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Phase II of the EVLA

Phase II of the EVLA

Phase II of the EVLA. Rick Perley EVLA Project Scientist. What is the Future for cm-wavelength Astronomy?. Any attendee of a recent AAS Meeting will know that astronomy is hardly in a state of decline.

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677 views • 58 slides
Astronomical Observational Techniques and Instrumentation

Astronomical Observational Techniques and Instrumentation

Astronomical Observational Techniques and Instrumentation. Professor Don Figer Radio Astronomy. Aims of Lecture. review radio imaging chain describe radio sources describe radio detection describe some common radio telescopes give examples of radio objects. Radio Imaging Chain.

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515 views • 51 slides
Astronomical Observational Techniques and Instrumentation

Astronomical Observational Techniques and Instrumentation

Astronomical Observational Techniques and Instrumentation. RIT Course Number 1060-771 Professor Don Figer Radio Astronomy. Aims of Lecture. review radio imaging chain describe radio sources describe radio detection describe some common radio telescopes give examples of radio objects.

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513 views • 51 slides
Astronomical Observational Techniques and Instrumentation

Astronomical Observational Techniques and Instrumentation

Astronomical Observational Techniques and Instrumentation. Professor Don Figer Radio Astronomy. Aims of Lecture. review radio imaging chain describe radio sources describe radio detection describe some common radio telescopes give examples of radio objects. Radio Imaging Chain.

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512 views • 51 slides
Thijs de Graauw

Thijs de Graauw

Thijs de Graauw. Instrument Top Level Requirements and Resulting Concept. Heterodyne spectroscopy single pixel on the sky very high spectral resolution 7 dual-pol mixer bands 480-1250 GHz (625-240 m m) 5x2 SIS mixers, IF 4-8 GHz 1410-1910 GHz(212-157 m m; 2x2 HEB mixers,

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237 views • 9 slides
Microwave Capabilities Multi-layer Modules

Microwave Capabilities Multi-layer Modules

Microwave Multi-layer Modules. Microwave Capabilities Multi-layer Modules. Wide Band IFM Receiver. Wide Band IFM Receiver. Main Characteristics: Instantaneous frequency coverage: UHF to Ku Band. Channelized receiver architecture for interference protection and high sensitivity.

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302 views • 6 slides

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