PKS 0655-319 , the SIMBAD biblio

PKS 0655-319 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST18:03:51


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Title First 3 Authors
1991MNRAS.251..330W viz 1195 35 Flux densities at 8400 MHz for a large sample of radiosources. WRIGHT A.E., WARK R.M., TROUP E., et al.
1995AuJPh..48..143S viz 2209 69 Radio sources observed with the Culgoora circular array. SLEE O.B.
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.
2011MNRAS.416..559B viz 15       D               1 172 19 The Planck-ATCA coeval observations project: the faint sample. BONAVERA L., MASSARDI M., BONALDI A., et al.
2011MNRAS.417.2651M viz 15       D               1 5893 47 Optical properties of high-frequency radio sources from the Australia Telescope 20 GHz (AT20G) Survey. MAHONY E.K., SADLER E.M., CROOM S.M., 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.
2016MNRAS.455.3249M viz 16       D               1 465 11 The Planck-ATCA Co-eval Observations project: analysis of radio source properties between 5 and 217 GHz. MASSARDI M., BONALDI A., BONAVERA L., et al.
2018MNRAS.476.2717H viz 16       D               1 1285 1 A novel approach for characterizing broad-band radio spectral energy distributions. HARVEY V.M., FRANZEN T., MORGAN J., et al.
2019ApJS..242....4D viz 16       D               1 9583 45 Two new catalogs of blazar candidates in the WISE Infrared sky. D'ABRUSCO R., ALVAREZ CRESPO N., MASSARO F., et al.
2020ApJ...897....5N viz 16       D               1 89 ~ Measuring HERA's primary beam in situ: methodology and first results. NUNHOKEE C.D., PARSONS A.R., KERN N.S., et al.
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.

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