8C 1821+643B , the SIMBAD biblio

8C 1821+643B , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST23:46:45

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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
1992AJ....103.1047S 12 38 The cluster of galaxies associated with the low-redshift quasar H1821+643. SCHNEIDER D.P., BAHCALL J.N., GUNN J.E., et al.
1992MNRAS.256..404L 59 25 A complete sample of radio sources in the North Ecliptic Cap, selected at 38 MHz - I. The radio data. LACY M., RAWLINGS S. and WARNER P.J.
1992MNRAS.258..828L 2 3 29 The radio properties and environment of the remarkable radio-quiet quasar E 1821+643. LACY M., RAWLINGS S. and HILL G.J.
1993MNRAS.263..707L 147 31 A complete sample of sources in the North Ecliptic Cap ,selected at 38 MHz. II. CCD observations and their implications. LACY M., HILL G.J., KAISER M.-E., et al.
1994PASP..106..646K viz 3193 29 The HST quasar absorption-line key project. VIII. CCD imaging of Hubble Space Telescope quasar fields. KIRHAKOS S., SARGENT W.L.W., SCHNEIDER D.P., et al.
1998ApJ...508..200T viz 14       D               279 154 The relationship between galaxies and low-redshift weak Lyα absorbers in the directions of H1821+643 and PG 1116+215. TRIPP T.M., LU L. and SAVAGE B.D.
1999MNRAS.308.1087L 34 7 A complete sample of radio sources in the North Ecliptic Cap, selected at 38 MHz - III. Further imaging observations and the photometric properties of the sample. LACY M., KAISER M.E., HILL G.J., et al.
1999MNRAS.308.1096L 158 44 Optical spectroscopy of two overlapping, flux-density-limited samples of radio sources in the North Ecliptic Cap, selected at 38 and 151 MHz. LACY M., RAWLINGS S., HILL G.J., et al.
2016MNRAS.459.2940K 252       D     X   F     6 8 6 How unusual is the cool-core radio halo cluster CL1821+643? KALE R. and PAREKH V.
2018MNRAS.480.1187B viz 16       D               1 198 1 Multi-object spectroscopy of CL1821+643: a dynamically relaxed cluster with a giant radio halo? BOSCHIN W. and GIRARDI M.

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