Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey
A&A, 457 3 (2006) 841-856
Published online: 2006-09-12
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The first analytical expression to estimate photometric redshifts suggested by a machine
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MEASURING THE STELLAR MASSES OF z ∼ 7 GALAXIES WITH THE SPITZER ULTRAFAINT SURVEY PROGRAM (SURFS UP)
R. E. Ryan, A. H. Gonzalez, B. C. Lemaux, et al.The Astrophysical Journal 786 (1) L4 (2014)
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TRACING RECENT STAR FORMATION OF RED EARLY-TYPE GALAXIES OUT TOz∼ 1
Jongwan Ko, Ho Seong Hwang, Myungshin Im, et al.The Astrophysical Journal 791 (2) 134 (2014)
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SOMz: photometric redshift PDFs with self-organizing maps and random atlas
Matias Carrasco Kind and Robert J. BrunnerMonthly Notices of the Royal Astronomical Society 438 (4) 3409 (2014)
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Hidden starbursts and active galactic nuclei at 0 < z < 4 from theHerschel-VVDS-CFHTLS-D1 field: Inferences on coevolution and feedback
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Evidence for major mergers of galaxies at 2 ≲z< 4 in the VVDS and VUDS surveys
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OPTICAL-FAINT, FAR-INFRARED-BRIGHT HERSCHEL SOURCES IN THE CANDELS FIELDS: ULTRA-LUMINOUS INFRARED GALAXIES AT z > 1 AND THE EFFECT OF SOURCE BLENDING
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The morphological transformation of red sequence galaxies in the distant cluster XMMU J1229+0151
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Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5
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KILOPARSEC-SCALE PROPERTIES OF EMISSION-LINE GALAXIES
Shoubaneh Hemmati, Sarah H. Miller, Bahram Mobasher, et al.The Astrophysical Journal 797 (2) 108 (2014)
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Star formation in the cluster CLG0218.3-0510 at z = 1.62 and its large-scale environment: the infrared perspective
J. S. Santos, B. Altieri, M. Tanaka, et al.Monthly Notices of the Royal Astronomical Society 438 (3) 2565 (2014)
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CLASH: EXTENDING GALAXY STRONG LENSING TO SMALL PHYSICAL SCALES WITH DISTANT SOURCES HIGHLY MAGNIFIED BY GALAXY CLUSTER MEMBERS
C. Grillo, R. Gobat, V. Presotto, et al.The Astrophysical Journal 786 (1) 11 (2014)
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Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3-square-degree XMM coverage of CFHTLS
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