NVSS J022233+584813 , the SIMBAD biblio

NVSS J022233+584813 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST12:20:48


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Title First 3 Authors
1980A&AS...42..227K 254 86 A 21 cm radio continuum survey of the galactic plane between l=93 and l=162. KALLAS E. and REICH W.
1986AJ.....92..787F viz 323 35 A complete VLA survey in the outer galaxy. FICH M.
1987AJ.....94..111L 72 22 Observations at 408 MHz of the supernova remnant HB 3 (G132.6+1.5). LANDECKER T.L., VANELDIK J.F., DEWDNEY P.E., et al.
1990AISAO..32..132T 84 1 Investigation of the second galactic quadrant radiosources from Kallas and Reich survey at 7.6 and 31.3 cm wavelengths. TRUSHKIN S.A.
2006MNRAS.373.1203K viz 15       D               258 2 A sharper view of the outer Galaxy at 1420 and 408 MHz from the Canadian Galactic Plane Survey - I. Revisiting the KR catalogue and new Gigahertz Peaked Spectrum sources. KERTON C.R.
2010A&A...511A..53V viz 15       D               1 107473 39 The SPECFIND V2.0 catalogue of radio cross-identifications and spectra. SPECFIND meets the Virtual Observatory. VOLLMER B., GASSMANN B., DERRIERE S., et al.
2010ApJ...721..267A 2201       D S   X C       57 15 33 Distance and proper motion measurement of the red supergiant, s Persei, with VLBI H2 O maser astrometry. ASAKI Y., DEGUCHI S., IMAI H., et al.
2014ApJS..212...15F viz 15       D               1 24788 60 A broadband polarization catalog of extragalactic radio sources. FARNES J.S., GAENSLER B.M. and CARRETTI E.
2021A&A...655A..17S viz 17       D               1 338578 3 The SPECFIND V3.0 catalog of radio continuum cross-identifications and spectra: Reaching lower frequencies. STEIN Y., VOLLMER B., BOCH T., et al.
2022ApJS..260....4P viz 17       D               1 7976 3 Direction of Parsec-scale Jets for 9220 Active Galactic Nuclei. PLAVIN A.V., KOVALEV Y.Y. and PUSHKAREV A.B.
2023A&A...676A..11L 17       D           *   1 161 ~ Enhancing the alignment of the optically bright Gaia reference frame with respect to the International Celestial Reference System. LUNZ S., ANDERSON J.M., XU M.H., et al.

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