2MASX J09582201-1103500 , the SIMBAD biblio

2MASX J09582201-1103500 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST09:03:10


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Title First 3 Authors
2003A&A...412...45P viz 15       D               1 956205 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
2008MNRAS.384.1502S viz 15       D               199 41 Near-infrared evolution of brightest cluster galaxies in the most X-ray luminous clusters since z = 1. STOTT J.P., EDGE A.C., SMITH G.P., et al.
2009A&A...499..357G viz 15       D               1 1272 20 The REFLEX galaxy cluster survey. VIII. Spectroscopic observations and optical atlas. GUZZO L., SCHUECKER P., BOEHRINGER H., et al.
2009MNRAS.399..683J viz 15       D               1 124640 796 The 6dF galaxy survey: final redshift release (DR3) and southern large-scale structures. JONES D.H., READ M.A., SAUNDERS W., 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.
2010ApJ...713.1037H 15       D               1 64 31 Brightest cluster galaxies and core gas density in REXCESS clusters. HAARSMA D.B., LEISMAN L., DONAHUE M., et al.
2010ApJ...715..881D 15       D               4 81 41 Star formation and UV colors of the brightest cluster galaxies in the representative XMM-Newton cluster structure survey. DONAHUE M., BRUCH S., WANG E., et al.
2012ApJS..199...23H viz 15       D               1 461 49 Infrared and ultraviolet star formation in brightest cluster galaxies in the ACCEPT sample. HOFFER A.S., DONAHUE M., HICKS A., et al.
2013ApJ...767..157G 16       D               1 73 11 Probing of the interactions between the hot plasmas and galaxies in clusters from z = 0.1 to 0.9. GU L., GANDHI P., INADA N., 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.

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