Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki | ||||||||
Line: 24 to 24 | ||||||||
Added: | ||||||||
> > | ||||||||
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki
| ||||||||
Changed: | ||||||||
< < | 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. | ||||||||
Line: 13 to 13 | ||||||||
| ||||||||
Changed: | ||||||||
< < | TMAS is a Caltech collaboration with scientists from JPL. The co-PI's are Drs. Sergi R. Hildebrandt![]() | |||||||
> > | TMAS is a Caltech collaboration with scientists from JPL. The co-PI's are Drs. Sergi R. Hildebrandt![]() | |||||||
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki | ||||||||
Line: 23 to 23 | ||||||||
Added: | ||||||||
> > | ||||||||
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki | ||||||||
Line: 22 to 22 | ||||||||
Added: | ||||||||
> > | ||||||||
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki | ||||||||
Line: 13 to 13 | ||||||||
| ||||||||
Changed: | ||||||||
< < | TMAS is a Caltech collaboration with scientists from JPL. The co-PI's are Drs. Sergi R. Hildebrandt![]() | |||||||
> > | TMAS is a Caltech collaboration with scientists from JPL. The co-PI's are Drs. Sergi R. Hildebrandt![]() | |||||||
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki | ||||||||
Line: 8 to 8 | ||||||||
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.
Project Status | ||||||||
Changed: | ||||||||
< < | 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. | |||||||
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki
| ||||||||
Changed: | ||||||||
< < | 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. | |||||||
Project Status | ||||||||
Changed: | ||||||||
< < | 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'. | |||||||
| ||||||||
Changed: | ||||||||
< < | 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![]() | |||||||
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki | ||||||||
Line: 21 to 21 | ||||||||
Run Notes | ||||||||
Added: | ||||||||
> > | ||||||||
Line: 68 to 70 | ||||||||
(advanced search) \ No newline at end of file | ||||||||
Added: | ||||||||
> > |
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki | ||||||||
Line: 20 to 20 | ||||||||
Team Meetings and Reviews
Run Notes | ||||||||
Added: | ||||||||
> > | ||||||||
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki | ||||||||
Line: 26 to 26 | ||||||||
Project Documentation
| ||||||||
Changed: | ||||||||
< < | ||||||||
> > | ||||||||
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki | ||||||||
Line: 26 to 26 | ||||||||
Project Documentation
| ||||||||
Added: | ||||||||
> > | ||||||||
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki | ||||||||
Line: 25 to 25 | ||||||||
| ||||||||
Changed: | ||||||||
< < | ||||||||
> > | ||||||||
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki
| ||||||||
Changed: | ||||||||
< < | 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. | ||||||||
Line: 17 to 17 | ||||||||
Changed: | ||||||||
< < | Team Meetings and Reviews | |||||||
> > | Team Meetings and Reviews
Run Notes | |||||||
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki | ||||||||
Line: 35 to 35 | ||||||||
| ||||||||
Added: | ||||||||
> > | *Progress Report* | |||||||
Organized by Product Breakdown Structure
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki
| ||||||||
Changed: | ||||||||
< < | 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. |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki
| ||||||||
Changed: | ||||||||
< < | 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. | |||||||
Project Status | ||||||||
Changed: | ||||||||
< < | 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. | |||||||
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Ten MilliArcsecond (TMAS) camera TWiki | ||||||||
Line: 28 to 28 | ||||||||
| ||||||||
Added: | ||||||||
> > | ||||||||
Deleted: | ||||||||
< < | ||||||||
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
| ||||||||
Changed: | ||||||||
< < | 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
| |||||||
> > | Ten MilliArcsecond (TMAS) camera TWiki
| |||||||
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
OIR Palomar/TMAS Project webProject Scope: Design, build, and deploy a diffraction-limited IR integral field spectrograph and imager | ||||||||
Changed: | ||||||||
< < | Partners: UCLA, Caltech, TMT | |||||||
> > | Partners: UCLA, Caltech, TMT, HIA | |||||||
Available Information |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
| ||||||||
Changed: | ||||||||
< < | 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 | |||||||
Available Information |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Changed: | ||||||||
< < | Welcome to the Palomar/TMAS web | |||||||
> > |
Welcome to the OIR Palomar/TMAS Project webProject Scope: Design, build, and deploy a new leading-edge science capabilityPartners: Caltech, ... | |||||||
Available Information | ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
| |||||||
|
Line: 1 to 1 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Changed: | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
< < | Welcome to the home of TWiki.Palomar/TMAS. This is a web-based collaboration area for ... | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
> > | Welcome to the Palomar/TMAS web | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Changed: | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
< < | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
> > | Available Information
| |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Changed: | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
< < | Site Tools of the Palomar/TMAS WebNotes:
| |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
> > |
Line: 1 to 1 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Welcome to the home of TWiki.Palomar/TMAS. This is a web-based collaboration area for ... | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Changed: | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
< < | Maintenance of the Palomar/TMAS web | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
> > | Site Tools of the Palomar/TMAS Web | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Notes: | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Changed: | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
< < |
| |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
> > |
| |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
|
Line: 1 to 1 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Welcome to the home of TWiki.Palomar/TMAS. This is a web-based collaboration area for ... | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Line: 18 to 18 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Changed: | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
< < | Warning: Can't find topic TWiki.TWikiWebsTable | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
> > |
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Welcome to the home of TWiki.Palomar/TMAS. This is a web-based collaboration area for ... | ||||||||
Line: 8 to 8 | ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
| |||||||
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Added: | ||||||||
> > | Welcome to the home of TWiki.Palomar/TMAS. This is a web-based collaboration area for ...
Maintenance of the Palomar/TMAS webNotes:
|