NAME SMM J04542-0301 , the SIMBAD biblio

NAME SMM J04542-0301 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST23:18:17

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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
2002MNRAS.330...92C 1 26 84 Submillimetre sources in rich cluster fields: source counts, redshift estimates and cooling flow limits. CHAPMAN S.C., SCOTT D., BORYS C., et al.
2003ApJ...592..674B 1 13 59 Peculiar velocity limits from measurements of the spectrum of the Sunyaev-Zeldovich effect in six clusters of galaxies. BENSON B.A., CHURCH S.E., ADE P.A.R., et al.
2003MNRAS.342..759A 105 78 Breaking the `redshift deadlock'- II. The redshift distribution for the submillimetre population of galaxies. ARETXAGA I., HUGHES D.H., CHAPIN E.L., et al.
2003PASJ...55..789T 17 21 Dusty ERO search behind two massive clusters. TAKATA T., KASHIKAWA N., NAKANISHI K., et al.
2007A&A...462..903B 35 6 Highly-magnified, multiply-imaged radio counterparts of the sub-mm starburst emission in the cluster-lens MS 0451.6-0305. BERCIANO ALBA A., GARRETT M.A., KOOPMANS L.V.E., et al.
2008A&A...477...55H viz 75           X         2 36 5 EROs found behind lensing clusters. II. Empirical properties, classification, and SED modelling based on multi-wavelength observations. HEMPEL A., SCHAERER D., EGAMI E., et al.
2009A&A...508..141F 76           X         2 8 4 On the abundance of gravitational arcs produced by submillimeter galaxies at radio and submm wavelengths. FEDELI C. and BERCIANO ALBA A.
2010A&A...509A..54B 595   K A     X C       15 49 13 Radio counterpart of the lensed submm emission in the cluster MS0451.6-0305: new evidence for the merger scenario. BERCIANO ALBA A., KOOPMANS L.V.E., GARRETT M.A., et al.
2012A&A...539A.155M 133       D     X         4 82 237 A Herschel view of the far-infrared properties of submillimetre galaxies. MAGNELLI B., LUTZ D., SANTINI P., et al.
2015A&A...582A..90Y 16       D               1 59 6 The spectral energy distribution of galaxies at z > 2.5: Implications from the Herschel/SPIRE color-color diagram. YUAN F.-T., BUAT V., BURGARELLA D., et al.

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