Releases: sdss/lvmgort
Releases Β· sdss/lvmgort
GORT 0.11.0
π New
- #23 Added observer calibration scripts as recipes
quick_cals
,bias_sequence
, andtwilight_flats
.
π§ Fixed
- Fixed a serious issue in which if the slew fails, the retry did not send the PA and it would default to PA=0.
- After the initial slew, subsequent slews of the spec telescope do not check for whether the enclosure state is remote.
GORT 0.10.0
π New
- #20 Added
GuiderSet.monitor()
which can be used to guide at zenith with low cadence and monitor transparency and FWHM while conditions are bad.
β¨ Improved
GORT 0.9.0
π New
- Tile standard coordinates can now be defined as a list of Gaia DR3 source IDs. If the standard coordinates is a single integer, it will be assumed to be a source ID and the coordinates will be retrieved from the database.
- Added code for telescope pointing models.
β¨ Improved
- Break out of `Gort.observe()`` on keyboard interrupt
- Added
utilities_room
light to enclosure. - Update astropy to 6.0.0 and avoid it requiring to download orientation data from the internet.
π§ Fixed
- Fixed exposure loop not restarting after a keyboard interrupt.
GORT 0.8.0
π New
- #13 Adds a signal handler for
SIGINT
andSIGTERM
. WhenGortObserver
is running and an interrupt is received the signal handler will run the cleanup routine. - Added
spectrograph_room
light to enclosure.
β¨ Improved
SpectrographSet.reset
now acceptsfull=True
which performs additional checks and opens/closes the shutter and hartmann doors as needed.reset
withfull=True
is run automatically during thecleanup
recipe.- The GORT websocket now uses the CLU model for
lvmecp
instead of asking the PLC to report its status on each call toWebsocketServer.enclosure_status()
.
GORT 0.7.1
β¨ Improved
- #14 Turn off dome lights as part of the
startup
andcleanup
recipes. - Use `lvmnps all-off`` to turn off all lamps faster.
π·οΈ Changed
- Disable marking tiles as bad on error for now. This could cause confusion if an exposure failed and the tile was marked bad, but then the images were recovered using lockfiles.
- Skip the calibration sequence on startup by default.
GORT 0.7.0
π New
- Added
selfie
position.
β¨ Improved
- Added NPS devices for telescopes and MOCON.
- Added spectrograph exposure and enclosure timeouts.
- Support exposing only some spectrographs.
- Verify the number of files writtent to disk by the spectrographs and their MD5s.
- Mark exposure bad in post-readout if it fails.
π·οΈ Changed
- Relaxed spec and sky telescope guiding tolerances to 3 arcsec.
π§ Fixed
- Updated
NPS
to handlelvmnps
1.0.0 (including upgrade tounclick
0.1.0).
GORT 0.6.2
β¨ Improved
- File logger logs to
logging.path
(defaults to/data/logs/lvmgort/<SJD>.log
).
π·οΈ Changed
- Disable guider corrections for
spec
telescope after acquisition. This prevents field rotation affecting the exposure at the cost of tracking error. - Pass
-PA
to the guider due to different handiness for PA between the guider and the tiling database.
π§ Fixed
- Fixed a bug in the recording of the standards acquisition and exposure times.
GORT 0.6.1
β¨ Improved
- Pass
force
to_prepare_telescopes()
.
π·οΈ Changed
- Do not run cleanup after each iteration in
Gort.observe()
- Set
stop_degs_before.sci
to 1.5.
GORT 0.6.0
π New
- #11 Support asynchronous readout during
GortObserved
-enabled observations and implement dithering:- Remove calls to
lvmguider stop --now
. The newstop
command always cancels the guider task. - Added
pre-readout
hook forExposure
. - Allow
GortObserver
to read out an exposure asynchronously. Gort.observe_tile()
will by default read the last exposure asynchronously to allow for the next slew and acquisition to happen during readout.- Added a context manager
GortObserver.register_overhead()
that measured the elapsed time in different parts of the slew and acquisition process and records the values to the database. - The dither positions associated with a
Tile
are now a list of positions that the scheduler wants us to observe.Gort.observe_tile()
will try to observe all dither positions without stopping the guider. - Added
Gort.observe()
with a simple loop for observing tiles.
- Remove calls to
- Add dither information to
Tile
and support exposing multiple dither positions in the same observation.
β¨ Improved
- Pass the observed sky and standard pks to the scheduler during registration.
- The K-mirror offset angle is now wrapped between -180 and 180 degrees. Hopefully this prevents some cases in which offsets angles very close to 360 degrees cause the K-mirror to fail because of a software limit.
π§ Fixed
- Fixed deprecations in Pandas
fillna()
withmethod='bfill'
.
GORT 0.5.0
π New
- Added support for telescope enclosure lights.
β¨ Improved
- #10
GortObserver.slew()
and the standard iteration task now calculate the adjusted target coordinates for the spec telescope so that the slew puts the star on top of the desired fibre to be observed. Most of this relies on code copied fromlvmtipo
used to calculate the field angle through the siderostat. SkyCoordinates
now accepts aname
attribute that is passed to theSKYENAME
andSKYWNAME
header keywords.- IFU PA angles passed to the headers.
- Pass exposure time when registering an exposure.
- Support new outputs from
lvmguider 0.4.0b1
. - Get actor versions on init.
- Support guiding in PA (disabled for now).
- Reconnect AGs during
startup
recipe. - Add
tile_id
as `OBJECT`` if no object string user-defined.
π·οΈ Changed
- Set
GR{telescope}FR{0|N}
with the range of guider frames in which we were guiding (as opposed to the entire guide loop including acquisition frames). - Changed default guide tolerance to 1 arcsec.
π§ Fixed
- Fixed some additional issues with the exception hooks that cause a recursion loop in IPython in some cases.
- Fixed a bug that would accumulate the range of guider frames for an spectrograph exposure if
GortObserver.expose()
was called multiple times. - Fixed a slicing issue with newer versions of Pandas.
- Fixed a bug that caused the exposure flavour not being passed to the headers.
- Deal with cases when the scheduler cannot find a good tile to observe.