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NVSS J062019+210229 , the SIMBAD biblio (22 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST21:01:55 |
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 |
---|---|---|---|---|---|---|---|---|---|
1997A&AS..126..413R | 1829 | 86 | The Effelsberg 21 cm radio continuum survey of the Galactic plane between l = 95.5deg and l = 240 deg. | REICH P., REICH W. and FUERST E. | |||||
1998MNRAS.300..790W | 541 | 128 | Interferometer phase calibrations sources - III. The regions +20deg ≤ delB1950 ≤ +35deg and +75deg ≤ delB1950 ≤ +90deg . | WILKINSON P.N., BROWNE I.W.A., PATNAIK A.R., et al. | |||||
2000ApJ...534...90P | 52 | 79 | The COINS sample: VLBA identifications of compact symmetric objects. | PECK A.B. and TAYLOR G.B. | |||||
2000ApJ...534..104P | 51 | 27 | Redshifts and neutral hydrogen observations of compact symmetric objects in the COINS sample. | PECK A.B., TAYLOR G.B., FASSNACHT C.D., et al. | |||||
2002ApJS..141...13B | 1501 | 304 | The VLBA calibrator Survey–VCS1. | BEASLEY A.J., GORDON D., PECK A.B., et al. | |||||
2002NewAR..46..295P | 9 | 1 | New VLBA identifications of compact symmetric objects. | PECK A.B. and TAYLOR G.B. | |||||
2003ApJ...583..272H | 27 | 26 | The sizes of OH (1720 MHz) supernova remnant masers: MERLIN and very long baseline array observations of IC 443. | HOFFMAN I.M., GOSS W.M., BROGAN C.L., et al. | |||||
2005ApJ...622..136G | 29 | 67 | Dating COINS: kinematic ages for compact symmetric objects. | GUGLIUCCI N.E., TAYLOR G.B., PECK A.B., et al. | |||||
2005MNRAS.356..637H | 32 | 15 | A MERLIN survey of 4.7-GHz excited OH masers in star-forming regions. | HARVEY-SMITH L. and COHEN R.J. | |||||
2007ApJ...661...78G | 21 | 14 | Polarimetry of compact symmetric objects. | GUGLIUCCI N.E., TAYLOR G.B., PECK A.B., et al. | |||||
2009ARep...53..319T | 15 | D | X | 1 | 49 | 0 | Study of compact radio sources using interplanetary scintillations at 111 MHz. Compact symmetric objects. | TYUL'BASHEV S.A. | |
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. | ||
2011A&A...535A..24S | 15 | D | 1 | 65 | 14 | VLBI-selected sample of compact symmetric object candidates and frequency-dependent position of hotspots. | SOKOLOVSKY K.V., KOVALEV Y.Y., PUSHKAREV A.B., et al. | ||
2014ApJS..212...15F | 16 | D | 1 | 24940 | 60 | A broadband polarization catalog of extragalactic radio sources. | FARNES J.S., GAENSLER B.M. and CARRETTI E. | ||
2015AJ....150...58F | 16 | D | 1 | 3421 | 241 | The second realization of the international celestial reference frame by very long baseline interferometry. | FEY A.L., GORDON D., JACOBS C.S., et al. | ||
2019ApJS..242....5X | 17 | D | 1 | 3393 | ~ | Structure effects for 3417 Celestial Reference Frame radio sources. | XU M.H., ANDERSON J.M., HEINKELMANN R., et al. | ||
2019ApJ...880..141N | 17 | D | 1 | 90 | 21 | Exploring the properties of warm and cold atomic hydrogen in the Taurus and Gemini regions. | NGUYEN H., DAWSON J.R., LEE M.-Y., et al. | ||
2019A&A...630A.101K | 17 | D | 2 | 3584 | ~ | Realization of a multifrequency celestial reference frame through a combination of normal equation systems. | KARBON M. and NOTHNAGEL A. | ||
2020MNRAS.499.1441D | 17 | D | X * | 3 | 7 | ~ | OH maser towards IRAS 06056+2131: polarization parameters and evolution status. | DARWISH M.S., RICHARDS A.M.S., ETOKA S., et al. | |
2020A&A...644A.159C | 17 | D | 1 | 4536 | 184 | The third realization of the International Celestial Reference Frame by very long baseline interferometry. | CHARLOT P., JACOBS C.S., GORDON D., 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. |