084.C-1063(A)

  

PI:Kraus/ Driebe/ Hofmann/ Schertl/ Weigelt

  
* Rank Class: B  

AMBER

Last update of this page: Wed Oct 7 15:41:08 2009

 
 
0 done (of 9 OBs)
0.00 hrs done (of 4.50 hrs)

Remaining + and M OBs for this run:
(Explanation of table contents)
PHOT CLR THN THK Seeing &
Airmass
Constraints:
--
9 OB(s) 		-- -- Seeing < 1.00
Airmass < 5.00

USD Review Status:
OK, accepted

Pre-Imaging?Special-Calibration?Time-Critical?Programme TypeCarry-Over?Chilean?
 

Special Remarks:
Abstract for MTS:
VLTI/UT AMBER observations in LR mode *without* Finito of the Herbig Be star HD98922. These observations complement earlier observations of this target with the goal to create an image (using the old and the new uv points). Run A: 3 observations with E0-G0-H0 Run B: 3 observations with D0-H0-K0 Run C: 5 observations with D0-H0-G1 Run D: 5 observations with A0-K0-G1 The observations are below the limiting magnitude from the AMBER table for the specified seeing, but a waiver has been granted to execute the observations. Longer than usual coherence time might help. There is a main calibrator (HD 104646) and an alternative calibrator (HD97595). The sequence is the standard sci/cal sequence.

Run status page 084.C-1063A

Approved README of this run:

  • Web version of approved README readme_84106300.html

    Check which ftp directories exist for this run:

    Finding charts are attached to the following OBs of this run:
    OB_IDOB_name Finding chart
    OB:387720 SCI_HD98922-A3 HD98922.jpg
    OB:387718 CAL_HD104646-A3 HD104646.jpg
    OB:387721 CAL_HD97595-A3 HD97595.jpg
    OB:387723 CAL_HD97595-A2 HD97595.jpg
    OB:387724 SCI_HD98922-A2 HD98922.jpg
    OB:387725 CAL_HD104646-A2 HD104646.jpg
    OB:387726 CAL_HD104646-A1 HD104646.jpg
    OB:386890 SCI_HD98922-A1 HD98922.jpg
    OB:387727 CAL_HD97595-A1 HD97595.jpg

    Ephemeris file attached to the following OBs of this run:
    OB_IDOB_name Ephemeris file

    USD tickets related to this run:
    USD-EntryId
    ProgId    		SenderEmail TimeStamps Ticket Status Short Problem Description