README web version of /home/usg/OPS/MTS/readme_xml/readme_84078901

Principal Investigator Email Address

• boekel@mpia.de

Estimated Total Execution Time (hours, including overheads)

• 3.3

General Description

• This is the TOO part of our NACO+VISIR monitoring programme of the T Tau
   system,
  aimed particularly at characterizing the (sometimes very fast) photometric variations
  in Sa, the more massive component of the southern close binary. For a more detailed
  description, see the readme of the main monitoring programme (084.C-0783(A+B)).
   
  Here we list only information specific to the TOO part.
  
  The normal monitoring programme consists of "monthly" observations during the whole
   of
  P84, and "weekly" observations during two months (preferably november+december).
   The
  TOO will be triggered in case substantial variations from one week to the next are
  detected in the weekly monitoring period. The TOO comprises even more intensive
  monitoring, with one observation every 1-2 days (do whatever is feasible on the
  mountain, and "every day" is not necessarily better than "every two days"). 
  
  In order for real time assessment of the brightness evolution of Sa, we will suply
  a custom made idl routine which provides brithness estimates of Sa (and Sb) relative
  to the non-variable T Tau N at the push of a button, when supplied with the raw
   NACO
  data. 
  
  Should the TOO be triggered, please stay in close contact with us during this period
  (boekel@mpia.de, ratzka@usm.uni-muenchen.de)
  
  many thanks for your help, we hope you'll have fun executing this programme, and
  that we will detect some nice and fast variations - those are the ones from which
  we learn most!
  
  with best regards, on behalf of the team
  Roy van Boekel
  Thorsten Ratzka

Waiver Requests

• No Waiver Request was submitted

Critical Observing Condition Constraints

• none other than those given in the OBs.

Time-Critical Aspects

• During the optional, intensive monitoring part of the campaign (i.e. this
   TOO programme),
  it is important that the NACO and VISIR observations are done during the same night,
  if at all possible, since we seek to characterize SED variations on time scales
   of days.

Special Execution Requirements

• ---(Empty)---

Special Calibration Information

• ---(Empty)---

ToO Information

• ---(Empty)---

ToO Activators List

• ---(Empty)---

Is this a Pre-imaging run ?

• false

Pre-imaging Requirements

• ---(Empty)---

Source(s) of Pre-imaging

• ---(Empty)---

Pre-imaging sources not listed above

• ---(Empty)---

Do all your OBs comply with the instrument-specific requirements listed
 on the instrument-specific Phase 2 web page ?

• YES

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 ?

• YES

If you submitted OBs for standard stars, did you specify the magnitude
 and spectral type of all standard stars in the OBs ?

• N/A

Have you included OBs for any calibrations that you need but which are
 not part of the Calibration Plan ?

• N/A

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 ?

• N/A

If this is a run that requires coordinated observations with other facilities,
 did you give proper instructions in the Time-Critical Aspects Section ?

• YES

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?

• N/A

Did you specify a guide star brighter than V=12mag within a field of
 r=5arcmin around the science target?

• NO