View - ResearchGate

More documents

Recommendations

Info

Hα@z=0.8: SFR Hα-based excess? Villar et al 08 The star formation rate density is 0.17 M yr -1 Mpc 3 , ~10-15 times higher than the local one. SFRd Hα evolution: ∝ (1+z) β β=3.8±0.5 Jesús Gallego – UCM Granada 2008 32
Hα@z=0.8: Field-to-field variance Villar et al 08 Field to field variances ~3x Jesús Gallego – UCM Granada 2008 33
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: Hα Luminosity Function @ z=0.8 Vil
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

View - ResearchGate

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?