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Hα@z=0.8: Massive systems O Local M~ K R e σ 2 ~10 11 Mo, Evidence of downsizing
On the nature of Hα @ z=0.8 A. Sánchez thesis @ UCM WHT/LIRIS near-IR spectroscopy WHT/LIRIS-MOS Hβ, [OIII]5007, Hα, [NII]6584 J-band, R∼700, 0”25/pix Hα for ∼30 NB galaxies Jesús Gallego – UCM Granada 2008 43
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 and 28: Hα @ z=0.40: SFRdensity Jesús
Page 29 and 30: Photo-redshifts Villar et al 08 Se
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: EW(OII) vs. M B Disk-like spectros
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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