Principal Investigator Email Address
acarmona@eso.org
Estimated Total Execution Time (hours, including overheads)
44.0h
General Description
HR spectroscopy of eigth disks around young stellar objects and two PDR's in the 12.27 micron H2 0-0 S(2) and 17.03 micron H2 0-0 S(1) line. The targets are expected to be point-sources in the acquisition images (exception Orion Bar); in all cases they are the brightest mid-infrared source within the FOV of VISIR.
Waiver Requests
A waiver request for OB duration > 1 hour was approved for this run.
Critical Observing Condition Constraints
Observations of the 12.27 micron H2 0-0 S2 line should be executed preferently with low relative humidity (< 10%)
Time-Critical Aspects
Observations of the 12.27 micron H2 0-0 S2 line should be executed preferentially on the dates mentioned below. The 12.27 lies very close to an atmospheric water line. The velocity shift should be the maximun possible for increase the probability of detection. OBJECT DATE UXOri before 30 Oct 2005 OR after 5 Jan 2006 HD34282 before 30 Oct 2005 OR after 5 Jan 2006 OrionBar before 30 Oct 2005 OR after 5 Jan 2006 NGC2023 before 30 Oct 2005 OR after 5 Jan 2006 HD100453 after 5 Dec 2005 HD104237 before 30 Sep 2005 OR after 15 Jan 2006 HD141569 before 5 Oct 2005 OR after 10 Dec 2005 HD142666 after 5 Jan 2006 HD143006 before 5 Oct 2005 OR after 10 Dec 2005 HD319139 after 5 Jan 2006
Special Execution Requirements
Special Calibration Information
We have supplied OBs for telluric standards in HRX mode with central wavelength 12.2786 microns. They should be observed preceding and following the respective science science OB: CAL_UXOri_H2S2_P is to be observed on the same night preceding the OB UXOri_H2S2 CAL_UXOri_H2S2_F is to be observed on the same night following the OB UXOri_H2S2 CAL_HD34282_H2S2_P is to be observed on the same night preceding the OB HD34282_H2S2 CAL_HD34282_H2S2_F is to be observed on the same night following the OB HD34282_H2S2 CAL_OrionBar_H2S2_P is to be observed on the same night preceding the OB OrionBar_H2S2 CAL_OrionBar_H2S2_F is to be observed on the same night following the OB OrionBar_H2S2 CAL_NGC2023_H2S2_P is to be observed on the same night preceding the OB NGC2023_H2S2 CAL_NGC2023_H2S2_F is to be observed on the same night following the OB NGC2023_H2S2 CAL_HD100453_H2S2_P is to be observed on the same night preceding the OB HD100453_H2S2 CAL_HD100453_H2S2_F is to be observed on the same night following the OB HD100453_H2S2 CAL_HD104237_H2S2_P is to be observed on the same night preceding the OB HD104237_H2S2 CAL_HD104237_H2S2_F is to be observed on the same night following the OB HD104237_H2S2 CAL_HD141569_H2S2_P is to be observed on the same night preceding the OB HD141569_H2S2 CAL_HD141569_H2S2_F is to be observed on the same night following the OB HD141569_H2S2 CAL_HD142666_H2S2_P is to be observed on the same night preceding the OB HD142666_H2S2 CAL_HD142666_H2S2_F is to be observed on the same night following the OB HD142666_H2S2 CAL_HD143006_H2S2_P is to be observed on the same night preceding the OB HD143006_H2S2 CAL_HD143006_H2S2_F is to be observed on the same night following the OB HD143006_H2S2 CAL_HD319139_H2S2_P is to be observed on the same night preceding the OB HD319139_H2S2 CAL_HD319139_H2S2_F is to be observed on the same night following the OB HD319139_H2S2 We have supplied OBs for telluric standards in HR mode with central wavelength 17.0348 microns: CAL_UXOri_H2S1 is to be observed on the same night as the OB UXOri_H2S1 CAL_HD34282_H2S1 is to be observed on the same night as the OB HD34282_H2S1 CAL_OrionBar_H2S1 is to be observed on the same night as the OB OrionBar_H2S1 CAL_NGC2023_H2S1 is to be observed on the same night as the OB NGC2023_H2S1 CAL_HD100453_H2S1 is to be observed on the same night as the OB HD100453_H2S1 CAL_HD104237_H2S1 is to be observed on the same night as the OB HD104237_H2S1 CAL_HD141569_H2S1 is to be observed on the same night as the OB HD141569_H2S1 CAL_HD142666_H2S1 is to be observed on the same night as the OB HD142666_H2S1 CAL_HD143006_H2S1 is to be observed on the same night as the OB HD143006_H2S1 CAL_HD319139_H2S1 is to be observed on the same night as the OB HD319139_H2S1
ToO Information
ToO Activators List
Is this a Pre-imaging run ?
false
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 ?
N/A
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?
N/A
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 ?
N/A
If the provided finding chart is at a different wavelength than the observations, did you clearly describe in the README file how to identify the target?
Did you specify a guide star brighter than V=12mag within a field of r=5arcmin around the science target?