Molecular Gas at High Redshift

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Ω(SFR) [Msun yr -1 Mpc -3 ] Research in last decade - Cosmic Evolution of the cosmic star form<strong>at</strong>ion r<strong>at</strong>e density t(Gyr) Deep fields: 100s hours,
A typical dusty high-redshift SED JWST SPICA ALMA+CCAT EVLA CNO fine structure lines CO ‘ladder’ PAHs + SiO Thermal dust(young stars)!
Page 1 and 2: Molecular Gas at High Redshift Fabi
Page 3: Ω(SFR) [Msun yr -1 Mpc -3 ] Resear
Page 7 and 8: frequency [GHz] practical issues CO
Page 9 and 10: frequency [GHz] practical issues CO
Page 11 and 12: Carilli & Walter, in prep. high red
Page 13 and 14: integrated CO emission CO velocity
Page 15 and 16: Other tracers at high density HCN 1
Page 17 and 18: Lensing helps The Eyelash CO(1-0) C
Page 19 and 20: Low-J observations: JVLA -- merger
Page 21 and 22: CO excitation: High Redshift T kin
Page 23 and 24: Evolutionary Sequence? L FIR , SFR,
Page 25 and 26: FIR vs. CO luminosity N=1.4 Kennicu
Page 27 and 28: Location of BzK galxies in ‘SF la
Page 29 and 30: Going from luminosities to masses F
Page 31 and 32: log (SFR surface density) high reds
Page 33 and 34: frequency [GHz] molecular deep fiel
Page 35 and 36: Full ALMA total ~300 hours FOV = 26
Page 37 and 38: predictions by numerical simulation
Page 39 and 40: frequency [GHz] first molecular dee
Page 41 and 42: spectrum at position of HDF850.1 Th
Page 43 and 44: The Case of HDF850.1 spectrum at po
Page 45 and 46: The Case of HDF850.1 spectrum at po
Page 47 and 48: lind detection of other sources: ex
Page 49 and 50: going to the highest redshifts, z>>
Page 51 and 52: CO line redshift coverage for ALMA
Page 53 and 54: CO line redshift coverage for ALMA
Page 55 and 56:
[CII] to the rescue? LMC may be eas
Page 57 and 58:
Maximum Starburst at z=6.4 - resolv
Page 59 and 60:
quick poll! SFRSD=1000 M sun yr -1
Page 61 and 62:
Walter et al. 2012 Search for [CII]
Page 63 and 64:
ALMA: An SMG-Quasar pair at z=4.7 B
Page 65 and 66:
[NII] as a tracer of ionized medium
Page 67:
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Molecular Gas at High Redshift

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