Your Observing Graphic Interface
Your Observing Graphic Interface (YOGI) is a set of front-end graphic
tools developed to make observer's life easier. It consists of packages
enabling telescope control, camera control, data aquisition and data
inspection. The heart of the system is the
Data Base Server - a powerfull
interface between different graphic packages and instrument control programs.
The following tools have been already implemented in the YOGI:
dATAview,
Telescope,
Camera,
Filters,
Map,
Command.
- dATAview
- general image viewing tool
which displays images read from the disk (FITS format),
Shared Memory or delivered by
the Image Server. Images can be viewed in
the three different windows: general view ,
default, large size image and in
zoomed box. Digital details of the images
may be inspected in the graphic window,
which is capable of displaying cuts, histograms, radial profiles,
surface and contour plots as well as showing magnitudes or FWHM of the selected
stars. Grapic window contains telescope focusing tool.
Control window enables rambling or
looping through the series of images and
controls many other features like measuring star magnitudes,
distances, angles, offsetting the telescope, marking frame orientation,
integrating multiple images, masking bad pixels or subtracting sky frames.
- Telescope
tool is a general tool
for positioning and offseting the telescope. Besides the obvious functions like
displaying and entering target coordinates it contains also input coordinates
dials, arrow panel for manual offseting, switch for different offset
coordinate systems,
equinox selector/converter, Cassegrain position input/display, current time
display (UT, siderial, JD). It gives indication whether the
telscope points to the required object, is offseted or is moving (animation).
Telescope tool will show actions started within other tools, e.g.
Map ,
dATAview or
Camera Mosaic .
- Camera
is a dedicated tool for controling
image aquisition instruments. Currently it supports three infrared
instruments:
MAGIC ,
OMEGA
and
MAX ,
but could be easily adapted for any other imaging or spectroscopic
system based on IR arrays or CCD detectors. Camera tool
controls mainly specific camera functions: readout modes, exposure
time, number of exposures, but also data managing (entering comments,
object names), data saving (paths, filenames, disk-space),
macro and mosaicing capabilities (generating, recording, replaying, pausing).
- filters
tool controls filter selection. It is separated from the
Camera tool for more flexibility. Wheels
supports any number of wheels with any nuber of positions -
configurable on fly with the Data Base.
Wheels tool serves both as an input (pull-down menu or graphic) and status
display (with animation).
- Map is a multipurpose tool
which serves as a sky atlas, SAO catalogue and IRAS catalogue. It also
displays objects from one of many user catalogues. Sky map can be zoomed
and telescope position is always marked on the display.
To move the telescope to the new position it is enough to select an
object on the map (or in the text window in case of user objects) and
press MOVE button.
Map tool may show also airmass window telling
the observer whether the selected object is high enough to be observed.
Map displays locations of the images taken during the current session, which is
especially usefull when creating time consuming mosaics.
Spectral types of the stars could be visualised with different colors - feature
usefull when one needs to find appropriate check star.
- Command tool is intended
for users that prefer keyboard rather than mouse input. Nice feature of the
commant tool it is history buffer (scrollable window) allowing one for
reselecting previously issued commands. Command tool is usable only for the
systems which have command language layer behind the Graphic Interface.
However this is the case for the Omega/Magic/Max system.
In addition there are three "windowless" components of the system:
- Data Base Server
- the heart (or rather brain) of the system, which interfaces graphic modules
to the command language layer. Data Base Server may run remotely, what
enables (in theory) remote graphic instrument control.
- Image Server which
is capable to deliver images over the net to the remote
dATAview tool.
During remote operation graphic tools are executed on the remote machines
and only vital data are send over the net. However if the is was too slow,
then remote operation may not work properly.
- Command Server which acts
as an interface between the Data Base Server
and the command language layer controling instrumentation.
Click button to see how the system might look on your screen:
(58 kB)
(18 kB)
You may now slect to go to Tutorial or
Frequently Ask Questions or
Feedback or
Technical Refernce Manual.
Grzegorz Pojmanski /
gp@sirius.astrouw.edu.pl