EAS Publications Series
Volume 6 (2003)
Observing with the VLTI
Les Houches, France, February 3-8, 2002G. Perrin and F. Malbet (Eds.)
ISBN: 2-86883-652-6
An introduction to interferometry p. 3
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An introduction to visibility modeling p. 23
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Introduction to the observing preparation tool ASPRO p. 35
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Exercise #1 Modeling an astrophysical source in preparation for interferometric observations p. 43
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Practical considerations in ground-based optical/infrared interferometry p. 49
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Observability and UV coverage p. 69
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Exercise #2 Observability and UV coverage p. 79
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The VLTI and its Subsystems p. 91
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The near infrared VLTI instrument AMBER p. 111
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MIDI, the 10 μm interferometer of the VLT p. 127
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Exercise #3 Signal-to-noise calculations with the AMBER & MIDI instruments p. 145
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Finding Calibrator Stars for Optical Interferometry Visibility Measurements p. 151
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Exercise #4 Search for calibration sources p. 161
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VLTI Observing Preparation Sequence p. 163
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Exercise #5 Observing program preparation p. 177
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From Visibilities to Science with Simple Models p. 181
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Interferometric observations of protoplanetary disks p. 191
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Spectral Observations of Envelopes around Stars in Late Stages of Stellar Evolution p. 203
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Astrophysics with Closure Phases p. 213
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Stellar surface imaging using closure phase p. 227
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Science with differential phases p. 237
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Binary Stars with Component Disks: The Case of Z CMa p. 249
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VLTI/MIDI observations of the circumstellar shell of an AGB star: W Hydrae p. 253
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The circumstellar disk of the Be star 28 (ω) CMa p. 257
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Reaching the jet engine with AMBER/VLTI p. 261
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Calibrating the Cepheid Period-Luminosity relation with the VLTI p. 265
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Spectral investigation of new candidates to lambda Bootis type stars p. 271
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Interacting binaries and extrasolar planets: Challenges for VLTI p. 273
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The Multi-wavelength Study of two Unique radio galaxies p. 279
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Spin-Orbital Evolution of Exoplanets p. 281
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Brown Dwarf Disks - A Challenge for MIDI p. 285
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Subdwarf B stars in HW Vir systems p. 287
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The Arches Mass Function p. 289
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Globular Clusters as they can be seen in Ly-alpha and H-alpha at z>1 p. 291
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Warm Debris Disks: Where Is Their Dust and Why? p. 293
Published online: 31 January 2003