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P2PP for Surveys



OVERVIEW


The User Support Department

Observing in Service Mode:
Philosophy and Scheduling

Data Distribution

Run Progress Reports

Frequently Asked Questions

Related Links

Service Mode Questionnaire


PHASE 2 PREPARATION


VLT and ESO-MPI 2.2m
Service Mode Guidelines


Instrument-Specific
Service Mode Instructions:
   AMBER
   CRIRES
   FLAMES
   FORS1/2
   HAWK-I
   ISAAC
   MIDI
   NACO
   SINFONI
   UVES
   VIMOS
   VISIR
   FEROS    WFI

NTT and 3.6m
Service Mode Guidelines


APEX Service Mode preparation

Visitor Mode Phase 2 Guidelines

Special procedures:
   Director's Discretionary Time
   Target of Opportunity
   Rapid Response Mode
   Moving Targets


TOOLS


The P2PP Page

Instrument-Specific
Preparation Software:

   FIMS
   NAOS PS
   FPOSS
   VMMPS
   GUIDECAM

Auxiliary Tools for
Phase 1 and 2 Preparation

   Finding Charts Tool
   Other Tools

 

User Manual and related documents Time-linking of OBs Concatenation of OBs Definition of groups of OBs Import of target fields produced by the Survey Area Definition Tool
P2PP has been in use at ESO telescopes since 1997 and has undergone much evolution since then, trying to adapt to both operational and user-friendliness needs as they have been identified, and providing enhanced functionality.

P2PP development continues, and it is currently focused on specific requirements that are set by the soon to start ESO Public Survey programmes with Survey Telescopes, VST and VISTA, on Paranal. However, most of these new functionalities and enhancements of P2PP will be of use for all Service Mode users of ESO telescopes, including those conducting short programmes. Therefore ESO plans to extend the use of the new P2PP for Surveys also for "normal" programmes on the VLT and other telescopes in the future.

This page provides a quick overview of the enhancements to the functionality of P2PP for Surveys and provides links to the relevant documentation.

P2PP for Surveys User Manual and related documents

The users preparing the observations for Public Survey programmes with VISTA and VST should read the P2PP for Surveys User Manual for a detailed description of the currently available functionalities.

For the preparation of the observations for Public Surveys the users will have to define the survey areas using the Survey Area Definition Tool (SADT). The output of the SADT will then be imported in the new P2PP for Surveys, version 3.1, to prepare valid observing blocks.

Time-linking of OBs

It is frequent that OBs must be executed within precise time windows, rather than any time when the external conditions (moon, seeing, transparency...) would allow the execution. The following types of time-dependencies can be recognized:

  • Absolute time constraints, meaning that an OB must be executed at specific dates that can be predetermined. An example is the observation of a binary star at a precise phase of its period.
  • Relative time links, implying that an OB must be executed within a time interval after the execution of a previous OB, but not necessarily at a fixed date. Examples of this are monitoring observations of a variable source at roughly constant intervals.
Only the first type of time-dependency is implemented in P2PP that is used for service mode programmes on VLT. In the new P2PP for Surveys, the relative time links are implemented within the new "Time Link" container.

Within a Time Link container, the user can define a series of OBs, having the earliest and latest time when a given OB in the series must be executed with respect to the preceding OB. The time-related information is stored in a database, from where it is retrieved by scheduling tools available to the operator on the mountain in order to build up a short-term schedule that properly takes these constraints into account.

Concatenation of OBs

In some cases it may be desired to execute the OBs consecutively, with no other observations in between. This has been implemented in the P2PP for Surveys within the new "Concatenation" container. The concatenation container consists of two or more OBs that must be executed "back-to-back" without breaks. The sequence of the execution of OBs in a concatenation cannot be specified.

Definition of groups of OBs

It is possible at present to assign an execution priority to each OB, so that the operator is aware of the ones that have a higher scientific importance at the time of deciding on observations to execute for a given programme.

It has been recognized nevertheless that such simple priority scheme is sometimes insufficient to deal with programmes containing large number of OBs, and especially for surveys containing large numbers of target fields observed in a number of instrumental setups. In such cases the need for a prioritization scheme above the individual OB level, which can take into account the past execution history of the programme, becomes clear. One can consider for instance the case of a survey of several target fields to be observed through several different filters, with each field and filter specified in a single OBs. Depending on the science goals of the programme it may be desirable to complete the observations of a given field in all filters before proceeding to the next field, or conversely to observe all the fields in a given filter before proceeding to the next filter, or even ensure that contiguous coverage among the fields takes priority.

The approach adopted to deal with such cases is the definition of groups of OBs, in which internal priorities within each group are reflected in the form of a contribution of each OB to the total group score. The short-term scheduling tools available on the mountain will take into account the current scores of each group of OBs, and will then apply a number of rules in order to prioritize the possible OBs to be executed according to them. Such rules will for instance give the highest execution priority to those OBs that set a new maximum of the score among the existing groups; and among those, the highest priority will be given in turn to those that produce the largest increase in group score. By assigning to the OBs the appropriate contributions to the scores of their respective groups, the users can make sure that the progress in the execution of the programme will take place in a way that is consistent with the scientific priorities of the observations. In addition, it will be possible to assign different priorities to each group.

Import of target fields produced by the Survey Area Definition Tool

The Survey Area Definition Tool (SADT) is a utility developed by the VISTA consortium that allows users to define areas to be covered by surveys executed with either VIRCAM at VISTA or OmegaCam at the VST according to a number of criteria. The SADT determines the central coordinates of the different pointings required to cover the field according to the specifications, as well as ancillary guide star information to allow acquisition and guiding. The output produced is a file to be ingested by P2PP containing all the target information needed for the preparation of the OBs with which the survey will be executed.

The latest version of the SADT User Manual is available from the VISTA consortium SADT web page.


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