implications for the formation of massive galaxies. | |
o | Tables 2, 3: <[VFF2004] M-NNNN> N=5, <[VFF2004] C-NNNN> N=2. |
Auth.: | VAN DOKKUM P.G.+ |
Ref: | =2004ApJ...616...40F |
by | FOERSTER-SCHREIBER N.M. , VAN DOKKUM P.G., FRANX M., LABBE I., RUDNICK G., DADDI E., ILLINGWORTH G.D., KRIEK M., MOORWOOD A.F.M., RIX H.-W., ROETTGERING H., TRUJILLO I., VAN DER WERF P., VAN STARKENBURG L., WUYTS S. |
Astrophys. J., 616, 40-62 (2004) | |
A substantial population of red galaxies at z > 2: modeling of the spectral energy distributions of an extended sample. | |
o | Fig.4: objects HDFS-NNN are [LFR2003] NNN in SIMBAD. |
o | Fig.4: <[VFF2004] M-NNNN> N=5 added. |
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