def make_source (ns,name,l,m,I=1):
"""Makes a source with a direction, using the current option set.
Returns None for sources out of the "sky".
(l^2+m^2>1)""";
l = math.sin(l);
m = math.sin(m);
if l*l + m*m <= 1:
srcdir = Meow.LMDirection(ns,name,l,m);
if source_spi is not None:
freq0 = source_freq0*1e+6 if source_freq0 else Meow.Context.observation.freq0();
spi = source_spi if source_spi_2 is None else [ source_spi,source_spi_2 ];
else:
spi = freq0 = None;
if source_pol:
Q = I*source_qi;
U = I*source_ui;
V = I*source_vi;
else:
Q = U = V = None;
if source_type == "point":
return Meow.PointSource(ns,name,srcdir,I=I,Q=Q,U=U,V=V,spi=spi,freq0=freq0);
elif source_type == "gaussian":
s1,s2 = gauss_smaj*ARCSEC,gauss_smin*ARCSEC;
pa = gauss_pa*DEG;
return Meow.GaussianSource(ns,name,srcdir,I=I,Q=Q,U=U,V=V,spi=spi,freq0=freq0,
lproj=s1*math.sin(pa),mproj=s1*math.cos(pa),ratio=s2/s1);
# else fall through and return none
return None;
def source_list(ns):
# figure out spectral index parameters
if spectral_index is not None:
spi_def = Meow.Parm(spectral_index)
freq0_def = ref_freq
else:
spi_def = freq0_def = None
if spectral_index1 is not None:
spi_def1 = Meow.Parm(spectral_index1)
freq0_def1 = ref_freq
else:
spi_def1 = freq0_def1 = None
# and flux parameters
i_def = Meow.Parm(1)
quv_def = Meow.Parm(0)
dir1 = Meow.Direction(ns, "3C343.1", 4.356645791155902, 1.092208429052697)
dir0 = Meow.Direction(ns, "3C343", 4.3396003966265599, 1.0953677174056471)
src1 = Meow.PointSource(ns,
"3C343.1",
dir1,
I=Meow.Parm(6.02061051),
Q=Meow.Parm(0.0179716185),
U=quv_def,
V=quv_def,
spi=spi_def1,
freq0=freq0_def1)
src0 = Meow.PointSource(ns,
"3C343",
dir0,
I=Meow.Parm(1.83336309),
Q=Meow.Parm(0.0241450607),
U=quv_def,
V=quv_def,
spi=spi_def1,
freq0=freq0_def1)
## define a parmgroup for source parameters
pg_src = ParmGroup.ParmGroup("source",
src1.coherency().search(tags="solvable") +
src0.coherency().search(tags="solvable"),
table_name="sources.mep")
ParmGroup.SolveJob("cal_sources", "Calibrate sources", pg_src)
return [src1, src0]
def transient_source (ns,name,l,m,tburst,duration,Ipeak=1):
"""shortcut for making a transient pointsource with a direction. Returns None for sources out of the "sky"
(l^2+m^2>1)""";
l = math.sin(l);
m = math.sin(m);
t_rel = ns.t_rel ** (Meq.Time() - (ns.time0 << 0))
lc = ns.lc << Meq.Exp((-Meq.Pow(t_rel-tburst,2))/(2*duration**2))
Ilc = ns.Ilc << Ipeak * lc
if l*l + m*m <= 1:
srcdir = Meow.LMDirection(ns,name,l,m);
return Meow.PointSource(ns,name,srcdir,I=Ilc);
else:
return None;
def point_source(ns, name, l, m, I=1):
"""shortcut for making a pointsource with a direction. Returns None for sources out of the "sky"
(l^2+m^2>1)"""
l = math.sin(l)
m = math.sin(m)
if l * l + m * m <= 1:
srcdir = Meow.LMDirection(ns, name, l, m)
if source_spi is not None:
freq0 = source_freq0 or Meow.Context.observation.freq0()
else:
freq0 = None
return Meow.PointSource(ns, name, srcdir, I=I, spi=source_spi, freq0=freq0)
else:
return None
def make_source(ns, name, az, el, I=1):
"""Makes a source with a fixed azimuth/elevation direction """
srcdir = Meow.AzElDirection(ns, name, az, el)
if source_spi is not None:
freq0 = source_freq0 * 1e+6 if source_freq0 else Meow.Context.observation.freq0(
)
else:
freq0 = None
if source_pol:
Q = I * source_qi
U = I * source_ui
V = I * source_vi
else:
Q = U = V = None
