EGSIRAC J141726.30+523031.1 , the SIMBAD biblio

EGSIRAC J141726.30+523031.1 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST01:43:52


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Title First 3 Authors
1995ApJ...455...75L viz 14       D               1 438 82 The Canada-France Redshift Survey. III. "Single emission-line" objects, analysis of repeat observations, and spectroscopic identifications in the 1415+52 and 2215+00 fields. LILLY S.J., HAMMER F., LE FEVRE O., et al.
1996ApJ...464...79S viz 143 87 Canada-france redshift survey. XI. Morphology of high-redshift field galaxies from high-resolution ground-based imaging. SCHADE D., LILLY S.J., LE FEVRE O., et al.
1996MNRAS.278...95S 33 16 Canada-France Redshift Survey. X. The quasar sample. SCHADE D., CRAMPTON D., HAMMER F., et al.
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.
2011ApJS..193...30B viz 15       D               1 7611 103 UV-to-FIR analysis of Spitzer/IRAC sources in the Extended Groth Strip. II. Photometric redshifts, stellar masses, and star formation rates. BARRO G., PEREZ-GONZALEZ P.G., GALLEGO J., et al.
2012ApJ...751...50G viz 15       D               1 8632 29 The DEEP2 Galaxy Redshift Survey: the Voronoi-Delaunay method catalog of galaxy groups. GERKE B.F., NEWMAN J.A., DAVIS M., et al.
2013ApJS..204...21M viz 16       D               1 34882 13 Extended photometry for the DEEP2 galaxy redshift survey: a testbed for photometric redshift experiments. MATTHEWS D.J., NEWMAN J.A., COIL A.L., et al.
2019A&A...631A...9B viz 17       D               1 8367 ~ The OTELO survey. I. Description, data reduction, and multi-wavelength catalogue. BONGIOVANNI A., RAMON-PEREZ M., PEREZ GARCIA A.M., et al.
2021A&A...647A..89N viz 17       D               1 3659 ~ The OTELO survey as a morphological probe. Last ten Gyr of galaxy evolution. The mass-size relation up to z = 2. NADOLNY J., BONGIOVANNI A., CEPA J., et al.

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