![]() |
![]() |
||||
---|---|---|---|---|---|
EUROPEAN SOUTHERN OBSERVATORY
|
|||||
|
(P2PP) |
Exposures are defined using templates or Observation Blocks (OBs). An OB is one observation, or group of observation, that constitute a logical entity which should not be interrupted. Typical examples are a UBVRI sequence, a Red and a Blue spectrum, or a sequence of dithered K images.
An OB is constituted by
These OBs are defined in advance, and can be executed in a very flexible way. For instance, some of the templates can be skipped, or the whole OB can be paused between templates.
A number of different OBs are defined, for different kind of observations,
such as, bias, darks, dome flat fields, twilight flat fields or a set of science
exposures. A number of templates can be combined in an observing block, which
is the smallest schedulable entity. Each observing block begins with a telescope
preset to the desired position (acquisition), followed by one or more templates
to be executed at this position. The defined Observation Blocks can be saved
in a local directory ("local cache") from where they can also be recovered for
further editing.
P2PP can be run on the off-line system (on kila, the main server at La Silla), to prepare your OBs before your observing run. P2PP is also run at the telescope for modifying the prepared OBs, or adding some new ones. Your support scientist will assist you with this; the preocedure is outlined in the next paragraph (that you can skip unless you enjoy this kind of reading)
The Login to P2PP window (screen copy) requesting for the log-in user validation: user id and password can be obtained from the observer support. After entering, the login window disappears and the user id appears in the second screen: the P2PP main window (screen copy).The P2PP main window is divided in three sub windows, called Observation Blocks, Observation Descriptions, and Targets. Observation Blocks contains the list of defined observations. Observation Descriptions lists pre-defined instrument configurations, and Targets pre-defined targets; Observation Blocks are generated by combining a predefined target (target package) with an instrument set-up. The top buttons can be used to define new entries in the sub windows.
Before starting to define your OBs, you will have to set the program ID (recover your program number(s) from the [File] [Observing Program] menu), set the Period (small Period window) and select your instrument ([Instrument] button).
Target definition: Under the File button on the P2PP window, open Target definitions. Enter the number of the period and click on Phase I. A list of all targets defined in your original proposal appears. Select one by double-clicking on it. A new window opens showing you the full information for this target. Information can be edited if required (check especially the equinox). Comments can also be entered.
Document | Comments |
![]()
|
Reference document. (Postscript) |
Detailed and complete P2PP Home Page. This is the absolute P2PP reference. | |
![]() |
Include the detailed description of the Observation,
Calibration and Acquisition templates (PostScript). The Observer should get the reference manual for the instrument(s) they plan to use. |
P2PP and OB page, by the ESO/User Support Group |
![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() |