David Hughes

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Scientific rationale for next-generation (sub)millimetre surveys • improved accuracy in source-counts • greater dynamic range in measured source-counts • increased wavelength coverage 850µm JCMT SPITZER submm galaxy flux
larger telescopes higher resolution lower confusion limit increased sensitivity 170µm 850µm JCMT 3mm GTM/LMT SPITZER larger-format cameras increased field-of-view faster mapping speed improved source statistics
Page 1 and 2: Millimetre Cosmology with the Large
Page 3 and 4: Primary Science with the LMT The fo
Page 5 and 6: γ-ray to radio extragalactic backg
Page 7 and 8: Why (sub-)millimeter observations ?
Page 9 and 10: Local Ultra-luminous Infrared Galax
Page 11 and 12: Arp 220 (z=0.018) Building galaxies
Page 13 and 14: Evolution history of star-formation
Page 15 and 16: 1997 SCUBA - a feedhorn-coupled bol
Page 17 and 18: • Sub-mm surveys (source-counts)
Page 19: Summary from submillimeter galaxy (
Page 23 and 24: The formation & evolution of struct
Page 25 and 26: El Gran Telescopio Milimétrico The
Page 27 and 28: marzo 2005
Page 29 and 30: Location of Large Millimetre Telesc
Page 31 and 32: LMT site Volcán Sierra Negra (Tlil
Page 33 and 34: LMT Site-Monitoring Characteristic
Page 35 and 36: 225GHz (1.3mm) opacity variations i
Page 37 and 38: Effective area of (3-ring) 30-LMT 3
Page 40 and 41: LMT panel segments (#180 in 5 rings
Page 42 and 43: February - September 2008 • Compl
Page 44 and 45: First-light LMT instruments (commis
Page 46 and 47: AzTEC • 144 pixel Si-Ni spiderweb
Page 48 and 49: 1997 SCUBA - a feedhorn-coupled bol
Page 50 and 51: Resolving 100% of the mm-background
Page 52 and 53: Wide-area LMT surveys detecting the
Page 54 and 55: 3mm Redshift Receiver & Correlator
Page 56 and 57: Ultra wideband redshift search rece
Page 58 and 59: SPEED (SPEctral Energy Distribution
Page 60 and 61: Measurement of the S-Z effect towar
Page 62 and 63: AzTEC 1.1mm observing campaigns •
Page 64 and 65: z ~ 1.4
Page 66 and 67: Radially-increasing (factor x 5-10)
Page 68 and 69: Evolution of point-source contamina
Page 70 and 71:
Milagros Zeballos (INAOE)
Page 72 and 73:
AzTEC 1.1mm observing campaigns •
Page 74:
www.lmtgtm.org
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David Hughes

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