Foreword: the RC80 telescope is controlled via CCDSH. As for another telescopes, CCDSH provides the frontend to the telscope and its instruments while customized modules are available for specific functionality regarding to this particular telescope.
Please read this manual before using the telescope, either in an interactive way or via the scheduler. This manual is acceptable both for the Piszkéstető site and for the Baja site. Differences are only minor, important differences are highlighted.
Before observations
Login to the computer m51.konkoly.hu
or bartobs.bajaobs.hu
with your own account and start the CCDSH frontend using the the command ccdsh
. Normally, the CCD>
prompt should pop up within a second without any warnings or errors. If another user is using the telescope, the system would be locked via one of the logger modules and an error is reported. In this case, CCDSH would not start at all.
Initialization
Load the RC80-specific initialization script: CCD> source /usr/local/ccdsh/scripts/load-asa.ccdsh
. Besides the essential backends, this command also loads and defines the camera and filter wheel modules. Filters are defined as follows:
define filter 1 u Sloan_u define filter 2 B Bessel_B define filter 3 g Sloan_g define filter 4 V Bessel_V define filter 5 r Sloan_r define filter 6 i Sloan_i define filter 7 z Sloan_z
Comment: Unlike on other telescope at Piszkéstető, this script also loads the module which communicates with the TCS. Thus, nothing will work without this step.
The fine-tunings of the alt-azimuth mount ASA800 telescope can be controlled via the asa
command. Use the CCD> asa --help
command to see the command options:
Usage: asa [-h|--help] <command> [...] status slew taudec <hour_angle>,<declination> slew radec <right_ascension>,<declination> cover {upper|lower} {open|close|stop} rotator auto|<rotator_angle> Internal commands - use when you know what are you doing: force respawn
Preparations: opening the telescope covers and dome slit
Open the telscope covers and the dome slit using the following steps:
- Open the dome slit door:
CCD> set dome slit open
. Note: currently, this command is not acceptable for the Baja site. - Open the telescope covers:
CCD> asa cover upper open
,CCD> asa cover lower open
.
- Warning: Open the upper cover first! Check
asa status
before opening the lower one! These covers open/close fully within ~5 seconds.
- Switch off the IR light of the interior dome cameras, i.e. the Piszkéstető camera or Baja camera:
CCD> set dome light 2 off
.
Preparations: automatic derotation and automatic dome tracking
Initialize the automatic modes as follows:
- Set the rotator on auto:
CCD> asa rotator auto
. Currently there is no home position for the derotator.CCD> asa rotator 213.1
(Piszkéstető) orCCD> asa rotator 160.6
(Baja) can be used as a "home position". This is the standard position of the derotator (i.e., whenasa rotator
is onauto
) when the telescope is looking at the meridian, providing images with the normal view orientation (north is up, west is to the right, etc.). - Set the dome on auto (the dome will follow the telescope):
CCD> set dome auto on
. This command is/can be ignored at the Baja site
Note: all of the three main "moving parts" of the whole telescope system (i.e. the telecope mount, the derotator and the dome) starts to move their intended position once the telescope is commanded to slew.
Checking the system
Use the CCD> asa status
to check telescope status. The output should be something like this:
ASA_mount: sidereal_time: 289.11738 ASA_mount: number_of_controlled_axes: 2 ASA_mount: right_ascension: 289.08803 ASA_mount: declination: 12.96731 ASA_mount: azimuth: 0.04978 ASA_mount: altitude: 55.04869 ASA_mount: is_slewing: 0 ASA_mount: is_tracking: 0 ASA_mount: is initializing: 0 ASA_mount: are_motors_started: 0 ASA_ACC: focuser: position: 7.94 ASA_ACC: derotator: angle: 213.072 ASA_ACC: cover: upper: position: 0.0 ASA_ACC: cover: lower: position: 0.2 MOD_ASA800: auto_derotation: 0 MOD_ASA800: auto_dome_azimuth: 0
If covers are opened properly, the positions are around 87...90 degrees:
ASA_ACC: cover: upper: position: 88.0 ASA_ACC: cover: lower: position: 87.7
Some notes:
- The
are_motors_started
line corresponds to the presence of the hold current on the stepper/servo motors and does not relate to any particular movement. Use theis_slewing
andis_tracking
to check whether is there any motion, or compare subsequent values ofazimuth
andaltitude
accordingly. - These lists above might be extended in the future. The outputs are intended to be both machine-readable and human-readable (i.e. easy-to-interpret).
