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Revision 272013-10-02 - RichardDekany

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Introduction

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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 (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 Status

TMAS 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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Partnership

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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).
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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). Software has been developed by Ms. Jennifer Milburn of COO.
 

Revision 262013-09-29 - RichardDekany

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Revision 252013-09-26 - RichardDekany

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Revision 242013-04-22 - SergiHildebrandt

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Partnership

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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).
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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).
 

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.

Project Status

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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 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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Ten MilliArcsecond (TMAS) camera TWiki

Introduction

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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.
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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.
 

Project Status

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TMAS is in development phase and is expected to be ready for on-sky testing in June 2012.
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TMAS' first light happened the nights of September, 28-29, 2012. In October, 2012, TMAS had its second 'first light'.
 

Partnership

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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.
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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).
 

Revision 212012-10-28 - SergiHildebrandt

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Run Notes

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META FILEATTACHMENT attachment="121028UT_TMAS_Observing_Log-2.ods" attr="h" comment="" date="1351438226" name="121028UT_TMAS_Observing_Log-2.ods" path="121028UT_TMAS_Observing_Log-2.ods" size="31523" stream="121028UT_TMAS_Observing_Log-2.ods" user="Main.SergiHildebrandt" version="2"

Revision 202012-10-10 - RichardDekany

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 Team Meetings and Reviews

Run Notes

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Revision 192012-10-08 - RichardDekany

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Project Documentation

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Revision 182012-09-11 - RichardDekany

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Project Documentation

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Revision 172012-09-11 - RichardDekany

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Project Documentation

  • Science
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Revision 162012-08-16 - RichardDekany

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Ten MilliArcsecond (TMAS) camera TWiki

Introduction

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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.
>
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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.
 

Project Status

TMAS 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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Team Meetings and Reviews

Run Notes

 

Project Documentation

Revision 152011-12-03 - SergiHildebrandt

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Technical Library

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*Progress Report*
 Organized by Product Breakdown Structure

Revision 132011-11-02 - RichardDekany

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Ten MilliArcsecond (TMAS) camera TWiki

Introduction

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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 Status

TMAS 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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Ten MilliArcsecond (TMAS) camera TWiki

Introduction

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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.
>
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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.
 

Project Status

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TMAS is in development phase and is expected to be ready for on-sky testing in 2012B.
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TMAS is in development phase and is expected to be ready for on-sky testing in June 2012.
 

Revision 112011-08-15 - RichardDekany

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Revision 102011-08-03 - OirAdmin

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Ten MilliArcsecond (TMAS) camera TWiki

Introduction

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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 1k x 1k science-grade staring array (known as Palomar CCD21), a high-speed 512 x 512 Andor EMCCD camera, and an optional fiber output port for precision RV spectroscopy tests. It integrates an atmospheric dispersion corrector (ADC) and dual filter wheels.
>
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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.
 

Project Status

TMAS is in development phase and is expected to be ready for on-sky testing in 2012B.

Revision 92011-08-01 - OirAdmin

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OIR Palomar/TMAS Project web

Project Scope: Design, build, and deploy a diffraction-limited IR integral field spectrograph and imager

Partners: UCLA, Caltech, TMT, HIA

Available Information

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Ten MilliArcsecond (TMAS) camera TWiki

Introduction

TMAS is a simple visible-light imager system to enable high-angular-resolution science with PALM-3000. It consists of a 1k x 1k science-grade staring array (known as Palomar CCD21), a high-speed 512 x 512 Andor EMCCD camera, and an optional fiber output port for precision RV spectroscopy tests. It integrates an atmospheric dispersion corrector (ADC) and dual filter wheels.

Project Status

TMAS is in development phase and is expected to be ready for on-sky testing in 2012B.

Partnership

TMAS is a Caltech collaboration with scientists from JPL. The co-PI's are Drs Sergi Hildebrandt and Richard Dekany, Caltech.
Team Meetings and Reviews

Project Documentation

Technical Library

Organized by Product Breakdown Structure
 

Revision 82008-02-01 - RichardDekany

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OIR Palomar/TMAS Project web

Project 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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Partners: UCLA, Caltech, TMT, HIA
 

Available Information

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Welcome to the OIR Palomar/TMAS Project web

Project Scope: Design, build, and deploy a new leading-edge science capability

Partners: Caltech, ...

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OIR Palomar/TMAS Project web

Project Scope: Design, build, and deploy a diffraction-limited IR integral field spectrograph and imager

Partners: UCLA, Caltech, TMT

 

Available Information

Revision 52005-03-28 - TWikiContributor

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Welcome to the home of TWiki.Palomar/TMAS. This is a web-based collaboration area for ...
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Welcome to the Palomar/TMAS web

 
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Revision 42002-04-14 - PeterThoeny

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