E-Book, Englisch, 402 Seiten
Kissler-Patig / Walsh Science Perspectives for 3D Spectroscopy
1. Auflage 2007
ISBN: 978-3-540-73491-8
Verlag: Springer-Verlag
Format: PDF
Kopierschutz: Wasserzeichen (»Systemvoraussetzungen)
Proceedings of the ESO Workshop held in Garching, Germany, 10-14 October 2005
E-Book, Englisch, 402 Seiten
ISBN: 978-3-540-73491-8
Verlag: Springer-Verlag
Format: PDF
Kopierschutz: Wasserzeichen (»Systemvoraussetzungen)
This volume contains the proceedings of possibly the last conference ever on integral-field spectroscopy. The contributors, noted authorities in the field, focus on the scientific questions that can be answered with integral-field spectroscopy, ranging from solar system studies all the way to high redshift surveys. Overall readers get a state-of-the-science review of astronomical 3D spectroscopy.
Autoren/Hrsg.
Weitere Infos & Material
1;Preface;5
2;Contents;7
3;List of Contributors;14
4;3D Instrumentation;18
4.1;3D Instrumentation;19
4.2;3D-NTT: A New Instrument for the NTT Based on Versatile Tunable Filter Technology;30
4.3;The Integral Field Unit of the Near Infrared Spectrograph for JWST;36
4.4;Scientific Prospects of the 3D-NTT Instrument;42
4.5;Handling IFU Datasets in the Virtual Observatory;44
4.6;Simulations of High- z Starburst Galaxies for the JWST- MIRI Integral Field Unit;47
4.7;IFUs: Disentangling the Light from Neighbour Fibers;51
4.8;OSIRIS – a New Integral-Field Spectrograph at Keck Observatory;54
4.9;A User–oriented Comparison of the Techniques for 3D Spectroscopy;57
5;Solar System(s);62
5.1;The Potential of Integral Field Spectroscopy Observing Extrasolar Planet Transits;63
5.2;Solar System Objects with the NACO Fabry- Perot and SINFONI;73
5.3;3D Spectroscopy with an Imaging FTS;83
6;Nearby Galaxies;90
6.1;Nearby Galaxies: 3D Spectroscopy as a Tool, not as a Goal;91
6.2;Nearby Galaxies Observed with the Kyoto Tridimensional Spectrograph II;101
6.3;Scalable N-body Code for the Modeling of Early- type Galaxies;107
6.4;Internal Kinematics of Galaxies: 3D Spectroscopy on Russian 6m Telescope;112
6.5;SAURON Observations of Sa Bulges: The Formation of a Kinematically Decoupled Core in NGC5953;118
6.6;Characterizing Stellar Populations in Spiral Disks;123
6.7;The Stellar Populations of E and S0 Galaxies as Seen with SAURON;129
6.8;VIMOS-IFU Spectroscopy of Extragalactic Star Forming Complexes;135
6.9;Analyzing Non-circular Motions in Spiral Galaxies Through 3D Spectroscopy;140
6.10;Harmonic Analysis of the Ha Velocity Field of NGC 4254;145
6.11;The NIR Tully-Fisher Relation in Different Environments: the Importance of 3D Observations;148
6.12;3D Kinematics of Local Galaxies and Fabry- Perot Database;151
6.13;Validation of Stellar Population and Kinematical Analysis of Galaxies;154
6.14;Non-Gravitational Motions in Galaxies;157
6.15;Studying the Roots of the Supergalactic Wind in NGC 1569 with Gemini GMOS/ IFU;159
7;Lensing Studies;163
7.1;Gravitational Lensing Studied with Integral Field Spectroscopy;164
7.2;3D Spectroscopy as a Tool for Investigation of the BLR of Lensed QSOs;174
7.3;A VIMOS-IFU Survey of z ~ 0.2 Massive Lensing Galaxy Clusters: Constraining Cosmography;179
7.4;First Results from the VIMOS-IFU Survey of Gravitationally Lensing Clusters at z ~ 0.2;185
7.5;Integral Field Spectroscopy of the Core of Abell 2218;191
8;Intermediate z Galaxies;197
8.1;Velocity Fields of z~ 0.6 Galaxies with GIRAFFE and Perspectives for ELTs;198
8.2;News from the Dentist’s Chair : Observations of AM1353- 272 with the VIMOS IFU;204
8.3;3D Spectroscopy of Low- z (Ultra)Luminous Infrared Galaxies;209
8.4;Optical Spectra in the Non-Nuclear Regions of ULIRGs: Evidence of Ionization by Shocks;217
9;Centres of Galaxies;222
9.1;Stellar Populations in the Galactic Center with SINFONI;223
9.2;Stellar Populations in the Centers of Nearby Disk Galaxies;228
9.3;AGN Shocks in 3D;234
9.4;Young Kinematically Decoupled Components in Early- Type Galaxies;245
9.5;SINFONI’s take on Star Formation, Molecular Gas, and Black Hole Masses in AGN;250
9.6;The Unified Model in Nearby Seyfert Galaxies Through Integral Field Spectroscopy;255
9.7;A 3D View of the Central Kiloparsec of the Seyfert Galaxy NGC 1358;258
9.8;VLT/SINFONI Integral Field Spectroscopy of the Superantennae;261
9.9;Integral-Field Observations of Centaurus A Nucleus;264
9.10;The Puzzling Case of XBONGs: Will 3D- spectroscopy Explain Their True Nature?;267
9.11;Studying of Some Seyfert Galaxies by Means of Panoramic Spectroscopy;271
10;Emission Nebulae and resolved Populations;274
10.1;3D Spectroscopy of Emission Nebulae;275
10.2;GMOS-IFU Observations of LV2;286
10.3;The Enigma of Ultraluminous X-ray Sources may be Resolved by 3D- Spectroscopy ( MPFS Data);291
10.4;Spatially Resolved Spectroscopy of Abell 30;296
10.5;Constraining the Galactic Structure with Stellar Clusters in Obscured Hii Regions;301
10.6;Integral Field Spectroscopy of a Peculiar Supernova Remnant MF16 in NGC6946;307
10.7;SN 1987A: A Complex Physical Laboratory;312
10.8;3D-Spectroscopy of Extragalactic Planetary Nebulae as Diagnostic Probes for Galaxy Evolution;317
10.9;3D Spectroscopy of Herbig-Haro Objects;321
10.10;High Mass Star Formation in the Light of SINFONI;324
10.11;Internal Kinematics of IIZw40;327
10.12;Integral Field Spectroscopy Survey of Classical LBV Stars in M33;330
10.13;Unravelling the Chemical Inhomogeneity of Planetary Nebulae with VLT FLAMES;333
11;Extended Emission Line Regions;337
11.1;Integral Field Spectroscopy of Galaxy Emission Line Haloes;338
12;The High Redshift Universe;344
12.1;Integral Field Spectroscopy of Galaxies in the Distant Universe;345
12.2;Integral-Field Studies of the High-Redshift Universe;352
12.3;3D Kinematics of High-z Galaxies as Seen Through the Gravitational Telescope;357
12.4;AGN Feedback at High Redshift: Shaping the Most Massive Galaxies?;362
12.5;Integral Field Observations of a Distant Cluster;365