Slewing
Slewing can be done with CCD> slew ra=hh:mm:ss dec=+-dd:mm:ss
, or in a fixed coordinate system (i.e., 1st equatorial), asa slew taudec tau_value,dec_value
, where the values are decimal. Like in all of the CCDSH-based environments, the command slew
accepts all of the objects whose coordinates can be resolved. The currently available resolve modules are:
- CDS/Sesame: resolves mainly all of the "static" celestial objects (Messier catalogue, NGC objects, ...).
- MPC/Ephemerides: resolves mainly all of the moving solar system objects in accordance with the naming conventions of the IAU Minor Planet Center
- MPC/Natural satellites: resolves the irregular moons of the giant planets using the Natural Satellites Ephemeris Service of the Minor Planet Center.
- CCDSH/active targets: this resolver uses the CCDSH target database of the TAO project: https://ccdsh.konkoly.hu/supernovae. Any objects listed here can therefore be resolved using the corresponding coordinates. Note that this resolver is case-sensitive.
Just check the coordinates of your favourite object using the CCDSH built-in command resolve
. If this resolve
command cannot resolve the target name, then slew ...
won't do either.
Important comment: There is no set mount track [on|off]
for this telescope. The command slew
automatically starts the mount tracking, while asa slew taudec
does not. Therefore, stopping the telescope movement is equivalent to send the telescope to some fixed position via this latter command.
If in doubt, check mount status with asa status
:
ASA_mount: right_ascension: 289.08803 ASA_mount: declination: 12.96731 ASA_mount: azimuth: 0.04978 ASA_mount: altitude: 55.04869 ASA_mount: is_slewing: 0 ASA_mount: is_tracking: 0
The image orientation set by the derotator is always absolute, however, images between the zenith and pole (i.e. having declinations larger than the latitude, i.e. ~48 or ~46 degrees) are rotated by 180 degrees.
Imaging
From then the usual acquire
, set filter ...
and sequence
commands can be used. For example: CCD> sequence -n SN2019odp-%N -V -x 3*([B,180],[V,180],[g,180],[r,180],[i,180],[z,180])
.
Closing
Close the telescope after observations using the following procedure:
- Send the telescope to home position:
CCD> asa slew taudec 0,10
(Piszkéstető)CCD> asa slew taudec 0,-40
(Baja, in order to allow the dome doors to safely be closed)
- Mount tracking will not start this way.
- At Piszkéstető: send the dome to home position: if dome tracking is not turned off, the dome should rotate to its home position after the command above. Otherwise:
CCD>set dome azimuth=0
. - Close the telescope covers:
CCD> asa cover lower close
,CCD> asa cover upper close
.
- Warning: Close the lower cover first! Check
asa status
before closing the upper one!
- Close the dome and set it to manual mode:
CCD> set dome slit close
,CCD> set dome auto off
.
Focusing
Autofocus
At Piszkéstető, autofocus feature is now implemented using a linear correlation between focuser temperatures and independently set focus values from the last year or so. It can be used with the following syntax: asa autofocus <offset> <slope>
, where the offset and slope values are the parameters of the linear fit. E.g.:
CCD> asa autofocus 8.08 -0.017
The autofocus can be turned off with asa autofocus off
. Its status can be checked with the following commands:
CCD> asa status [...] ASA_ACC: focuser: position: 7.998 ASA_ACC: focuser: temperature: 15.9375
CCD> asa autofocus offset=8.08 slope=-0.017
CCD> asa autofocus off
A valid focus value still has to be set, but in case the autofocus is on, it is disregarded (in practice: while using TCS80_generate.sh
, an arbitrary focus value still has to be set).
Unfortunately, at the Baja site, the telescope does not have a built-in thermometer. Workarounds are underway!
Finding the right focus manually
- Slew to your favorite open cluster.
- Run this script:
source /usr/local/ccdsh/scripts/focus-longrange.ccdsh
- Check the result from a terminal:
display-focus.sh focus*.fits
- Apply the best focus value when observing or running the scheduler:
TCS80_generate.sh --start now --plot --verbose --sequential --focus 7.77 --already-open
Differences between the Piszkéstető and Baja site
Just a quick list about the subtle differences between Piszkéstető and Baja sites:
- Besides the infra light of the interior dome camera, there is no `dome` support for the Baja site.
- The home position is at
asa slew taudec 0,-40
at the Baja site - otherwise, it is extremely dangerous to close the dome. Please be very careful! - The Baja telescope does not have a thermometer, automatic temperature-compensated focusing does not work (until further improvements).
- While treated automatically, the zero point of the field rotators differ at the two sides. You don't have to care about this during routine operations but it is worth to know.
Known issues
See also this page for further minor issues. Issues stroke out like this have already been solved, you can ignore those. See also the end of this page: [1]