The Large Millimeter Telescope - Berkeley Center for Cosmological ...

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Conclusions • SEQUOIA, Redshift receiver & AzTEC all commissioned and have operated as scientific instruments on other 10- 15m class (sub-)mm telescopes • AzTEC completed 3 seasons on JCMT and ASTE. • blank-fields (GOODS-N, COSMOS, CDFS, Lockman Hole, SXDF, SEP, ….) • biased-fields (ACES survey – 40 HzRG and cluster environments) • ~3 sq. degrees surveyed at 18-30 arcsec resolution. > 2000 SMGs detected (>>10^12 Lsun, SFR >> 100 Msun/yr)
Conclusions • Increasing likelihood that ACT, SPT, Planck (i.e. low- • resolution experiments, > 1 arcmin beams) will suffer from • pt-source contamination from lensed SMG population and • SMGs intrinsic to high-z clusters • Need higher-resolution (5- 20 arcsec) observations (e.g. • LMT) to complement SZE survey experiments and • maximise the accuracy of cosmological parameters and • understanding of cluster physics derived from arcminute- • resolution SZE observations
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The Large Millimeter Telescope Davi
Page 3 and 4:
The LMT/GTM project The LMT book El
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Cosmology at millimeter-wavelengths
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Volcán Sierra La Negra (97 o 18’
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LMT site Volcán Sierra Negra (Tlil
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Monthy-averaged opacity above LMT s
Page 13 and 14: LMT panel segments
Page 15 and 16: Surface Alignment • Inner 32-m in
Page 17 and 18: Effective area of (5-ring) 50m LMT
Page 19 and 20: March 2006
Page 21 and 22: First-light Instrumentation Overvie
Page 23 and 24: Future Instrument Development • C
Page 25 and 26: LMT 12GHz holography map (inner 32-
Page 27 and 28: Taurus Molecular Cloud Survey (FCRA
Page 29 and 30: D.2. “How do galaxies arise and m
Page 31 and 32: • 144-pixel Si-Ni spiderweb bolom
Page 33 and 34: . Arp 220 (z=0.018) L FIR = 2x10 12
Page 35 and 36: Comparison of LMT and other facilit
Page 37 and 38: LMT advantage - sensitivity & resol
Page 39 and 40: Resolving the FIR extragalactic bac
Page 41 and 42: LMT Redshift Search Receiver bandwi
Page 43 and 44: Ultra Wideband Redshift Search Rece
Page 45 and 46: Room temp frontend components mount
Page 47 and 48: Beams separated in azimuth with spa
Page 49 and 50: CO (1-0) Survey of Local ULIRGs T s
Page 51 and 52: LMT High-redshift molecular-line sp
Page 53 and 54: Point-source contamination of the S
Page 55 and 56: 12 mJy pt-source + SZ ~ 3 mJy/beam
Page 57 and 58: Lensing the millimeter galaxy popul
Page 59 and 60: Confusion-limit due to SMG populati
Page 61 and 62: SMGs point-sources SZE with pt-sour
Page 63: Conclusions • LMT (32-m) is neari
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The Large Millimeter Telescope - Berkeley Center for Cosmological ...

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