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| < < | TMAS ("Thomas") is a simple visible-light imager system to enable high-angular-resolution science with PALM-3000. It consists of a high-speed 2.5k x 2.1k Andor NEO sCMOS camera, with an option of alternatively using a borrowed Andor 888 L3CCD which would provide higher QE but slower frame rate and smaller FoV in one of the arms. Future options include a fiber output port to support precision RV spectroscopy tests, or the addition of a tunable filter for ultra-narrow-band imaging. TMAS integrates an atmospheric dispersion corrector (ADC) and dual filter wheels. | |||||||
| > > | TMAS (aka "Thomas") is a simple visible-light imager system to enable high-angular-resolution science with PALM-3000. It consists of a high-speed 2.5k x 2.1k Andor NEO sCMOS camera, with an option of alternatively using a borrowed Andor 888 L3CCD which would provide higher QE but slower frame rate and smaller FoV in one of the arms. Future options include a fiber output port to support precision RV spectroscopy tests, or the addition of a tunable filter for ultra-narrow-band imaging. TMAS integrates an atmospheric dispersion corrector (ADC) and dual filter wheels. | |||||||
Project StatusTMAS first light happened the nights of September, 28-29, 2012. In October, 2012, TMAS had its second 'first light'. See Run Notes below. | ||||||||
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| < < | TMAS is a Caltech collaboration with scientists from JPL. The co-PI's are Drs. Sergi R. Hildebrandt (JPL/Caltech) and Richard Dekany (Caltech). | |||||||
| > > | TMAS is a Caltech collaboration with scientists from JPL. The co-PI's are Drs. Sergi R. Hildebrandt (JPL/Caltech) and Richard Dekany (Caltech). Software has been developed by Ms. Jennifer Milburn of COO. | |||||||
Revision 262013-09-29 - RichardDekany
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Revision 242013-04-22 - SergiHildebrandt
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| < < | TMAS is a Caltech collaboration with scientists from JPL. The co-PI's are Drs. Sergi R. Hildebrandt (JPL/Caltech) and Richard Dekany (Caltech). | |||||||
| > > | TMAS is a Caltech collaboration with scientists from JPL. The co-PI's are Drs. Sergi R. Hildebrandt (JPL/Caltech) and Richard Dekany (Caltech). | |||||||
Revision 232013-03-13 - SergiHildebrandt
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TMAS ("Thomas") is a simple visible-light imager system to enable high-angular-resolution science with PALM-3000. It consists of a high-speed 2.5k x 2.1k Andor NEO sCMOS camera, with an option of alternatively using a borrowed Andor 888 L3CCD which would provide higher QE but slower frame rate and smaller FoV in one of the arms. Future options include a fiber output port to support precision RV spectroscopy tests, or the addition of a tunable filter for ultra-narrow-band imaging. TMAS integrates an atmospheric dispersion corrector (ADC) and dual filter wheels.
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| < < | TMAS' first light happened the nights of September, 28-29, 2012. In October, 2012, TMAS had its second 'first light'. | |||||||
| > > | TMAS first light happened the nights of September, 28-29, 2012. In October, 2012, TMAS had its second 'first light'. See Run Notes below. | |||||||
Revision 222013-03-13 - SergiHildebrandt
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| < < | TMAS ("Thomas") is a simple visible-light imager system to enable high-angular-resolution science with PALM-3000. It consists of a pair of high-speed 2k x 2k Andor NEO sCMOS cameras (borrowed, for now), with an option of alternatively using a borrowed Andor 888 L3CCD which would provide higher QE but slower frame rate and smaller FoV in one of the arms. Future options include a fiber output port to support precision RV spectroscopy tests, or the addition of a tunable filter for ultra-narrow-band imaging. TMAS integrates an atmospheric dispersion corrector (ADC) and dual filter wheels. | |||||||
| > > | TMAS ("Thomas") is a simple visible-light imager system to enable high-angular-resolution science with PALM-3000. It consists of a high-speed 2.5k x 2.1k Andor NEO sCMOS camera, with an option of alternatively using a borrowed Andor 888 L3CCD which would provide higher QE but slower frame rate and smaller FoV in one of the arms. Future options include a fiber output port to support precision RV spectroscopy tests, or the addition of a tunable filter for ultra-narrow-band imaging. TMAS integrates an atmospheric dispersion corrector (ADC) and dual filter wheels. | |||||||
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| < < | TMAS is in development phase and is expected to be ready for on-sky testing in June 2012. | |||||||
| > > | TMAS' first light happened the nights of September, 28-29, 2012. In October, 2012, TMAS had its second 'first light'. | |||||||
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| < < | TMAS is a Caltech collaboration with scientists from JPL. The co-PI's are Drs Sergi Hildebrandt and Richard Dekany, Caltech. | |||||||
| > > | TMAS is a Caltech collaboration with scientists from JPL. The co-PI's are Drs. Sergi R. Hildebrandt (JPL/Caltech) and Richard Dekany (Caltech). | |||||||
Revision 212012-10-28 - SergiHildebrandt
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Revision 202012-10-10 - RichardDekany
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Revision 192012-10-08 - RichardDekany
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Revision 182012-09-11 - RichardDekany
