7C 182631.60+651044.00 , the SIMBAD biblio

7C 182631.60+651044.00 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST15:10:42


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Title First 3 Authors
1992MNRAS.256..404L 59 25 A complete sample of radio sources in the North Ecliptic Cap, selected at 38 MHz - I. The radio data. LACY M., RAWLINGS S. and WARNER P.J.
1993MNRAS.263..707L 147 31 A complete sample of sources in the North Ecliptic Cap ,selected at 38 MHz. II. CCD observations and their implications. LACY M., HILL G.J., KAISER M.-E., et al.
1994ApJS...93..145K viz 2561 29 A sensitive 1.5 GHz radio survey around the north ecliptic pole. KOLLGAARD R.I., BRINKMANN W., McMATH CHESTER M., et al.
1995A&AS..110..419V viz 2780 24 The 7C survey of radio sources at 151 MHz - a 418-square-degree region centred at RA 17h, Dec. 65deg. VISSER A.E., RILEY J.M., ROETTGERING H.J.A., et al.
1995MNRAS.276..614L viz 406 16 A radio-optical survey of the North Ecliptic Cap. LACY M., RILEY J.M., WALDRAM E.M., et al.
1999MNRAS.307..420L 35 10 Radio-optical alignments in a low radio luminosity sample. LACY M., RIDGWAY S.E., WOLD M., et al.
1999MNRAS.308.1087L 34 7 A complete sample of radio sources in the North Ecliptic Cap, selected at 38 MHz - III. Further imaging observations and the photometric properties of the sample. LACY M., KAISER M.E., HILL G.J., et al.
1999MNRAS.308.1096L 158 44 Optical spectroscopy of two overlapping, flux-density-limited samples of radio sources in the North Ecliptic Cap, selected at 38 and 151 MHz. LACY M., RAWLINGS S., HILL G.J., 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.
2014MNRAS.445..955B viz 16       D               1 220 89 The cosmic evolution of radio-AGN feedback to z = 1. BEST P.N., KER L.M., SIMPSON 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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