if source_type == "point":
return Meow.PointSource(ns,
name,
srcdir,
I=I,
Q=Q,
U=U,
V=V,
spi=source_spi,
freq0=freq0)
elif source_type == "gaussian":
s1, s2 = gauss_smaj * ARCSEC, gauss_smin * ARCSEC
pa = gauss_pa * DEG
return Meow.GaussianSource(ns,
name,
srcdir,
I=I,
Q=Q,
U=U,
V=V,
spi=source_spi,
freq0=freq0,
lproj=s1 * math.sin(pa),
mproj=s1 * math.cos(pa),
ratio=s2 / s1)
# else fall through and return none
return None
def source_list (ns,name="cps"):
# figure out spectral index parameters
if spectral_index is not None:
spi_def = Meow.Parm(spectral_index);
freq0_def = ref_freq;
else:
spi_def = freq0_def = None;
i_def = Meow.Parm(1);
quv_def = Meow.Parm(0);
srcdir = Meow.LMDirection(ns,name,0,0);
src = Meow.PointSource(ns,name,srcdir,I=i_def,Q=quv_def,U=quv_def,V=quv_def,spi=spi_def,freq0=freq0_def);
## define a parmgroup for source parameters
## now make a solvejobs for the source
#pg_src = ParmGroup("source",
#src.coherency().search(tags="solvable"),
#table_name="sources.mep",
#individual=True,
#bookmark=True);
## now make a solvejobs for the source
#options.append(pg_src.make_solvejob_menu("Calibrate source fluxes"));
return [ src ];
def source_list (self,ns,max_sources=None,**kw):
"""Reads LSM and returns a list of Meow objects.
ns is node scope in which they will be created.
Keyword arguments may be used to indicate which of the source attributes are to be
created as Parms, use e.g. I=Meow.Parm(tags="flux") for this.
The use_parms option may override this.
""";
if self.filename is None:
return [];
if self.lsm is None:
self.load(ns);
# all=1 returns unsorted list, so use a large count instead, to get a sorted list
plist = self.lsm.queryLSM(count=9999999);
# parse the beam expression
if self.beam_expr is not None:
try:
beam_func = eval("lambda r,fq:"+self.beam_expr);
except:
raise RuntimeError("invalid beam expression");
else:
beam_func = None;
# make list of direction,punit,I,I_apparent tuples
parm = Meow.Parm(tags="source solvable");
srclist = [];
for pu in plist:
ra,dec,I,Q,U,V,spi,freq0,RM = pu.getEssentialParms(ns);
if self.solve_pos:
ra = parm.new(ra);
dec = parm.new(dec);
direction = Meow.Direction(ns,pu.name,ra,dec,static=not self.solve_pos);
Iapp = I;
if beam_func is not None:
# if phase centre is already set (i.e. static), then lmn will be computed here, and we
# can apply a beam expression
lmn = direction.lmn_static();
if lmn is not None:
r = sqrt(lmn[0]**2+lmn[1]**2);
Iapp = I*beam_func(r,freq0*1e-9 or 1.4); # use 1.4 GHz if ref frequency not specified
# append to list
srclist.append((pu.name,direction,pu,I,Iapp));
# sort list by decreasing apparent flux
from past.builtins import cmp
from functools import cmp_to_key
srclist.sort(key=cmp_to_key(lambda a,b:cmp(b[4],a[4])));
srclist_full = srclist;
# extract active subset
srclist = self._subset_parser.apply(self.lsm_subset,srclist_full,names=[src[0] for src in srclist_full]);
# extract solvable subset
solve_subset = self._subset_parser.apply(self.solve_subset,srclist_full,names=[src[0] for src in srclist_full]);
solve_subset = set([src[0] for src in solve_subset]);
# make copy of kw dict to be used for sources not in solvable set
kw_nonsolve = dict(kw);
# and update kw dict to be used for sources in solvable set
if self.solvable_sources:
if self.solve_I:
kw.setdefault("I",parm);
if self.solve_Q:
kw.setdefault("Q",parm);
if self.solve_U:
