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Scientific Drivers for ESO Future VLT/VLTI Instrumentation
MAXIMUS: Exploiting the Full Power of OzPoz
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Author(s):
Matthew Colless
,
Keith Taylor
Publication date
(Print):
2002
Publisher:
Springer-Verlag
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There is no author summary for this book yet. Authors can add summaries to their books on ScienceOpen to make them more accessible to a non-specialist audience.
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IET Power Engineering
Author and book information
Book Chapter
Pages
: 93-98
DOI:
10.1007/10857019_15
SO-VID:
9e4ab298-b060-4471-a267-1895e25e42f5
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Book chapters
pp. 3
Introduction to Meeting: Towards VLT/VLTI 2nd Generation Instruments
pp. 11
The Physics of Gamma-Ray Burst Afterglows and the Nature of Their Host Galaxies
pp. 23
Faint Object Spectroscopy and GRBs: The Need for a Spectroscopic Laboratory at the VLT
pp. 30
Absorption Studies with GRB Afterglows
pp. 36
Advanced Telerobotic Field Spectrometer
pp. 42
REM - Rapid Eye Mount. A Fast Slewing Robotized Telescope to Monitor the Prompt Infra-Red Afterglow of GRBs
pp. 48
Observing the First Galaxies - A Case for an Intermediate Resolution Multi-Object IR Spectrograph
pp. 54
3D Spatial Distribution of the Intergalactic Medium: The ESO Blues?
pp. 60
Galaxy Evolution from Deep Multicolor Surveys: The VLT Perspective
pp. 66
Astrophysical Applications of Tunable Imaging Filters for the VLT
pp. 72
High Redshift Ellipticals: Prospects for the VLT
pp. 78
Future VLT Instrumentation: An IoA View
pp. 81
Multi-Object Spectroscopy: The Faint Object Case
pp. 87
A Wide Field Multi-Object IR Imager and Spectrograph
pp. 93
MAXIMUS: Exploiting the Full Power of OzPoz
pp. 99
A Million Element Integral Field Unit (MEIFU)
pp. 108
A Mega Integral Field Spectrograph for the VLT
pp. 118
CROMOS: A Cryogenic Near-Infrared, Multi-Object Spectrometer for the VLT
pp. 128
Multiple Integral Field Spectroscopy
pp. 136
Crowded Field 3D Spectroscopy - The Next Step: First Light for PMAS
pp. 139
The FALCON Concept: Multi-Object Spectroscopy Combined with MCAO in Near-IR
pp. 149
Scientific Potential of Enhancing the Integral-Field Spectrometer SPIFFI with a Large Detector and High Spectral Resolution
pp. 158
Multi-Conjugate Adaptive Optics with Laser Guide Stars
pp. 164
MOEMS, Key Optical Components for the Future Instrumentation of VLT
pp. 169
Spectroscopy of Faint Emission Line Nebulae
pp. 175
Near-IR Spectroscopy with VLT/ISAAC: Distribution and Kinematics of Molecular Gas in the Nucleus of NGC 1068
pp. 178
Dwarf Galaxies in the Local Group: The VLT Perspective
pp. 184
Identification and Study of Blue Supergiants in Nearby Galaxies
pp. 190
Quantitative Spectroscopy of Local Group Supergiants
pp. 193
A Super-Imaging Fourier Transform Spectrometer for the VLT
pp. 199
Rectifying Échelle Spectra - A Comparison Between UVES, FEROS and FOCES
pp. 205
Scientific Objectives and Design Study of an Adaptive Optics Visual Echelle Spectrograph and Imager Coronograph (AVES-IMCO) for the NAOS Visitor Focus at the VLT
pp. 213
Massive Spectroscopy of (Stellar) Fields
pp. 219
Stellar Oscillations Studies with STOMACH
pp. 225
Proposal for a VLT Multichannel Infrared Heterodyne Instrument Based on THIS (Tuneable Heterodyne Infrared Spectrometer)
pp. 231
Imaging Polarimetry and Spectropolarimetry of Bright Objects
pp. 238
High-Resolution Spectropolarimetry on the VLT
pp. 244
Transmission Spectroscopy for Extrasolar-Planet Studies: UVES Search and Future Prospects
pp. 247
Zero Noise CCD: A New Readout Technique for Extremely Low Light Levels
pp. 253
A Differential Imager for Adaptive Optics
pp. 258
Very Accurate Imaging of the Close Environment of Bright Objects in Visible and Near-Infrared
pp. 264
High-Contrast Imaging Science with Adaptive Optics
pp. 267
Coronagraphy with 4Q Phase Mask on the VLT
pp. 273
Achromatic Interfero-Coronagraphy and VLT
pp. 279
Growing Up - The Completion of the VLTI
pp. 289
The VLTI Adulthood: Scientific Drivers for Future VLTI Instrumentation
pp. 293
Imaging Interferometry - Experience from COAST and Implications for the VLTI
pp. 303
VLTI Imaging Instrument Using the Full Potential of the Interferometric Array
pp. 311
The Pre-PRIMA Survey Project: Turning the Problem Around
pp. 314
The Scientific Potential of MIDI in the 20 μm Window
pp. 320
The Potential of an Extension of Amber to the Visible
pp. 328
FINITO: A Fringe Sensor for VLTI in Two and Three Beam Configuration
pp. 331
Scientific Drivers for a Future Polarimetric Mode for the VLTI: VISPER
pp. 334
Search and Characterization of Extrasolar Planets Using VLT/VLTI Instrumentation
pp. 340
Optimizing a Differential Interferometric Instrument
pp. 347
NEVEC: The NOVA ESO VLTI Expertise Centre
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