README web version of /home/usg/OPS/MTS/readme_xml/readme_79059500
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Our scientific objective is the observation of the inner region of the
proposed TTauri objects with AMBER in order to study disc formation and disc geometry
considering the effects of dust grains in the hottest part of circumstellar discs.
This run consists of 4 OBs, 2 for targets, 2 calibrators.
Waiver Requests
Critical Observing Condition Constraints
It is mandatory to schedule the observations in such a way that the targets
are not closer than 5 degrees, at least. As the visual brightness for the scientific
target HBC 639 (V=14.8) is close to the limit at that Coude Guiding is working,
we recommend to use a larger angular distance 'target-moon' for this target.
Time-Critical Aspects
Special Execution Requirements
The scientific target AS205 is a 1.3''-binary (position angle = 204degrees,
measured from North to East and seen from the bright component). Only the bright
component of the binary should be observed as it is defined in the OBs.
The scientific target HBC639 is a 2.2''-binary (position angle = 150degrees, measured
from North to East and seen from the bright component). The bright component should
be observed.
Special Calibration Information
The calibrators were chosen because of their proximity to the scientific
targets.
Calibrator for AS205A is
HD143033: V=7.12, K=3.05, spect. type: M0III, separation: 6.1degrees, obtained from
CalVin-List
Calibrator for HBC 639 is
HD143900: V=6.23, K=3.11, spect. type: K2/K3III, separation: 5.1degrees, obtained
from CalVin-List
Of course, the Paranal Science Operation Team should have the right to exchange
these suggested calibrators if it is necessary.
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 ?
Last creation of page: Tue Oct 6 15:40:19 2009
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