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ALMA Early Science: Submm Galaxies

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There are only ~200 SMGs in ALMA-accessible fields... Mix of detailed investigation of well-studied SMGs, detection of fainter pops ... – PowerPoint PPT presentation

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Title: ALMA Early Science: Submm Galaxies


1
ALMA Early ScienceSubmm Galaxies
  • Submm galaxies (SMGs)
  • ALMA accessible sub/mm-surveys
  • COSMOS - COSBO
  • SXDF - SHADES
  • ECDFS - LESS
  • CUDSS-3hr, SA22, cluster lenses, etc
  • (A370, Cl2244, MS0451, etc)
  • S2CLS - SCUBA2 Cosmology Legacy Survey

Ian Smail, Durham
2
SMGs - Submm Galaxies
  • Submm galaxies
  • SMGs with S850umgt3-5mJy (confusion limit)
    and z2.2 LFIRgt1012Lo Ultraluminous Infrared
    Galaxies (ULIRGs)
  • Most FIR-luminous sources at high-z, massive,
    gas-rich
  • Proto-ellipticals?

Lagache et al. 2003
Greve et al. 2005
Chapman et al. 2005
Tacconi et al. 2008
3
SHADES - SXDF
Coppin et al. 2006
60 SHADES 850um sources in SXDF gt3.3?
?870um2mJy 38 have radio IDs (Ivison et al.
2007) 1.1mm AzTEC survey of SXDF 28srcs in 0.37
deg2 (Austermann et al. 2009)
Chapman et al. 2005
Pope et al. 2006
Clements et al. 2008
4
COSBO
Bertoldi et al. 2006
MAMBO 1.2mm Array _at_ IRAM 30m telescope Observatio
ns 80hrs on-source (in total 120 hrs)
240 arcmin2 area resolution 11 FWHM
rms 1 mJy/beam 15 sources S/N gt 4 (12
S/Ngt3 with radio counterparts) z4.5 SMG
identified with UV-bright merger, detected with
IRAM in CO4-3
Capak et al. 2008 Schinnerer et al. 2009
5
ECDFS
  • Southern field (03h -27deg)
  • Full 0.5x0.5 deg imaged in
  • Optical-NIR MUSYC/COMBO17
  • HST GEMS/GOODS
  • MIR/FIR (3.6-160um) GOODS/FIDEL/SIMPLE
  • 1.4GHz VLA
  • X-ray ECDFS 250ks/2Ms (5Ms?)
  • FIR (250, 350, 500um) BLAST (HerMES)
  • LABOCA survey (LESS) adds submm

6
LESS
Joint ESO/MPI project LABOCA ECDFS Submm Survey
(LESS) PIs Walter/Smail ESO Weiss MPI
40 co-Is 330hrs from ESOMPI Final map
finished in January, catalog paper (Weiss et al.
2009) submitted in next month 121 sources above
3.7? (4.5mJy) Currently the deepestlargest submm
survey. Awarded a VLT LP (200hrs with VIMOS
FORS2) for spectroscopy of SMGs (PI Smail)
40x40 30x30 _at_ 1.2mJy rms
Weiss et al. 2009
7
LESS
LESSJ03229.40 z4.76 - currently highest-z SMG
known
AGN-SB within 1Gyr of Big Bang Undetectable by
Herschel? There may be 10 others in LESS map
Coppin et al. 2009
8
LESS
Stacking probes sub-confusion population (ltmJy) -
LIRGs at zgt1
Greve et al. 2009
Exploit 45k photo-z in ECDFS Stack K-selected
samples Identify populations with average fluxes
0.5mJy at z2 Progenitors of normal galaxies?
9
SCUBA2
  • Field of view 8x8 10x SCUBA
  • 8 arrays of 40x32 TES detectors 4 at 850um, 4
    at 450um
  • Fully sampled imaging at 850 um
  • Currently being commissioned with engineering
    devices
  • Fully operational with full focal planes by Q4
    2009
  • Map 1 deg2 to confusion at 850um in 40hrs

10
SCUBA2 Cosmology Legacy Survey
  • 850um survey (2yr goal)
  • 20 deg2 ?870um0.7mJy
  • 450um survey (2yr goal)
  • 0.6 deg2 ?450um0.5mJy

S2CLS - UK/NL/Ca open consortium. Coordinators
Smail Dunlop (UK), van der Werf (NL), Halpern
(Ca)
11
Summary
  • There are only 200 SMGs in ALMA-accessible
    fields
  • We should have S2CLS sources by ALMA early
    science
  • However, were unlikely to have follow-up (zs,
    etc)
  • Mix of detailed investigation of well-studied
    SMGs, detection of fainter pops and
    identification work on S2CLS sources?
  • Science goals
  • Dynamics masses, mergers - triggering of
    activity, connection to z2 reddead galaxies?
  • SF extent mode of SF?
  • CO ladders gas masses, gas fractions -
    evolution and variation with AGN activity
    (feedback) e.g. gas in QSOs?
  • Dense gas tracers relation to SFRs?
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