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87GB 115916.7+393541 , the SIMBAD biblio (22 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST10:06:49 |
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 |
---|---|---|---|---|---|---|---|---|---|
1986A&A...168...25G | 95 | 30 | 408 MHz variability of complete samples of radio sources. | GREGORINI L., FICARRA A. and PADRIELLI L. | |||||
1989AJ.....98..419V | 1091 | 103 | Structures, spectral indexes, and optical identifications of radio sources selected from the B3 catalogue. | VIGOTTI M., GRUEFF G., PERLEY R., et al. | |||||
1990A&AS...82...41K | 751 | 14 | Spectral index distribution for a sample of sources from the B3 catalogue. | KULKARNI V.K., MANTOVANI F. and PAULINY-TOTH I.I.K. | |||||
1995PASP..107..369M | 16 | 9 | Optical identification of radio galaxies from the B3VLA survey. | MAXFIELD L., THOMPSON D., DJORGOVSKI S., et al. | |||||
1999A&A...345..769M | 1 | 47 | 231 | Synchrotron spectra and ages of compact steep spectrum radio sources. | MURGIA M., FANTI C., FANTI R., et al. | ||||
1999A&AS..139..359V | 1047 | 11 | Multi-frequency study of the B3-VLA sample. II. The database. | VIGOTTI M., GREGORINI L., KLEIN U., et al. | |||||
2001A&A...369..380F | O | 98 | 77 | Multi-frequency VLA observations of a new sample of CSS/GPS radio sources. | FANTI C., POZZI F., DALLACASA D., et al. | ||||
2002A&A...389..115D | 28 | 29 | The B3-VLA CSS sample. II. VLBA images at 18 cm. | DALLACASA D., TINTI S., FANTI C., et al. | |||||
2004A&A...426..463O | O | 22 | 20 | The B3-VLA CSS sample. V. VLBA images at 6 and 3.6 cm. | ORIENTI M., DALLACASA D., FANTI C., et al. | ||||
2004A&A...427..465F | O | 88 | 33 | The B3-VLA CSS sample. IV. Kp-scale polarization properties. | FANTI C., BRANCHESI M., COTTON W.D., et al. | ||||
2006A&A...450..945K | O | 13 | 22 | FIRST-based survey of compact steep spectrum sources. IV. Multifrequency VLBA observations of very compact objects. | KUNERT-BAJRASZEWSKA M., MARECKI A. and THOMASSON P. | ||||
2008ApJ...687..141K | 164 | 17 | The fate of young radio galaxies: decelerations inside host galaxies? | KAWAKATU N., NAGAI H. and KINO M. | |||||
2008A&ARv..15...67M | 15 | D | 2 | 222 | 321 | Distant radio galaxies and their environments. | MILEY G. and DE BREUCK C. | ||
2009ApJ...698..840C | 15 | D | 1 | 74 | 132 | Accretion disk model of short-timescale intermittent activity in young radio sources. | CZERNY B., SIEMIGINOWSKA A., JANIUK A., et al. | ||
2010A&A...511A..53V | 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. | ||
2010MNRAS.408.2261K | 15 | D | 1 | 168 | 106 | A survey of low-luminosity compact sources and its implication for the evolution of radio-loud active galactic nuclei - I. Radio data. | KUNERT-BAJRASZEWSKA M., GAWRONSKI M.P., LABIANO A., et al. | ||
2011A&A...528A.110F | 361 | D | X C | 9 | 124 | 7 | The B3-VLA CSS sample. VIII. New optical identifications from the Sloan Digital Sky Survey The ultraviolet-optical spectral energy distribution of the young radio sources. | FANTI C., FANTI R., ZANICHELLI A., et al. | |
2011AJ....142...89P | 15 | D | 1 | 857 | 22 | Precise absolute astrometry from the VLBA imaging and polarimetry survey at 5 GHz. | PETROV L. and TAYLOR G.B. | ||
2014ApJ...786...17W | 16 | D | 1 | 426 | 38 | The galaxy cluster mid-infrared luminosity function at 1.3 < z < 3.2. | WYLEZALEK D., VERNET J., DE BREUCK C., et al. | ||
2014ApJS..213....3M | 16 | D | 1 | 28367 | 27 | The Low-frequency Radio Catalog of flat-spectrum sources. | MASSARO F., GIROLETTI M., D'ABRUSCO R., et al. | ||
2016MNRAS.459..820T | 16 | D | 1 | 112 | 37 | Compact symmetric objects and supermassive binary black holes in the VLBA Imaging and Polarimetry Survey. | TREMBLAY S.E., TAYLOR G.B., ORTIZ A.A., et al. | ||
2021A&A...655A..17S | 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. |