4C 13.65 , the SIMBAD biblio

4C 13.65 , the SIMBAD biblio (25 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST20:47:21

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1967BAN....19..201D 188 61 A 1417 MHz search for radio sources having a flux excess at short wavelengths. DAVIS M.M.
1968MNRAS.139..289W 372 34 The radio spectra of sources in the fourth Cambridge catalogue -III. WILLIAMS P.J.S., COLLINS R.A., CASWELL J.L., et al.
1969AJ.....74..833H 199 10 Declination measurements of selected 4C sources using the Arecibo 1000-ft reflector. HAZARD C., JAUNCEY D.L., GULKIS S., et al.
1971A&A....11..171W 322 35 A statistically complete sample of radio-sources at 1400 MHz. WITZEL A., VERON P. and VERON M.P.
1972AJ.....77..405B viz 574 259 Flux densities, positions, and structures for a complete sample of intense radio sources at 1400 MHz. BRIDLE A.H., DAVIS M.M. and FOMALONT E.B.
1972AJ.....77..797P viz 242 111 The NRAO 5-GHz radio source survey. III. The 140-ft "strong" source survey. PAULINY-TOTH I.I.K. and KELLERMANN K.I.
1974AJ.....79.1006J 134 43 Optical identifications from the NRAO 5-GHz radio survey. JOHNSON K.H.
1974AJ.....79.1220C 462 84 Spectra of sources in the NRAO 5000-MHz surveys. CONDON J.J. and JAUNCEY D.L.
1983AJ.....88..239B 42 9 Coherence time for 430-MHz VLBI. BRIGGS F.H.
1984AJ.....89.1784A 21 38 Multifrequency light-curves of low-frequency variable radio sources. ALTSCHULER D.R., BRODERICK J.J., CONDON J.J., et al.
1988ApJ...328..275C 40 20 HI emission-absorption studies with high-velocity resolution. COLGAN S.W.J., SALPETER E.E. and TERZIAN Y.
1994ApJS...93..441M viz 38 25 Results of a five-year program of multifrequency monitoring of low-frequency variable radio sourcces. MITCHELL K.J., DENNISON B., CONDON J.J., et al.
1995ApJ...441..200G 1 2 14 Star counts from the HST snapshot survey. II. Wide binaries. GOULD A., BAHCALL J.N., MAOZ D., et al.
1995AuJPh..48..143S viz 2209 69 Radio sources observed with the Culgoora circular array. SLEE O.B.
1999ApJS..120...77S 41 10 14-year program monitoring the flux densities of 33 radio sources at low frequencies. SALGADO J.F., ALTSCHULER D.R., GHOSH T., et al.
2003ApJ...586.1067H 1 84 486 The millennium Arecibo 21 centimeter absorption-line survey. II. Properties of the warm and cold neutral media. HEILES C. and TROLAND T.H.
2003ApJS..145..329H viz 74 137 The millennium Arecibo 21 centimeter absorption-line survey. I. Techniques and gaussian fits. HEILES C. and TROLAND T.H.
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...725..466C 17       D               2 94 414 Magnetic fields in interstellar clouds from Zeeman observations: inference of total field strengths by Bayesian analysis. CRUTCHER R.M., WANDELT B., HEILES C., 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.
2014ApJS..215...14D viz 15       D               1 7877 110 The WISE blazar-like radio-loud sources: an all-sky catalog of candidate γ-ray blazars. D'ABRUSCO R., MASSARO F., PAGGI A., et al.
2018ApJ...860...33F 16       D               1 87 14 Synthetic observations of 21 cm H I line profiles from inhomogeneous turbulent interstellar H I gas with magnetic fields. FUKUI Y., HAYAKAWA T., INOUE T., et al.
2018ApJ...862...49N 16       D               1 58 51 Dust-gas scaling relations and OH abundance in the galactic ISM. NGUYEN H., DAWSON J.R., MIVILLE-DESCHENES M.-A., 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.
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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