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| # makeschedule :: Task to create JVLA schedules for mosaics or observations of large source lists.
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| pointing_file = '' # Input file
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| frame = 'equatorial' # Coordinate frame (equatorial or galactic)
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| position = '1:33:51.00,30:39:37' # Central position of mosaic (hh:mm:ss.s,dd:mm:ss.s)
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| delta = 6 # Pointing spacing (arcmin)
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| x_points = 12 # Pointings in RA (l)
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| y_points = 12 # Pointings in DEC (b)
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| poi_type = 'hexagonal' # Options: 'hexagonal' or 'rectangular'
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| start_LST = 20 # Start LST time
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| setup_time = 8.0 # Initial setup time (min)
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| cal_order = 'BTF' # Order of different parts of the schedule (F=Flux cal; B=bandpass cal; T=target
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| # sources- including phase calibrators)
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| flux_cal = '3C48' # Flux calibrator ('3C48','3C147','3C286', or '3C138')
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| flux_time = 2.0 # Time on flux calibrator (min)
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| bp_cal = 'J1733-1304' # Bandpass calibrator '' => same as flux_cal
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| bp_time = 4.0 # Time on Bandpass calibrator (min)
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| n_visits = 2 # number of cycles
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| scan_time = 33 # Duration of each pointing (sec)
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| cal_time = 60 # Duration on phase-cal (sec)
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| cal_freq = 20 # Max. time between phase-cal scans (min)
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| do_poi = True # True: Do reference pointing; False: Do not do this.
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| poi_freq = 60.0 # Time between reference pointing scans (min)
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| poi_res = 'Primary X band pointing' # Resource for pointing
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| poi_time = 180.0 # Time for reference pointings (sec)
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| max_diff = [15.0, 15.0] # Do new reference pointing if new calibrator is not within x deg (az,el) of old
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| # reference pointing
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| phase_cals = ['J0137+3309'] # List of phase calibrators.
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| optimize = 'simple' # Options: 'simple' (optimize for ra,dec) or 'complex' (optimize for az,el)
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| start_first_poi = True # True: Start with first pointing in list; False: Start with closest pointing to
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| # calibrator
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| use_loops = True # True: Group all scans between phase-calibrators into a loop; False: Do not do
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| # this.
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| group_name = '' # Source group name in SCT
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| source_cat = 'Methanol' # Source Catalog Name in SCT
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| resource_cat = 'RSRO' # Resource Catalog Name in RCT
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| resource = 'C-Band + RRL (Galaxy)' # Resource Name in RCT
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| beam = 12 # beam in arcmin (regions)
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| plot = [1, 0, 1, 0, 0] # Plot start,end,raster,slew,uptime
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| max_scan_length = 120 # Maximal scan length (sec)
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| async = False # If true the taskname must be started using makeschedule(...)
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Download task files: Download task files: File:Task makeschedule.py, File:Makeschedule.xml
Task to create complete schedules for JVLA observations that can be imported as a scan lists into the OPT,
including initial setup, observations of flux and banpass calibrators, pointing scans, and phase calibrators.
The task can run either on a pre-defined 'pointing_file' in SCT format, or it can generate a mosaic either in
equatorial (J2000.0) or galactic coordinates centered at a specific 'position'.
If many sources at different positions in the sky are observed, the program will pick the closest phase
calibrator from 'phase_cals' and group sources related to each phase calibrator together. The task will then
schedule the groups in the order of the list of phase calibrators given in 'phase_cals'. Phase calibrators with
no associated targets will be ignored.
The task will try to optimize the sequence of pointings, by always selecting the closest remaining target source
for optimization = 'simple'. The 'complex' optimization can reduce settling times and gain a few seconds on source,
but it runs much slower (in particular for large mosaics with a few hundred pointings). This is only recomended for
mosacis with very short time per pointing (e.g. 12 seconds).
Output files are:
pointings.pst -- File with pointing positions in SCT format to be read into the OPT.
scan_list_xxLST.opt -- Scan list to be imported to the OPT (import scans) for the specified LST start time.
regions.reg -- Region file for ds9
Example:
