m and 3.6µm photometric observation of
N=8 Lyman-break galaxies in the redshift range z∼6.6-7 behind strong lensing clusters.
Use of archival HST ACS images, as part of the CLASH survey.
Ref:&=
2014ApJ...784...58S
by&SMIT R.
, BOUWENS R.J., LABBE I., ZHENG W., BRADLEY L., DONAHUE M., LEMZE D., MOUSTAKAS J., UMETSU K., ZITRIN A., COE D., POSTMAN M., GONZALEZ V., BARTELMANN M., BENITEZ N., BROADHURST T., FORD H., GRILLO C., INFANTE L., JIMENEZ-TEJA Y., JOUVEL S., KELSON D.D., LAHAV O., MAOZ D., MEDEZINSKI E., MELCHIOR P., MENEGHETTI M., MERTEN J., MOLINO A., MOUSTAKAS L.A., NONINO M., ROSATI P., SEITZ S.
&Astrophys. J., 784, 58 (2014)
&
Evidence for ubiquitous high-equivalent-width nebular emission in z ~ 7 galaxies: toward a clean measurement of the specific star-formation rate using a sample of bright, magnified galaxies.
o&
Tables 1-2: <[SBL2014] macsHHMMZ-MSSssMSSss> N=3, <[SBL2014] aNNNNZ-MSSssMMSSs> N=3, <[SBL2014] rxjHHMMZ-MSSssMMSSs> N=2.
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