'16 ghz' presentation slideshows

MUSE & ALMA

430 views • 30 slides

A 30 GHz Real-Time Digitizing Oscilloscope February 12, 2009

A 30 GHz Real-Time Digitizing Oscilloscope February 12, 2009. Why Would You Need 30 GHz? Bandwidth requirements related to signal speed. 5 th harmonic. Power spectral density (dB). This plot shows Power Spectral Density (PSD) as a function of bit rate.

295 views • 18 slides

Radio Continuum Observations of Low Mass Young Stars Driving Outflows

Radio Continuum Observations of Low Mass Young Stars Driving Outflows. Rachael Ainsworth (DIAS) Radio Stars and Their Lives in the Galaxy 3-5 October 2012. Overview. Introduction Observations & Results: AMI Spectral Energy Distributions Radio Luminosity Correlations Summary of Results

152 views • 15 slides

FUTURE DIRECTIONS ON THE VLBA

FUTURE DIRECTIONS ON THE VLBA. Craig Walker National Radio Astonomy Observatory. IVS General Meeting Ottawa, Feb 2004. OUTLINE. Mark5 High frequency upgrades Spacecraft tracking Ka band receiver EVLA Receivers LO/IF (bandwidth, fibers etc) Correlator New Mexico Array

246 views • 13 slides

SZ effect

Observing the SZ Effect with the IRAM 30-meter and the Plateau de Bure Interferometer (on behalf of Francois-Xavier Desert). SZ effect. Diffraction is 18" at 2 mm. - High resolution measurements - Complement to X-ray data (XMM-Newton, Chandra, Rosat) and the future Planck. Diabolo cryostat

333 views • 12 slides

SZ effect

Observing the SZ Effect with the IRAM 30-meter and the Plateau de Bure Interferometer (on behalf of Francois-Xavier Desert). SZ effect. Diffraction is 18" at 2 mm. - High resolution measurements - Complement to X-ray data (XMM-Newton, Chandra, Rosat) and the future Planck. Diabolo cryostat

260 views • 12 slides

Correlator Specifications

229 views • 11 slides