forked from tammojan/facet-calibration
-
Notifications
You must be signed in to change notification settings - Fork 0
/
a2256.parset
62 lines (41 loc) · 2.02 KB
/
a2256.parset
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
##### "example parset file" ####
#### USER INPUT #####
username = pwd.getpwuid(os.getuid())[0]
## USER INPUT ##
SCRIPTPATH = '/home/'+username+'/scripts/a2256_hba/'
buildmytasks = '/home/rvweeren/software/casapy/casapy-42.2.30986-1-64b/buildmytasks'
os.system('cp /home/'+username+'/scripts/a2256_hba/*.rgn .')
peelsourceinfo = '/home/'+username+'/scripts/a2256_hba/peel_source_info_a2256.txt'
wsclean = '/home/rvweeren/software/WSClean/wsclean-1.7/build/wsclean'
import os
os.system('cp ' + SCRIPTPATH + '/ftw.xml .')
os.system('cp ' + SCRIPTPATH + '/task_ftw.py .')
os.system(buildmytasks) # make casapy tasks
# this might need fixing for some
#example to use another selfcal script, not the default
#config.update({"selfcal":"selfcalv19_ww_jsm"})
clusterdesc='bla'
dbserver='bla'
dbname='bla'
dbuser='bla'
BANDS = range(160,239,10)
# or for example
# BANDS = range(50,359,10)
NAME = "A2256"
RES = "2ch10s"
do_sources=['s3','s4']
StartAtStep='preSC'
nterms = 1 # will be forced to 2 if WScleanWBgroup < len(mslist)
cellsize = 1.5 # still hardcoded in a few places, do not change for now
TEC = "True" # automatically set to False if needed
makemasks = False # not used anymore, keep to False
do_ap = True # normally this should be True, correct with instrument_ap_smoothed
uvrange = 5.0 # wavelength
WSCleanRobust = -0.25 # Briggs robust factor for facet imaging
BlankField = True # This blanks the field outside the facet boundary for the source detection, True should speed things up
StefCal = False # experimental, not working at the moment
Padding = False # To reduce aliasing in FFT subtract.
rmscheck = True # Check for much worse rms in the latest facet map
# for wideband clean set WScleanWBgroup below (must be smaller then len(mslist))
# for the -best- results use WScleanWBgroup=1, note this slows down the imaging considerably
WScleanWBgroup= 1 # number of blocks over which the spectral index is assumed to be constant, used in Wideband clean