3XLSS J232206.7-544532 , the SIMBAD biblio

3XLSS J232206.7-544532 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST05:38:30

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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
1964AuJPh..17..340B 303 139 The Parkes catalogue of radio sources declination zone -20 to -60 degres. BOLTON J.G., GARDNER F.F. and MacKEY M.B.
1966AuJPh..19..649S 642 54 Accurate positions of 644 radio sources. SHIMMINS A.J., CLARKE M.E. and EKERS R.D.
1972MNRAS.157..367H 312 61 Accurate positions of radio sources at 408 MHz. HUNSTEAD R.W.
1985RMxAA..10..101C 87 2 A search for variable radiosources at 1410 MHz. COLOMB F.R., GIACANI E.B., LOISEAU N., et al.
1988Ap&SS.141..303B 677 71 Catalogue of unambiguous (Faraday-thin, one-component, spectrum-selected) rotation measures for galaxies and quasars. BROTEN N.W., MacLEOD J.M. and VALLEE J.P.
1990MNRAS.247..387R 536 29 Molonglo radio sources in the directions of southern Abell clusters. ROBERTSON J.G. and ROACH G.J.
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.
1994ApJS...91..111W viz 5741 324 The Parkes-MIT-NRAO (PMN) Surveys: II. Source catalog for the Southern Survey (-87deg.5 < delta < -37deg). WRIGHT A.E., GRIFFITH M.R., BURKE B.F., et al.
1994PASAu..11...33C 58 22 Variable radio sources at 843 MHz. CAMPBELL-WILSON D. and HUNSTEAD R.W.
2000PASA...17...72G 55 23 Long-term monitoring of Molonglo calibrators. GAENSLER B.M. and HUNSTEAD R.W.
2006MNRAS.370.2064B 33 10 1.4-GHz polarimetric observations of the two fields imaged by the DASI experiment. BERNARDI G., CARRETTI E., SAULT R.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.
2011ApJ...734L..34J viz 15       D               1 442 32 New 145 MHz source measurements by PAPER in the southern sky. JACOBS D.C., AGUIRRE J.E., PARSONS A.R., et al.
2011MNRAS.417.2651M viz 15       D               1 5894 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.
2012ApJ...744...84Y viz 15       D               1 1143 18 On the evolution of the cores of radio sources and their extended radio emission. YUAN Z. and WANG J.
2012MNRAS.422.1527M viz 15       D               1 11134 22 ATPMN: accurate positions and flux densities at 5 and 8 GHz for 8385 sources from the PMN survey. McCONNELL D., SADLER E.M., MURPHY T., et al.
2015MNRAS.448.2085L 40           X         1 49 13 Analysis of Sunyaev-Zel'dovich effect mass-observable relations using South Pole Telescope observations of an X-ray selected sample of low-mass galaxy clusters and groups. LIU J., MOHR J., SARO A., et al.
2016A&A...592A...1P viz 16       D               2 5977 212 The XXL Survey. I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme. PIERRE M., PACAUD F., ADAMI C., et al.
2016A&A...592A...5F viz 16       D               1 1006 26 The XXL Survey. VI. The 1000 brightest X-ray point sources. FOTOPOULOU S., PACAUD F., PALTANI S., 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.
2020A&A...633A...6E 145       D     X         4 15 ~ The XXL Survey. XXXIX. Polarised radio sources in the XXL-South field. EYLES R.A.J., BIRKINSHAW M., SMOLCIC V., 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.
2023ApJS..265...32M viz 93           X         2 163 ~ Powerful Radio Sources in the Southern Sky. I. Optical Identifications. MASSARO F., WHITE S.V., GARCIA-PEREZ A., et al.

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