[NHD2010] SDP 17 lens , the SIMBAD biblio

[NHD2010] SDP 17 lens , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST17:13:31

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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
2010Sci...330..800N 11 15 348 The detection of a population of submillimeter-bright, strongly lensed galaxies. NEGRELLO M., HOPWOOD R., DE ZOTTI G., et al.
2012ApJ...752..152H 131       D     X         4 33 117 Blind detections of CO J = 1-0 in 11 H-ATLAS galaxies at z = 2.1-3.5 with the GBT/Zpectrometer. HARRIS A.I., BAKER A.J., FRAYER D.T., et al.
2012MNRAS.424.2429S 77           X         2 19 61 Strong biases in infrared-selected gravitational lenses. SERJEANT S.
2012PASJ...64L...2I 61     A     X         2 8 14 Initial results from Nobeyama molecular gas observations of distant bright galaxies. IONO D., HATSUKADE B., KOHNO K., et al.
2012ApJ...757..135L 688     A D     X C       18 19 76 Measurements of CO redshifts with z-spec for lensed submillimeter galaxies discovered in the H-ATLAS survey. LUPU R.E., SCOTT K.S., AGUIRRE J.E., et al.
2013A&A...551A.115O 208       D     X         6 32 74 H2O emission in high-z ultra-luminous infrared galaxies. OMONT A., YANG C., COX P., et al.
2013ApJ...774L..30T 38           X         1 19 2 Detection of an ultra-bright submillimeter galaxy behind the Small Magellanic Cloud. TAKEKOSHI T., TAMURA Y., MINAMIDANI T., et al.
2013ApJ...779...25B 16       D               1 66 171 Gravitational lens models based on Submillimeter Array imaging of Herschel-selected strongly lensed sub-millimeter galaxies at z > 1.5. BUSSMANN R.S., PEREZ-FOURNON I., AMBER S., et al.
2014MNRAS.440.1999N 753       D     X C       19 10 55 Herschel -ATLAS: deep HST/WFC3 imaging of strongly lensed submillimetre galaxies. NEGRELLO M., HOPWOOD R., DYE S., et al.
2014MNRAS.440.2013D 250       D     X C       6 10 44 Herschel-ATLAS: modelling the first strong gravitational lenses. DYE S., NEGRELLO M., HOPWOOD R., et al.

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