emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a...

18

Transcript of emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a...

Page 1: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 2: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 3: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 4: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 5: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 6: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 7: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 8: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 9: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 10: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 11: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 12: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 13: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 14: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 15: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 16: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 17: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992
Page 18: emissions for more than 40 years. These observations had been at fixed frequencies until 1988 when a spectrograph (70-500 MHz) with a 10-m antenna was built. In F Y 1992 (April 1992

FLAMES Fibre Large Array Multi-Element Spectrograph (

FLAMES Fibre Large Array Multi-Element Spectrograph (

FAINT OBJECT SPECTROGRAPH INSTRUMENT HANDBOOK A.L. … · Faint Object Spectrograph Instrument Handbook Version 5.0 1 INTRODUCTION The Faint Object Spectrograph and its use are described

FAINT OBJECT SPECTROGRAPH INSTRUMENT HANDBOOK A.L. … · Faint Object Spectrograph Instrument Handbook Version 5.0 1 INTRODUCTION The Faint Object Spectrograph and its use are described

Ultraviolet Spectrograph Telescopefor …€¦ · Web viewUltraviolet Spectrograph Telescopefor Astronomical Research (UVSTAR) UVSTAR, experiment was jointly developed by NASA and

Ultraviolet Spectrograph Telescopefor …€¦ · Web viewUltraviolet Spectrograph Telescopefor Astronomical Research (UVSTAR) UVSTAR, experiment was jointly developed by NASA and

Spectrograph Mode Overview

Spectrograph Mode Overview

EUCLID NEAR IR SPECTROGRAPH FOCAL PLANE

EUCLID NEAR IR SPECTROGRAPH FOCAL PLANE

The Optical Spectroscopy Division - Freesti.mermoz.free.fr/physique/TPMS_TS2/SERIE2_phyS_TS2/14...Spectrograph CP140 Imaging Spectrograph equipped with Symphony CCD detector CP140

The Optical Spectroscopy Division - Freesti.mermoz.free.fr/physique/TPMS_TS2/SERIE2_phyS_TS2/14...Spectrograph CP140 Imaging Spectrograph equipped with Symphony CCD detector CP140

Gemini Multi-Object Spectrograph · Gemini Multi-Object Spectrograph. Itajubá, 09 de abril de 2008 Rodrigo Carrasco 2 Gemini Multi-Object Spectrograph GMOS at Gemini North. Itajubá,

Gemini Multi-Object Spectrograph · Gemini Multi-Object Spectrograph. Itajubá, 09 de abril de 2008 Rodrigo Carrasco 2 Gemini Multi-Object Spectrograph GMOS at Gemini North. Itajubá,

IGRINS Immersion GRating INfrared Spectrograph: Current Design

IGRINS Immersion GRating INfrared Spectrograph: Current Design

Spectrograph Fundamentals

Spectrograph Fundamentals

Magellan Planet Finder Spectrograph

Magellan Planet Finder Spectrograph

LISA spectrograph Long slit Intermediate resolution Spectrograph for Astronomy Performances and application Christian Buil Active Spectroscopy in Astronomy.

LISA spectrograph Long slit Intermediate resolution Spectrograph for Astronomy Performances and application Christian Buil Active Spectroscopy in Astronomy.

Spectrograph Fundamentals DSS-7 Spectrograph by SBIG ST-7XME CCD Camera by SBIG .

Spectrograph Fundamentals DSS-7 Spectrograph by SBIG ST-7XME CCD Camera by SBIG .

Shamrock 500i Czerny-Turner Spectrograph

Shamrock 500i Czerny-Turner Spectrograph

Wide Field Optical Spectrograph - WFOS Architecture ...

Wide Field Optical Spectrograph - WFOS Architecture ...

SuperNova Integral Field Spectrograph

SuperNova Integral Field Spectrograph

The Subaru Prime Focus Spectrograph (PFS)...Spectrograph Mechanical Layout Each spectrograph carries 3 vacuum Schmidt cameras, f/1.10, with a 275mm beam. Modular design of cryostats

The Subaru Prime Focus Spectrograph (PFS)...Spectrograph Mechanical Layout Each spectrograph carries 3 vacuum Schmidt cameras, f/1.10, with a 275mm beam. Modular design of cryostats

R&O Buoy Spectrograph System

R&O Buoy Spectrograph System

The Mass Spectrograph & Average Atomic Mass

The Mass Spectrograph & Average Atomic Mass

A wide field spectrograph/camera

A wide field spectrograph/camera

AEOS Telescope + Image-Slicer/ Spectrograph

AEOS Telescope + Image-Slicer/ Spectrograph