[CBK2002] 14 , the SIMBAD biblio

[CBK2002] 14 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST00:17:25

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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
1991ApJ...366..405P 2 9 93 A straight gravitational image in Abell 2390: a striking case of lensing by a cluster of galaxies. PELLO R., LE BORGNE J.-F., SOUCAIL G., et al.
1997A&A...317..661B 27 21 Redshift survey of gravitational arclets in Abell 2390. BEZECOURT J. and SOUCAIL G.
1998A&A...334L..21L 1 10 45 Deep ISOCAM view of the core of the lensing cluster A2390. LEMONON L., PIERRE M., CESARSKY C.J., et al.
1998ApJ...499L.115F 1 14 65 Discovery of red selected arcs at z = 4.04 behind Abell 2390. FRYE B. and BROADHURST T.
2000ApJ...531...95B 29 21 Resolving the stellar populations in a z=4 lensed galaxy. BUNKER A.J., MOUSTAKAS L.A. and DAVIS M.
2002AJ....123.2197C 1 37 177 Faint submillimeter counts from deep 850 micron observations of the lensing clusters A370, A851, and A2390. COWIE L.L., BARGER A.J. and KNEIB J.-P.
2003A&A...407..791M viz 154 97 An ISOCAM survey through gravitationally lensing galaxy clusters. I. Source lists and source counts for A370, A2218 and A2390. METCALFE L., KNEIB J.-P., McBREEN B., et al.
2005ApJ...627...32S viz 213 83 A systematic search for gravitationally lensed arcs in the Hubble Space Telescope WFPC2 archive. SAND D.J., TREU T., ELLIS R.S., et al.
2008ApJ...675..262R 61 90 Mid-infrared spectroscopy of lensed galaxies at 1 < z < 3: the nature of sources near the MIPS confusion limit. RIGBY J.R., MARCILLAC D., EGAMI E., et al.
2014ApJ...789...12C 1137       D S   X C       28 31 20 SMA observations on faint submillimeter galaxies with S850< 2 mJy: ultra dusty low-luminosity galaxies at high redshift. CHEN C.-C., COWIE L.L., BARGER A.J., et al.
2014AJ....148...65O 2492       D     X C F     63 11 2 A magnified view of star formation at z = 0.9 from two lensed galaxies. OLMSTEAD A., RIGBY J.R., SWINBANK M., et al.

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