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Hα @ z=0.8 Villar et al 08 CAHA3.5m / Ω-2000 1,21 μm narrow-band filter, J band ~10 4 s exposures Groth strip, GOODS-N 0.31 sqr deg 165 objects J NB HST extended Groth strip WHT4.2m / INGRID 1,18 μm NB, J band ~10 4 s exposures Groth strip 32 sqr arcmin ~15 objects J NB
Photo-redshifts Villar et al 08 Sextractor stellarity BzK criterium (Daddi+04) IRAC and nIR criteria (Eisenhardt+04) Photometric redshifts from Pérez-González+05,08 BRI criteria (Fujita+03) z < 0.7 B-R C z > 0.7 R C -I C
Page 1 and 2: An Hα approach to the evolution of
Page 3 and 4: Observational tests: The cosmic SFR
Page 5 and 6: Galaxy evolution: SFR tracers SFR [
Page 7 and 8: Downsizing since z
Page 9 and 10: Open questions How the overall pic
Page 11 and 12: The Hα approach Evolution of the
Page 13 and 14: Redshifts considered z=0.02 6563Å
Page 21 and 22: Hα@z=0.24: Disk-like objects Pascu
Page 23 and 24: Hα@z=0.24: Contaminants • Ugriz
Page 25 and 26: Contaminants • 2 objects are sele
Page 27: Hα @ z=0.40: SFRdensity Jesús
Page 31 and 32: Hα Luminosity Function @ z=0.8 Vil
Page 33 and 34: Hα@z=0.8: Field-to-field variance
Page 35 and 36: Hα-based Madau plot Villar et al 0
Page 37 and 38: On the nature of Hα @ z=0.8 Most
Page 39 and 40: Hα @ z=0.8 IRAC data for stellar m
Page 41 and 42: EW(OII) vs. M B Disk-like spectros
Page 43 and 44: On the nature of Hα @ z=0.8 A. Sá
Page 45 and 46: SFR tot - M* relation Massive galax
Page 47 and 48: The first quantification of downsiz
Page 49 and 50: Future studies @ z>1.5 Jesús G
Page 51 and 52: FISIR: a fully criogenic TF in the

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