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Revision 172012-09-11 - RichardDekany
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Revision 162012-08-16 - RichardDekany
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| < < | TMAS is a simple visible-light imager system to enable high-angular-resolution science with PALM-3000. It consists of a pair of high-speed 2k x 2k Andor NEO sCMOS cameras (borrowed, for now), with an option of alternatively using a borrowed Andor 888 L3CCD which would provide higher QE but slower frame rate and smaller FoV in one of the arms. Future options include a fiber output port to support precision RV spectroscopy tests, or the addition of a tunable filter for ultra-narrow-band imaging. TMAS integrates an atmospheric dispersion corrector (ADC) and dual filter wheels. | |||||||
| > > | TMAS ("Thomas") is a simple visible-light imager system to enable high-angular-resolution science with PALM-3000. It consists of a pair of high-speed 2k x 2k Andor NEO sCMOS cameras (borrowed, for now), with an option of alternatively using a borrowed Andor 888 L3CCD which would provide higher QE but slower frame rate and smaller FoV in one of the arms. Future options include a fiber output port to support precision RV spectroscopy tests, or the addition of a tunable filter for ultra-narrow-band imaging. TMAS integrates an atmospheric dispersion corrector (ADC) and dual filter wheels. | |||||||
Project StatusTMAS is in development phase and is expected to be ready for on-sky testing in June 2012. | ||||||||
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| < < | Team Meetings and Reviews | |||||||
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Revision 152011-12-03 - SergiHildebrandt
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Revision 132011-11-02 - RichardDekany
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| < < | TMAS is a simple visible-light imager system to enable high-angular-resolution science with PALM-3000. It consists of a pair of high-speed 2k x 2k Andor NEO sCMOS cameras (borrowed, for now), with an option of alternatively using a borrowed Andor 888 L3CCD which would provide higher QE but slower frame rate and smaller FoV in one of the arms. Future options include a fiber output port to support precision RV spectroscopy tests. TMAS integrates an atmospheric dispersion corrector (ADC) and dual filter wheels. | |||||||
| > > | TMAS is a simple visible-light imager system to enable high-angular-resolution science with PALM-3000. It consists of a pair of high-speed 2k x 2k Andor NEO sCMOS cameras (borrowed, for now), with an option of alternatively using a borrowed Andor 888 L3CCD which would provide higher QE but slower frame rate and smaller FoV in one of the arms. Future options include a fiber output port to support precision RV spectroscopy tests, or the addition of a tunable filter for ultra-narrow-band imaging. TMAS integrates an atmospheric dispersion corrector (ADC) and dual filter wheels. | |||||||
Project StatusTMAS is in development phase and is expected to be ready for on-sky testing in June 2012. | ||||||||
Revision 122011-10-06 - RichardDekany
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| < < | TMAS is a simple visible-light imager system to enable high-angular-resolution science with PALM-3000. It consists of a high-speed 1k x 1k Andor EMCCD camera (borrowed, for now), an optional k x 1k science-grade staring array (known as Palomar CCD21) which would provide higher sensitivity, and an optional fiber output port for precision RV spectroscopy tests. It integrates an atmospheric dispersion corrector (ADC) and dual filter wheels. | |||||||
| > > | TMAS is a simple visible-light imager system to enable high-angular-resolution science with PALM-3000. It consists of a pair of high-speed 2k x 2k Andor NEO sCMOS cameras (borrowed, for now), with an option of alternatively using a borrowed Andor 888 L3CCD which would provide higher QE but slower frame rate and smaller FoV in one of the arms. Future options include a fiber output port to support precision RV spectroscopy tests. TMAS integrates an atmospheric dispersion corrector (ADC) and dual filter wheels. | |||||||
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| < < | TMAS is in development phase and is expected to be ready for on-sky testing in 2012B. | |||||||
| > > | TMAS is in development phase and is expected to be ready for on-sky testing in June 2012. | |||||||
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| < < | OIR Palomar/TMAS Project webProject Scope: Design, build, and deploy a diffraction-limited IR integral field spectrograph and imagerPartners: UCLA, Caltech, TMT, HIA Available Information
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OIR Palomar/TMAS Project webProject Scope: Design, build, and deploy a diffraction-limited IR integral field spectrograph and imager | ||||||||
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| < < | Partners: UCLA, Caltech, TMT | |||||||
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| < < | Welcome to the OIR Palomar/TMAS Project webProject Scope: Design, build, and deploy a new leading-edge science capabilityPartners: Caltech, ... | |||||||
| > > | OIR Palomar/TMAS Project webProject Scope: Design, build, and deploy a diffraction-limited IR integral field spectrograph and imagerPartners: UCLA, Caltech, TMT | |||||||
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| < < | Welcome to the Palomar/TMAS web | |||||||
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Revision 42002-04-14 - PeterThoeny
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