87GB 065856.0+500639 , the SIMBAD biblio

87GB 065856.0+500639 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST07:20:02


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Title First 3 Authors
2007AJ....133.2097C viz 15       D               1 58 68 FIRST ``Winged'' and X-shaped radio source candidates. CHEUNG C.C.
2009ApJS..181..548C viz 15       D               1 53 11 FIRST "Winged" and X-shaped radio source candidates. II. New redshifts. CHEUNG C.C., HEALEY S.E., LANDT H., et al.
2010A&A...511A..53V viz 15       D               1 107940 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.
2010A&A...518A..10V viz 15       D               1 168913 597 A catalogue of quasars and active nuclei: 13th edition. VERON-CETTY M.-P. and VERON P.
2010MNRAS.408.1103L 244       D     X   F     6 63 16 The optical spectra of x-shaped radio galaxies. LANDT H., CHEUNG C.C. and HEALEY S.E.
2014ApJS..212...15F viz 16       D               1 24940 60 A broadband polarization catalog of extragalactic radio sources. FARNES J.S., GAENSLER B.M. and CARRETTI E.
2015ApJ...810L...6R 79             C       1 17 4 The abundance of X-shaped radio sources: implications for the gravitational wave background. ROBERTS D.H., SARIPALLI L. and SUBRAHMANYAN R.
2018ApJ...852...47R viz 16       D               2 100 12 What are "X-shaped" radio sources telling us? I. Very Large Array imaging of a Large sample of candidate XRGs. ROBERTS D.H., SARIPALLI L., WANG K.X., et al.
2018ApJ...852...48S viz 16       D               1 95 10 What are "X-shaped" radio sources telling us? II. Properties of a sample of 87. SARIPALLI L. and ROBERTS D.H.
2019AJ....157..195L 226       D     X         6 31 5 GMRT low-frequency imaging of an extended sample of X-shaped radio galaxies. LAL D.V., SEBASTIAN B., CHEUNG C.C., et al.
2021A&A...655A..17S viz 17       D               1 338596 3 The SPECFIND V3.0 catalog of radio continuum cross-identifications and spectra: Reaching lower frequencies. STEIN Y., VOLLMER B., BOCH T., et al.

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