-m dish at 4.2 GHz (11': S=16040 Jy). -
G292.0+1.8
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G292.0+1.8.htmlMSH 1154. Right Ascension: 11 24 36. Declination: 59 16. Size (/arcmin): 128. -
G357.7-0.1
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G357.7-0.1.htmlLaRosa et al. 2000, AJ, 119, 207. VLA at 333 MHz (24''43''). -
G69.0+2.7
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G69.0+2.7.htmlAngerhofer et al. 1981, A&A, 94, 313. WSRT at 610 MHz (56''103'') 1.4 GHz (24''44'') and 5 GHz (7''13''), plus optical. -
https://www.mrao.cam.ac.uk/projects/surveys/6C/data/6C5a.list
https://www.mrao.cam.ac.uk/projects/surveys/6C/data/6C5a.list13 May 1993: 45 - 13 : 030058 3 0 36.3 67 14 18 3.36 4.26 27 : 030058 3 0 49.1 49 24 24 0.60 - 6 : 030058 3 0 52.0 ... 030058 3 24 22.2 54 58 47 6.24 6.52 -22 : 030058 3 24 24.4 61 6 8 0.32 - 1 : 050058 3 24 24.7 64 53 -
G43.3-0.2
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G43.3-0.2.htmlBrogan & Troland 2001, ApJ, 550, 799. VLA at 1.4 GHz (24''27'' and 5'') for HI Zeeman splitting. -
G260.4-3.4
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G260.4-3.4.htmlDistance: Association with HI implies 1.3 kpc. References:. Green 1971, AuJPh, 24, 773. -
G184.6-5.8
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G184.6-5.8.htmlG184.65.8 ADS: search fulltext or title/keyword/abstract. Crab Nebula, 3C144, SN1054. Right Ascension: 05 34 31. Declination: 22 01. Size (/arcmin): 75. Type: F. Flux density at 1 GHz (/Jy): 900. Spectral Index: 0.30. Notes: This is the remnant of -
G327.6+14.6
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G327.6+14.6.htmlReynolds & Gilmore 1993, AJ, 106, 272. VLA at 1.37 and 1.67 GHz (24''), including polarisation. -
G189.1+3.0
https://www.mrao.cam.ac.uk/surveys/snrs/snrs.G189.1+3.0.htmlMitra et al. 2014, IAUS, 296, 376. Combined GMRT and CLFST observations at 150 MHz (19''24'').
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