CFRS 03.0570 , the SIMBAD biblio

CFRS 03.0570 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST01:17:40

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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
1995ApJ...455...88H viz 272 51 The Canada-France Redshift Survey. IV. Spectroscopic selection effects and 0300+00 field spectroscopic data. HAMMER F., CRAMPTON D., LE FEVRE O., et al.
1997ApJ...481...49H viz 411 191 Canada-France Redshift Survey. XIV. Spectral properties of field galaxies up to z=1. HAMMER F., FLORES H., LILLY S.J., et al.
2001ApJ...550..570H 2 15 111 Luminous compact galaxies at intermediate redshifts: progenitors of bulges of massive spirals? HAMMER F., GRUEL N., THUAN T.X., et al.
2002MNRAS.337..369T 1 34 109 The H α luminosity function and star formation rate up to z ∼ 1. TRESSE L., MADDOX S.J., LE FEVRE O., et al.
2003ApJ...597..730L 67 117 The metallicities of star-forming galaxies at intermediate redshifts 0.47. LILLY S.J., CAROLLO C.M. and STOCKTON A.N.
2004A&A...415..885F 20 57 Star formation rates of distant luminous infrared galaxies derived from Hα and IR luminosities. FLORES H., HAMMER F., ELBAZ D., et al.
2004A&A...421..847Z 57 63 HST/WFPC2 morphologies and color maps of distant luminous infrared galaxies. ZHENG X.Z., HAMMER F., FLORES H., et al.
2004AJ....127.2002K viz 136 353 [O II] as a star formation rate indicator. KEWLEY L.J., GELLER M.J. and JANSEN R.A.
2005A&A...430..115H viz 174 227 Did most present-day spirals form during the last 8 Gyr? A formation history with violent episodes revealed by panchromatic observations. HAMMER F., FLORES H., ELBAZ D., et al.
2005ApJ...635..260S 1 93 442 The Gemini Deep Deep Survey. VII. The redshift evolution of the mass-metallicity relation. SAVAGLIO S., GLAZEBROOK K., LE BORGNE D., et al.
2006A&A...447..113L 50 43 Significant evolution of the stellar mass-metallicity relation since z ∼ 0.65. LIANG Y.C., HAMMER F. and FLORES H.
2012MNRAS.421.2888R viz 15       D               2 68 25 A decrease of the gas exchanges between galaxies and the intergalactic medium, from 12 to 6 billion years ago. RODRIGUES M., PUECH M., HAMMER F., et al.

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