4C 05.78 , the SIMBAD biblio

4C 05.78 , the SIMBAD biblio (14 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST10:00:54


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Title First 3 Authors
1975AJ.....80..335S 1092 38 Positions and flux densities of 1075 radio sources at 365 MHz. SHARP J.R. and BASH F.N.
1977ApJS...35..359G 212 31 Optical identification of 664 Ohio sources using accurate radio and optical positions measured by the Texas interferometers. GHIGO F.D.
2002MNRAS.337..981S 49 24 A Parkes half-Jansky sample of GHz peaked spectrum galaxies. SNELLEN I.A.G., LEHNERT M.D., BREMER M.N., et al.
2006A&A...445..889T 123 24 Constraints on evolutionary properties of GHz Peaked Spectrum galaxies. TINTI S. and DE ZOTTI G.
2006MNRAS.373..972G 103 113 Probing radio source environments via Hi and OH absorption. GUPTA N., SALTER C.J., SAIKIA D.J., et al.
2007A&A...463...97L viz         O           185 32 GPS radio sources: new optical observations and an updated master list. LABIANO A., BARTHEL P.D., O'DEA C.P., et al.
2007A&A...464..879D 15       D               1 37 18 Complete identification of the Parkes half-Jansky sample of GHz peaked spectrum radio galaxies. DE VRIES N., SNELLEN I.A.G., SCHILIZZI R.T., et al.
2007A&A...469..451T viz 15       D               97 24 Radio continuum spectra of gigahertz-peaked spectrum galaxies. TORNIAINEN I., TORNIKOSKI M., LAEHTEENMAEKI A., et al.
2007A&A...470...97L 20 9 VLBI observations of nineteen GHz-peaked-spectrum radio sources at 1.6 GHz. LIU X., CUI L., LUO W.-F., et al.
2008A&A...482..483T viz         O           207 8 Cluster analyses of gigahertz-peaked spectrum sources with self-organising maps. TORNIAINEN I., TORNIKOSKI M., TURUNEN M., et al.
2009AN....330..145L 46 2 Structure, spectra and variability of some GPS radio sources. LIU X., SONG H.-G. and CUI L.
2010A&A...518A..23C 452     A D S   X C       11 15 2 The follow-up european VLBI network observations of twelve GPS radio sources at 5 GHz. CUI L., LIU X., LIU J., et al.
2020MNRAS.498..883G viz 16       D               1 261 ~ The evolution of neutral hydrogen over the past 11 Gyr via H I 21 cm absorption. GRASHA K., DARLING J., LEROY A.K., et al.
2020A&A...643A.174M viz 16       D               1 83 ~ uGMRT HI 21-cm absorption observations of two extremely inverted spectrum sources. MHASKEY M., PAUL S., GUPTA N., et al.

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