WORKING GROUP SPECTROSCOPIC SURVEY
- complete down to Bj=17.5 the Horologium redshift survey
- define and carry out a spectroscopic survey of Horologium to
obtain redshifts for fainter galaxies (magnitude-limited, TBD) for LSS,
LS dynamics and LFs
- outline the spectroscopic follow-up at VLT and preparing the
- Aims of the VLT spectroscopy are
- to obtain spectroscopic characterisation (stellar
populations, SFR, etc...) of galaxies belonging to the full range of
environments, both in local (z=0.05) and in distant (z=0.3-0.5)
- to derive internal kinematics (scaling laws) for fair
samples of galaxies
- to derive scaling laws and stellar population
properties for magnitude-limited samples in the "ultra deep" field.
- This leads to an estimated need of 30 nights for the local
sample, 28 nights for the distant sample, and 15 nights for the "ultra
deep" field (this last to be coordinated with the supernovae survey).
In total, we estimate that we need 55 VIMOS nights for the completion
of the bulk of the VESUVIO survey, plus 15 nights for the ultra-deep
field coordinated with the supernovae survey. This requires
approximately 70 VLT-VIMOS nights.
- define and carry out a spectroscopic survey of Hercules to obtain
redshifts (magnitude-limited, TBD) for LSS and LS dynamics and LFs
- find other facilities for redshifts- AAOmega
Paola Merluzzi, Scott Trager, Jim Rose, Matthew Fleenor,
Gianni Busarello, Massimo Capaccioli,
Amata Mercurio, FL B, Reynier Peletier, Manolis Plionis, A. Rifatto, G.
Sorrentino, Rien van de Weijgaert>
Pages maintained by Gijs