Science with the VLT in the ELT Era [electronic resource] /
Moorwood, Alan F.M.editor.
European Southern Observatory.
The Workshop “Science with the VLT in the ELT Era” held in Garching from 8th to 12th October 2007 was organised by ESO, with support from its Scienti c and Technical Committee, to provide a forum for the astronomical community to debate the long term future of ESO’s Very Large Telescope (VLT) and its interferometric mode (VLTI). In particular it was considered useful for future planning to evaluate how its science use may evolve over the next decade due to competition and/or synergy with new facilities such as ALMA, JWST and, hopefully, at least one next generation 30–40 m extremely large telescope whose acronym appears in the title to symbolise this wider context. These discussions were also held in the fresh light of the Science Vision recently developed within ASTRONET as the rst step towards a 20 year plan for implementing astronomical facilities—the rst such attempt within Europe. Speci c ideas and proposals for new, second generation VLT/I instruments were also solicited following a tradition set by several earlier Workshops held since the start of the VLT development. The programme consisted of invited talks and reviews and contributed talks and posters. Almost all those given are included here although, unfortunately not the several lively but constructive discussion sessions.
Description based upon print version of record.
VLT Science Highlights; Pushing the VLT Spectroscopy of Distant Galaxies to the Limits and Future Prospects; Pushing FORS to the Limit-A New Population of Faint Extended Ly a Emitters at z ~3; VIMOS Integral Field Spectroscopy of Gaseous Nebulae in Local Group Dwarf Galaxies; Near IR Integral Field Spectroscopy of a Nearby Starburst; The ESO Large Programme "First Stars"; The Contribution of UVES@VLT to the New Era of QSO Absorption Line Studies; IMAGES: A Unique View of the Galaxy Mass Assembly Since z =1; The Metallicity Evolution at High Redshift; Near-IR Spectroscopy of Blue Supergiants
Integral Field Spectroscopy of Protoplanetary Disks in Orion with VLT FLAMESMAD@VLT: Deep into the Madding Crowd of Omega Centauri; Chemical Evolution of the Galaxy and Supernova Yields after UVES; VLTI Science Highlights; MIDI Sees Active Galactic Nuclei; The Use of the VLTI for Studying the Asymmetric Mass Loss of Evolved Stars; Mid-infrared Interferometric Observations of Young Circumstellar Discs; VLTI-AMBER Observations of . Carinae with High Spatial Resolution and Spectral Resolutions of . /. . =1500 and 12.000*
Resolving the Inner Active Accretion Disk Around the Herbig Be Star MWC 147 with VLTI/MIDI.+.AMBER Spectro-interferometryMulti-epoch VLTI/MIDI Observations of the Carbon-rich Mira Star V Oph; A Mid-infrared Interferometric Study of the Circumstellar Environment of Dusty OH/IR Stars with VLTI/MIDI; The Closest Dusty Cloud Ever Detected Around a R CrB Variable Star Using the VLTI/MIDI Instrument; A Twenty Year Science Vision for European Astronomy; Baryonic Acoustic Oscillations; Galaxy Formation and Evolution; Exoplanets: The Road to Earth Twins
Next Generation Deep Redshift Surveys with the VLTGUAIX: The UCM Group of Extragalactic Astrophysics and Astronomical Instrumentation; VISTA Public Surveys and VLT followup; Probing Dark Energy with Cosmological Redshift Surveys at the VLT; The First Galaxies and Galaxy Clusters; Narrow Band Surveys and the Epoch of Reionization; Stellar Archaeology and Galaxy Genesis: The Need for Large Area Multi-Object Spectrograph on 8 m-Class Telescopes; Near-field Cosmology with the VLT; Chemical Evolution of Local Group Galaxies
The VLTI as a Tool to Study Eclipsing Binaries for an Improved Distance ScaleStatus of the European ELT; The Science Case for the European ELT; GRB Afterglows in the ELT Era; On the Way to an E-ELT Instrumentation Plan; From ESPRESSO to CODEX; First Results of AQuEye, a Precursor 'Quantum' Instrument for the E-ELT; The E-ELT: A Chance to Measure Cosmic Magnetic Fields; The Experience from VISIR and the Design of an ELT Mid-infrared Instrument; HARMONI: A Narrow Field Near-infrared Integral Field Spectrograph for the E-ELT; Which Synergies Between LBT/LINC Nirvana and Future ELTs?
TMT Science and Instruments
Includes bibliographical references.
The Workshop “Science with the VLT in the ELT Era” held in Garching from 8th to 12th October 2007 was organised by ESO, with support from its Scienti c and Technical Committee, to provide a forum for the astronomical community to debate the long term future of ESO’s Very Large Telescope (VLT) and its interferometric mode (VLTI). In particular it was considered useful for future planning to evaluate how its science use may evolve over the next decade due to competition and/or synergy with new facilities such as ALMA, JWST and, hopefully, at least one next generation 30–40 m extremely large telescope whose acronym appears in the title to symbolise this wider context. These discussions were also held in the fresh light of the Science Vision recently developed within ASTRONET as the rst step towards a 20 year plan for implementing astronomical facilities—the rst such attempt within Europe. Speci c ideas and proposals for new, second generation VLT/I instruments were also solicited following a tradition set by several earlier Workshops held since the start of the VLT development. The programme consisted of invited talks and reviews and contributed talks and posters. Almost all those given are included here although, unfortunately not the several lively but constructive discussion sessions.
Observations, Astronomical.
Astronomy—Observations.
Astrophysics.
Gravitation.
Lasers.
Photonics.
Electronics.
Microelectronics.
Astronomy, Observations and Techniques.
Astrophysics and Astroparticles.
Classical and Quantum Gravitation, Relativity Theory.
Optics, Lasers, Photonics, Optical Devices.
Electronics and Microelectronics, Instrumentation.
Astrophysics and Space Science Proceedings