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| PKS 1355+01 , the SIMBAD biblio (22 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST17:35:03 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1966AuJPh..19...35D | 540 | 112 | The Parkes catalogue of radio sources. Declination zone 0 to +20. | DAY G.A., SHIMMINS A.J., EKERS R.D., et al. | |||||
| 1968AJ.....73..135G | 627 | 132 | Survey of radio sources observed in the continuum near 1420 MHz, declinations -5 to +70. | GALT J.A. and KENNEDY J.E.D. | |||||
| 1968ApJS...15..203F | 535 | 123 | The east-west structure of radio sources at 1425 MHz. | FOMALONT E.B. | |||||
| 1971AJ.....76....5F | 354 | 74 | Positions of 352 small-diameter radio sources. | FOMALONT E.B. and MOFFET A.T. | |||||
| 1971AuJPA..19....1W | 797 | 63 | The Parkes 2700 MHz survey catalogues for the ±4 declination zone and for selected regions. | WALL J.V., SHIMMINS A.J. and MERKELIJN J.K. | |||||
|
1972AJ.....77..405B |
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. | |||||
| 1973AJ.....78....1D | 627 | 61 | First results from the Texas interferometer: positions of 605 discrete sources. | DOUGLAS J.N., BASH F.N., GHIGO F.D., et al. | |||||
| 1974AJ.....79..437C | 384 | 61 | Intensity dependent radio spectral distributions in the Parkes 2700-MHz survey. | CONDON J.J. and JAUNCEY D.L. | |||||
| 1975MmRAS..80....1M | 340 | 68 | Accurate positions and identifications for a complete sample of 341 radio sources from the Parkes ± 4 degres survey. | McEWAN N.J., BROWNE I.W.A. and CROWTHER J.H. | |||||
| 1977AJ.....82...21B | 456 | 21 | Variability of extragalactic sources at 2.7 GHz II. Flux densities of 550 sources and further evidence for variations. | BRIDLE A.H., KESTEVEN M.J.L. and BRANDIE G.W. | |||||
| 1983ApJ...269..387P | 102 | 15 | A statistical VLBI study of milli-arcsecond cores in extragalactic radio sources. | PRESTON R.A., MORABITO D.D. and JAUNCEY D.L. | |||||
| 1985AJ.....90.1599P | 1228 | 160 | A VLBI survey at 2.29 GHz. | PRESTON R.A., MORABITO D.D., WILLIAMS J.G., et al. | |||||
| 1986ApJS...61..105L | 949 | 82 | 5 GHz radio structure and optical identifications of sources from the MG survey. II. Maps and finding charts. | LAWRENCE C.R., BENNETT C.L., HEWITT J.N., et al. | |||||
|
2008MNRAS.390..819G |
15 | D | 279 | 15 | The Combined NVSS-FIRST Galaxies (CoNFIG) sample - I. Sample definition, classification and evolution. | GENDRE M.A. and WALL J.V. | |||
|
2010A&A...511A..53V |
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. | ||
| 2012AJ....144..124Y | 92 | D | X | 3 | 86 | 5 | Invisible active galactic nuclei. I. Sample selection and Optical/Near-IR spectral energy distributions. | YAN T., STOCKE J.T., DARLING J., et al. | |
|
2014ApJS..212...15F |
15 | D | 1 | 24788 | 60 | A broadband polarization catalog of extragalactic radio sources. | FARNES J.S., GAENSLER B.M. and CARRETTI E. | ||
|
2014MNRAS.445..955B |
15 | D | 2 | 220 | 89 | The cosmic evolution of radio-AGN feedback to z = 1. | BEST P.N., KER L.M., SIMPSON C., et al. | ||
|
2016AJ....151...74Y |
921 | D | S X C | 22 | 92 | 12 | Invisible active galactic nuclei. II. Radio morphologies and five new H I 21cm absorption line detectors. | YAN T., STOCKE J.T., DARLING J., et al. | |
|
2016MNRAS.462.4197C |
16 | D | 1 | 103 | 8 | A comparative study of intervening and associated H I 21-cm absorption profiles in redshifted galaxies. | CURRAN S.J., DUCHESNE S.W., DIVOLI A., et al. | ||
| 2021MNRAS.506.1548C | 17 | D | 1 | 49 | ~ | Intervening or associated? Machine learning classification of redshifted H I 21-cm absorption. | CURRAN S.J. | ||
|
2021A&A...655A..17S |
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. |