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AzTEC 4c41-17 AzTEC/SHADES Lockman Hole AzTEC GOODS-N Perera et al. 2008 AzTEC/SHADES SXDF Austermann et al. 2008b AzTEC/ASTE Data from 2008 AzTEC/ASTE Data from 2007 Expect >1000 SMGs in final catalog. Robust statistical comparisons of source populations finally possible. AzTEC MS0451 AzTEC COSMOS Scott et al. 2008 Austermann et al. 2008a Millennium Simulation 1 º x1 º at z=1.4 Submm survey 1 sigma depth [1.1mm mJy] 2 1.8 1.4 1.0 0.7 0.6 MAMBO Lockman Hole SCUBA/SHADES Greve et al. 2004 Lockman Hole Dunlop etal. 2006 Bolocam Lockman Hole Laurent et al. 2005 CUDSS Eales et al. 2000 CUDSS Eales et al. 2000 SCUBA/SHADES SXDF Dunlop et al. 2006 Hughes HDF HDF Super-map Borys etal. MAMBO COSMOS Bertoldi et al. 2007 Bolocam COSMOS Aguirre et al. 2008 MAMBO Elais-N2 Greve et al. 2004
Comparison of LMT and other facilities TolTEC adapted from CCAT Feasibility/Concept Study Review CCAT 850 microns AzTEC on LMT comparable mapping speed to SCUBA-2 (0.55 sq. degs/hr/mJy^2) Large-format camera (TolTEC) with 6400 pixels at 1.1mm we expect (10 sq. degs/hr/mJy^2) • TolTEC more than 100x faster than ALMA detection rate for sources > 0.5mJy sources at 1.1mm
Page 1 and 2: The Large Millimeter Telescope Davi
Page 3 and 4: The LMT/GTM project The LMT book El
Page 5 and 6: Cosmology at millimeter-wavelengths
Page 7 and 8: Volcán Sierra La Negra (97 o 18’
Page 9 and 10: LMT site Volcán Sierra Negra (Tlil
Page 11 and 12: 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: . Arp 220 (z=0.018) L FIR = 2x10 12
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 and 64: Conclusions • LMT (32-m) is neari
Page 65: Conclusions • Increasing likeliho

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