<?xml version="1.0"?>
<!DOCTYPE RTML SYSTEM "http://www.astro.livjm.ac.uk/HaGS/rtml2.1.dtd" >
<RTML version="2.1" type="score">
<Contact PI="true">
<User>
je
</User>
<Name>
Jason Etherton
</Name>
<Institution>
Liverpool John Moores University
</Institution>
<Address>
Astrophysics Research Institute
Twelve Quays house
Egerton Wharf
Birkenhead
CH41 1LD
</Address>
<Telephone>
+44 (0) 151 231 2903
</Telephone>
<Fax>
+44 (0) 151 231 2921
</Fax>
<Email>
je@astro.livjm.ac.uk
</Email>
<Url>
http://www.astro.livjm.ac.uk
</Url>
</Contact>
<Project>
<Title>
Demonstration RTML document.
</Title>
<Abstract>
This project is designed to test the RTML parsing modules.
</Abstract>
This document specifies ALL the information that will be required
by a Discovery Node to SCORE an observation request.
</Project>
<Telescope region="optical" alias="LT">
The Telescope is defined to specify a telescope to observe with.
There is no need to define the Aperture, FocalLength, FocalRatio etc as
the specific Telescope has this data.
If partial Telescope details are defined, whilst the Name is not, then
any Telescope satisfying the criteria can be used.
Also, specifying a Telescope renders the Location data redundent.
Both have been completely filled in for completeness.
<Name>
Liverpool Telescope
</Name>
It is doubtful that the following will be filled by the Astronomer as
the specification of a telescope will determine all data below.
<Aperture units="meters">
2.0
</Aperture>
<EffectiveAperture units="meters">
1.8
</EffectiveAperture>
<FocalLength units="metres">
20.0
</FocalLength>
<FocalRatio units="metres">
f/10
</FocalRatio>
<PlateScale units="arcsec/mm">
10.0
</PlateScale>
</Telescope>
<Location>
The Location is defined to specify a site to observe from. Again, if a
Telescope has been specified this will be filled on return, otherwise
the observatory site will be specified.
<Name>
Roque de los Muchachos.
</Name>
<Longitude format="sddd mm ss E" units="dms">
-017 52 54 E
</Longitude>
<Latitude format="sdd mm ss" unit="dms">
+28 45 36
</Latitude>
<Altitude units="metres">
2395
</Altitude>
</Location>
<Observation status="ok">
This is the 1st Observation request.
<Score>
0.833
</Score>
<CompletionTime>
12:34T31/01/2002
</CompletionTime>
<Target type="normal" ident="Observation">
This is the 1st observation Target.
The Target attribute ident should be filled in by the Telescope.
e.g. Target ident="LT00001"
<TargetName>
NGC 1234
</TargetName>
<Coordinates type="equatorial">
<RightAscension format="hh mm ss.s" units="hms">
12 34 56.7
<ProperMotion format="ss.s" angleUnits="sec" timeUnits="yr"
useEpoch="true">
01.1
</ProperMotion>
</RightAscension>
<Declination format="sdd mm ss.s" units="dms">
+12 34 56.7
<ProperMotion format="ss.s" angleUnits="arcsec"
timeUnits="yr" useEpoch="true">
02.2
</ProperMotion>
</Declination>
<Equinox>
J2000
</Equinox>
<Epoch>
2000.0
</Epoch>
</Coordinates>
<Parallax>
0.72
</Parallax>
<RadialVelocity type="LSR" units="km/s">
-22.0
</RadialVelocity>
<Flux type="continuum" wavelength="6563" units="mag">
18.8
</Flux>
<TrackRate type="sidereal" />
<Device name="RATCAM" region="optical" type="camera">
LT RATCAM
<Filter>
<FilterType>R-Johnson</FilterType>
</Filter>
</Device>
</Target>
Calcuate the minimum exposure time needed to obtain the Signal-to-Noise
ratio.
<Schedule priority="3">
No binning.
<Exposure type="snr">
5.0
</Exposure>
<ExposureFactor>
0.0
</ExposureFactor>
<SeeingConstraint nominal="1.0" maximum="2.0">
Need at least 2.0 arcsec seeing for this!
</SeeingConstraint>
Sky must be NO brighter than 0.2 mags in the R-band.
<SkyConstraint sky="dark" value="0.2" units="R-mag" />
Moon must be no fuller than 10%, and at least 30 degrees from the
target.
<MoonConstraint maxPhase="0.1" distance="30.0" units="degs"/>
The night MUST be photometric.
<ExtinctionConstraint magnitudes="0.0" clouds="clear" />
The target MUST be observed at ZD less than 60 degrees.
<AirmassConstraint minimum="2.0" />
Take observation between 31st Oct 2001 and 30th Nov 2001.
<TimeConstraint>
<StartDateTime>
2001.10.31T23:00:00
</StartDateTime>
<EndDateTime>
2001.11.30T23:00:00
</EndDateTime>
</TimeConstraint>
Time varying target.
<PhaseConstraint>
Object has phase = 0.0 @ MJD 501029
Object has period = 124.5 hours
Only interested in observing phase transition
<PhaseTime units="MJD">501029</PhaseTime>
<PhasePeriod units="hours">124.5</PhasePeriod>
<StartPhase>-0.05</StartPhase>
<EndPhase>0.05</EndPhase>
</PhaseConstraint>
</Schedule>
<Calibration>
Bias is the frame used to de-bias, and will be filled in after the
correction. The `number' attribute will be filled in unless
specified.
<Bias correct="true" overscan="true" mean="true" />
The Dark current correction will also be filled in after the
correction is performed. The `number' attribute will be filled in
unless specified.
<DarkCurrent correct="true" />
Bad pixels will be corrected for. The returned data is the URL
of the frame showing the bad pixels.
<BadPixels correct="true" />
Correct by flat fielding using either dome- or sky-flats. Again the
data is filled on return with the correction frame and number.
<FlatField correct="true" sky="true" dome="true" />
Putting "true" to a correction will only ask for it. If the
correction is not available it will be reset to "false".
<Fringing correct="true" />
Remove cosmic rays.
<CosmicRays correct="true" />
</Calibration>
<Telemetry>
This will be filled in on completion of the observation.
</Telemetry>
<ImageData type="FITS16" compressed="gzip" delivery="ftp">
Possibly the URL of the reduced data file.
</ImageData>
<Reduction>
Create an object list of the 5 brightest stars within 20 arceseconds
of the target
<Magnitude maximum="maximum" />
<Position radius="20" units="arcsec" />
<ObjectList number="5" />
</Reduction>
</Observation>
</RTML>