Spectroscopy of IR-Selected Galaxy Clusters at 1 < z < 1.5

Details Spectroscopy of IR-Selected Galaxy Clusters at 1 < z < 1.5 Spectroscopy of IR-Selected Galaxy Clusters at 1 < z < 1.5

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11597s&link_type=abstract

HST Proposal ID #11597. Cycle 17

Physics

Scientific paper

We propose to obtain WFC3 G141 and G102 slitless spectroscopy of galaxy clusters at 1 < z < 1.5 that were selected from the IRAC survey of the Bootes NDWFS field. Our IRAC survey contains the largest sample of spectroscopically confirmed clusters at z > 1. The WFC3 grism data will measure H-alpha to determine SFR, and fit models to the low resolution continua to determine stellar population histories for the brighter cluster members, and redshifts for the red galaxies too faint for ground-based optical spectroscopy.;

Affiliated with

Also associated with

No associations

Rating

Spectroscopy of IR-Selected Galaxy Clusters at 1 < z < 1.5 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spectroscopy of IR-Selected Galaxy Clusters at 1 < z < 1.5, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopy of IR-Selected Galaxy Clusters at 1 < z < 1.5 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1320247