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P2PP for Surveys | |||||
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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 documentsThe 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 OBsIt 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:
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 OBsIn 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 OBsIt 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 ToolThe 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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