README web version of /home/usg/OPS/MTS/readme_xml/readme_76011900

Principal Investigator Email Address

• angela.bragaglia@bo.astro.it

Estimated Total Execution Time (hours, including overheads)

• 6:00:03

General Description

• This is a program to derive colour-magnitude diagrams for three open clusters:
   Biu 11, Biu 13, and Ber 36 in decreasing order of importance.
  We require BVI observations (short/medium/long in each filter) for 
  1) a field centered on the cluster (repeated twice, at PA=0 and =90 deg for Biu
   11 and Biu 13, only once with PA=0 for Ber 36); 
  2) one field near to each cluster (at about 30 arcmin, taken only with PA=0 deg).
   
  Magnitudes have to be calibrated to the standard photometric system, so we require
   PHOT conditions.
  We ask to finish with one cluster (central(s)+external field) before beginning with
   the next one, in order of decreasing priority.
  We wish to add to the standard calibration plan another standard area (SA98), that
   has to be taken near our science OB; one area is enough if more than one science
   OB is executed on same night, but we put in enough OBs to cover the possibility
   that only 1 single OB per night is executed.
  All finding charts are 5.5'x5.5

Waiver Requests

• No Waiver Request was submitted

Critical Observing Condition Constraints

• We require photometric conditions

Time-Critical Aspects

• Not applicable

Special Execution Requirements

• We require to finish with one cluster (Biurakan 11 first, then Biurakan
   13, and last Berkeley 36) before beginning with another one.
  Priority:
  1- Biurakan_11_a, Biurakan_11_b, Biurakan_11_EXT (with an extra exposure on SA98
   each separate night)
  2- Biurakan_13_a, Biurakan_13_b, Biurakan_13_EXT (with an extra exposure on SA98
   each separate night)
  3- Berkeley_36, Berkeley_36_EXT (with an extra exposure on SA98 each separate night)

Special Calibration Information

• We wish to add to the standard calibration plan another standard area
   (SA98), that has to be taken near our science OB; one area is enough if more than
   one science OB is executed on same night, but we put in enough OBs to cover the
   possibility that only 1 single OB per night is executed.
  V, B-V for all 7 standard stars in the chosen 5.5'x5.5' field are listed under "user
   comments"

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 ?

• YES

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 ?

• YES

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