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

More documents

Recommendations

Info

SMGs point-sources Advantage of higher-resolution observations: with Large Millimeter Telescope SZE + SMGs 60 arcsec FWHM SZE with pt-sources identified with highresolution mask & removed SZE only + σ~4 mJy noise (input map) simulacion por Alfredo Montaña (tesis)
Conclusions • LMT (32-m) is nearing completion of construction phase • mechanical & drive-control systems working • installation of M2 & M3 mirrors and M1 surface alignment required before scientific commissioning begins • first-light & commissioning instrumentation ready (optical camera, holography receiver, Rx-z & AzTEC) • first-light science in 32-m format expected in early 2010 • funding being sought for completion of 50-m surface
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 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: SMGs point-sources SZE with pt-sour
Page 65: Conclusions • Increasing likeliho
show all

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

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?