1. SINFONI observations of massive galaxies from the GMASS sample at z~2
GMASS3D
Jaron Kurk - MPIA, Heidelberg
A. Cimatti (P.I.), N. Foerster Schreiber, N. Bouche, G. Cresci, R. Genzel, E. Daddi, A. Renzini, L. Pozzetti, G. Zamorani, M. Mignoli,
P. Cassata, A. Franceschini, G. Rodighiero, P. Rosati, M. Dickinson
3D2008, Garching
Jaron Kurk (MPIA, Heidelberg)

2. Jaron Kurk (MPIA, Heidelberg)
GMASS2D
Galaxy Mass Assembly ultra-deep Spectroscopic Survey
Ha in H and K band
Sample selected with m(4.5mu)<23.0, B<26.5, I<26.5, zphot>1.4, avoid known redshifts.
Goals: study galaxies selected on mass, explore redshift desert, high-z LF.
Method: SED fitting, up to 30h optical spectroscopy with FORS, total of 145h.
Results: ~150 redshifts out of 170 observed, >130 at z>1.4.
3D2008, Garching
Jaron Kurk (MPIA, Heidelberg)

3. Jaron Kurk (MPIA, Heidelberg)
The 3D sample
18.2 < K < 20.9
9.6 < log M* < 11.0
Selection on exact redshift, estimate of SFR, ACS/NICMOS morphology.
Blue: z=1.5, red: z=2.4.
3D2008, Garching
Jaron Kurk (MPIA, Heidelberg)

4. Jaron Kurk (MPIA, Heidelberg)
GMASS1084 K=19.6 z=1.552
3D2008, Garching
Jaron Kurk (MPIA, Heidelberg)

5. Jaron Kurk (MPIA, Heidelberg)
GMASS2113 K=20.2 z=1.613
3D2008, Garching
Jaron Kurk (MPIA, Heidelberg)

6. Jaron Kurk (MPIA, Heidelberg)
GMASS2363 K=21.0 z=2.448
3D2008, Garching
Jaron Kurk (MPIA, Heidelberg)

7. Jaron Kurk (MPIA, Heidelberg)
GMASS2471 K=20.9 z=2.430
3D2008, Garching
Jaron Kurk (MPIA, Heidelberg)

8. Jaron Kurk (MPIA, Heidelberg)
Outlook
Uniqueness of GMASS SINFONI sample
selection in MIR (better measure of mass)
deep optical spectroscopy
HST optical and (some) NIR coverage
deep IRAC and MIPS coverage
also includes faint (K>20) targets
SINS integration
Velocity differences between optical and NIR lines
Derive metallicity from (stacked) optical spectra and NIR spectra
3D2008, Garching
Jaron Kurk (MPIA, Heidelberg)

9. Jaron Kurk (MPIA, Heidelberg)
3D2008, Garching
Jaron Kurk (MPIA, Heidelberg)