AMBER+FINITO+UTs Science Verification
The Science Verification (SV) of AMBER+FINITO+UTs is carried out following the same guidelines applied to all VLT instruments and summarised in the VLT Science Verification Policy and Procedures document.
The AMBER+FINITO+UTs SV run took place on 13-15 October, 2008.
The AMBER+FINITO+UTs SV Team is chaired by J. Melnick and includes the following team members: C. Hummel (DMO), J.B. Le Bouquin (LSPO), I. Percheron (DMO), Stan Stefl (LSPO), M. Wittkowski (DMO).
Useful Links
- AMBER instrument pages
- FINITO page
- (Historic) Call for Science Verification Proposals with AMBER+FINITO+UT1,UT2,UT4
AMBER Science Verification Observing Runs
Science verification raw data are available through the ESO archive. Links are provided below to download the data (when available).
- Weigelt et al.: Resolving the cores of nearby AGN and
Wittkowski et al.: Investigating the near-infrared cores of bright AGN
Programme ID is: 60.A-9053(W). No scientifically useful data obtained. - Sana and Le Bouquin: Absolute mass determination of Massive Stars
Programme ID is: 60.A-9053(S). No scientifically useful data obtained. - Kraus et al.: Studying the gas kinematics in the accretion and outflow-launching region of YSOs and
Tatulli et al.: A unique view of the gas+dust inner environment of the Herbig Be star HD50138
Programme ID is: 60.A-9053(K). No scientifically useful data obtained. - Kraus et al.: Resolving the magnetic wind confinement region of the Orion Trapezium star theta1 Ori C
Programme ID is: 60.A-9053(E). The raw data (science target only) can be downloaded. - Nisini et al.: Investigating the gas emission regions of the T Tauri system GW Ori and
Patience et al.: Resolving Circumbinary disks
Programme ID is: 60.A-9053(N). No scientifically useful data obtained. - Merand and Gallene: First measurement of a Long Period Cepheid's Dynamical Mass
Programme ID is: 60.A-9053(A). The raw data can be downloaded. - Hummel and Peterson: Triple star Sigma Orionis: a Helium rich star in Orion
Programme ID is: 60.A-9053(H). The raw data can be downloaded. - Wittkowski et al.: The mass-loss envelopes of dusty post-AGB stars
Programme ID is: 60.A-9053(I). No scientifically useful data obtained. - Melnick and Kaufer: Are all LBVs fast rotators?
Programme ID is: 60.A-9053(M). No scientifically useful data obtained. - Zinnecker et al.: A Sharp View on the Tip of Orion's Sword - The distance to iota Ori
Programme ID is: 60.A-9053(Z). The raw data can be downloaded. - Moreira et al.: Sizing red giants with AMBER, asteroseismic modelling of COROT data
Programme ID is: 60.A-9053(O).The raw data can be downloaded. - Gil et al.: How many of the RV-detected exoplanets are tuly planetary ? Using AMBER+FINITO+UTs to determine the true mass of these companions
Programme ID is: 60.A-9053(G). The raw data can be downloaded. - Chesneau et al.: Wind stratification and perturbations of the prototype WN star WR 6
Programme ID is: 60.A-9053(C). No scientifically useful data obtained. - Hummel and Elias II: The origin of radio flares in the RS CVn star UX Arietis
Programme ID is: 60.A-9053(B). The raw data can be downloaded. - Le Bouqin et al.: Density wave in circumstellar disks of Be stars
Programme ID is: 60.A-9053(L). No scientifically useful data obtained. - Driebe et al.: Probing the Brgamma-emitting wind region around the massive hypergiant IRC+10420 with VLTI/AMBER in high-spectral resolution mode
Programme ID is: 60.A-9053(D). The raw data can be downloaded. - Wittkowski and Karovicova: High S/N measurement of the molecular layers of a Mira stars
Programme ID is: 60.A-9053(F). The raw data can be downloaded.
Nightlog information and calibration data:
- Nightlog from Oct 13 -> 14
- Nightlog from Oct 14 -> 15
- Nightlog from Oct 15 -> 16
- Calibration star data in LR mode
- Calibration star data in MR 2.1 mode
- Calibration star data in MR 2.3 mode
- Calibration star data in HR 2.172 mode
- P2VM data in LR mode
- P2VM data in MR 2.1 mode
- P2VM data in MR 2.3 mode
- P2VM data in HR 2.172 mode