README web version of /home/usg/OPS/MTS/readme_xml/readme_83059000
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We aim to measure the geometry of the circumstellar material around a
sample of 11 T Tauri and Herbig Ae/Be stars.
Using AMBER's HR-K (for MWC297) and MR-K (for the 9 target stars) and FINITO fringe
tracking, we want to measure the visibility both in the K-band continuum as well
as in the Brackett-Gamma 2.1661 micron emission line.
As DIT, we have specified the recommended value of 0.5s (for MR-K) and 3s (for HR-K).
If necessary, please adjust this value to the given atmospheric conditions and
to the FINITO performance (using the same DIT for the calibrator and science OB).
*** PLEASE NOTE FOR SCI_HD144432:
HD144432 has a faint companion at a separation of 1.4" (PA=4 deg; Delta-V approx.
4.5 mag; Delta-K=3.1 mag; see Carmona et al. 2007, A&A 464, 687). Please center
the AMBER fiber on the brighter/southern component (see also attached high-resolution
finding chart).
*** PLEASE NOTE FOR SCI_MWC863:
MWC863 has a companion at a separation of 1.1" (PA=236 deg; Delta-V approx. 3.4
mag; Delta-K=2.4 mag; see Carmona et al. 2007, A&A 464, 687). Please center
the AMBER fiber on the brighter/north-eastern component (see also attached high-resolution
finding chart).
*** PLEASE NOTE FOR SCI_SCrA:
SCrA has a companion at a separation of 1.4" (PA=157 deg; Delta-V approx. 1.0 mag;
Delta-K=0.7 mag; see Carmona et al. 2007, A&A 464, 687). Please center the
AMBER fiber on the brighter/north-western component (see also attached high-resolution
finding chart).
The calibrators and their characteristics are (UD diameters from ASPRO):
HD 98560, F6IV, UD diameter=0.478 +/- 0.033 mas
HD 142542, F5V, UD diameter=0.378 +/- 0.026 mas
HD 144172, F8, UD diameter=0.331 +/- 0.023 mas
HD 145825, G1V, UD diameter=0.451 +/- 0.031 mas
HD 145921, K2III, UD diameter=0.943 +/- 0.065 mas
HD 153363, F3V, UD diameter=0.478 +/- 0.033 mas
HD 166460, K2III, UD diameter=1.577 +/- 0.109 mas
HD 177565, G8V, UD diameter=0.563 +/- 0.039 mas
HD 179758, G5, UD diameter=0.426 +/- 0.029 mas
HD 187660, K5III, UD diameter=1.865 +/- 0.129 mas
HD 193799, G9III, UD diameter=0.448 +/- 0.031 mas
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Is this a Pre-imaging run ?
Pre-imaging Requirements
Source(s) of Pre-imaging
Pre-imaging sources not listed above
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
If this is a pre-imaging run, did you select PRE-IMAGING for the Observing
Category for each Observing Template ?
Do all your finding charts comply with both the general and instrument-specific
Phase 2 Web Pages ?
If you submitted OBs for standard stars, did you specify the magnitude
and spectral type of all standard stars in the OBs ?
Have you included OBs for any calibrations that you need but which are
not part of the Calibration Plan ?
If you are observing Moving Targets, have you attached suitable ephemeris
files to your OBs?
If you have preferences which OBs should be executed first, did you make
use of the User Priority field in the OBs ?
If this is a run that requires coordinated observations with other facilities,
did you give proper instructions in the Time-Critical Aspects Section ?
Did you indicate for each science star OB the corresponding calibrator
star OB (and vice versa) in the 'Instrument Comments' field ?
Did you check that your chosen calibrator is bright enough for the instrument
mode used ?
If you use calibrator stars which are not in the CalVin database, did
you specify their characteristics in the README file and in the OBs ?
Do you use the same DIT for pairs of science target and associated calibrator?
Are the magnitudes of science target and calibrator within +/- 1 mag
?
Did you verify that your coordinates are as accurate as possible (2Mass
coordinates recommended) and that they include proper motions if available ?
Did you specify the LST range of the calibrators such that they cover
the range from 30 min before the start of the LST range of the science target to
30 min after the end of the LST range of the science target ?
Last creation of page: Tue Oct 6 15:40:30 2009
If you have comments, please contact usd-help@eso.org