README web version of /home/usg/OPS/MTS/readme_xml/readme_77023501
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The aim of our proposal is to obtain the series
of surface temperature maps from line profile variations
for LQ Hya (a young single K2 dwarf with extreme
photospheric and chromospheric activity) with time resolution
comparable with a few rotational periods of the star and for the first time
to trace the rapid evolution of spots configuration
continiously during several months.
We ask for 14 min exposure observations with FEROS
during 5 consequative nights each month - one block, every month
in the period from April, 2006 to July, 2006.
We ask for 4 blocks of observations:
1-5 April, 1-5 May, 1-5 June and 1-5 of July (one spectra per night).
Observations in April-July, 2006 should be obtained during the
first half of the night (evening hours are possible).
Waiver Requests
Date: Tue, 31 Jan 2006 16:49:39 +0100
From: Fernando Comeron
To: isavanov@aip.de
Cc: fcomeron@eso.org
Subject: your waiver request for run 077.D-0235(B)
Dear Dr. Savanov,
I am pleased to let you know that the waiver request regarding the
non-submission of finding charts is accepted.
Best regards,
Fernando Comeron
ESO User Support Department
Critical Observing Condition Constraints
We ask for 14 min exposure observations with FEROS
during 5 consequative nights
each month - one block, every month
in the period from April, 2006 to July, 2006.
We ask for 4 blocks of observations:
1-5 April, 1-5 May, 1-5 June and 1-5 of July (one spectra per night).
Observations in April-July, 2006 should be obtained during the
first half of the night (evening hours are possible).
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 set 'New Preset' flag in all acquisition templates to 'True'?
If you use any lamp, did you check that it should never be left on at
the end of any OB?
Last creation of page: Tue Oct 6 15:40:12 2009
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