kw.setdefault("U",parm);
if self.solve_V:
kw.setdefault("V",parm);
if self.solve_spi:
kw.setdefault("spi",parm);
if self.solve_RM:
kw.setdefault("RM",parm);
if self.solve_pos:
kw.setdefault("ra",parm);
kw.setdefault("dec",parm);
if self.solve_shape:
kw.setdefault("sx",parm);
kw.setdefault("sy",parm);
kw.setdefault("phi",parm);
# make Meow list
source_model = []
## Note: conversion from AIPS++ componentlist Gaussians to Gaussian Nodes
### eX, eY : multiply by 2
### eP: change sign
for name,direction,pu,I,Iapp in srclist:
# print "%-20s %12f %12f"%(pu.name,I,Iapp);
src = {};
( src['ra'],src['dec'],
src['I'],src['Q'],src['U'],src['V'],
src['spi'],src['freq0'],src['RM'] ) = pu.getEssentialParms(ns)
(eX,eY,eP) = pu.getExtParms()
# scale 2 difference
src['sx'] = eX*2
src['sy'] = eY*2
src['phi'] = -eP
# override zero values with None so that Meow can make smaller trees
if not src['RM']:
src['RM'] = None;
if not src['spi']:
src['spi'] = None;
if src['RM'] is None:
src['freq0'] = None;
## construct parms or constants for source attributes
## if source is in solvable set (solvable_source_set of None means all are solvable),
## use the kw dict, else use the nonsolve dict for source parameters
if name in solve_subset:
solvable = True;
kwdict = kw;
else:
solvable = False;
kwdict = kw_nonsolve;
for key,value in src.items():
meowparm = kwdict.get(key);
if isinstance(meowparm,Meow.Parm):
src[key] = meowparm.new(value);
elif meowparm is not None:
src[key] = value;
if eX or eY or eP:
# Gaussians
if eY:
size,phi = [src['sx'],src['sy']],src['phi'];
else:
size,phi = src['sx'],None;
src = Meow.GaussianSource(ns,name=pu.name,
I=src['I'],Q=src['Q'],U=src['U'],V=src['V'],
direction=direction,
spi=src['spi'],freq0=src['freq0'],RM=src['RM'],
size=size,phi=phi);
else:
src = Meow.PointSource(ns,name=pu.name,
I=src['I'],Q=src['Q'],U=src['U'],V=src['V'],
direction=direction,
spi=src['spi'],freq0=src['freq0'],RM=src['RM']);
# check for beam LM
if pu._lm is not None:
src.set_attr('beam_lm',pu._lm);
src.solvable = solvable;
src.set_attr('Iapp',Iapp);
source_model.append(src);
return source_model;
def source_list(self, ns, max_sources=None, **kw):
"""Reads LSM and returns a list of Meow objects.
ns is node scope in which they will be created.
Keyword arguments may be used to indicate which of the source attributes are to be
created as Parms, use e.g. I=Meow.Parm(tags="flux") for this.
The use_parms option may override this.
"""
if self.filename is None:
return []
# load the sky model
if self.lsm is None:
self.lsm = Tigger.load(self.filename)
# sort by brightness
import functools
from past.builtins import cmp
from functools import cmp_to_key
sources = sorted(
self.lsm.sources,
key=cmp_to_key(lambda a, b: cmp(b.brightness(), a.brightness())))
# extract subset, if specified
sources = SourceSubsetSelector.filter_subset(self.lsm_subset, sources,
self._getTagValue)
# get nulls subset
if self.null_subset:
nulls = set([
src.name for src in SourceSubsetSelector.filter_subset(
self.null_subset, sources)
])
else:
nulls = set()
parm = Meow.Parm(tags="source solvable")
# make copy of kw dict to be used for sources not in solvable set
kw_nonsolve = dict(kw)
# and update kw dict to be used for sources in solvable set
# this will be a dict of lists of solvable subgroups
parms = []
subgroups = {}
if self.solvable_sources:
subgroup_order = []
for sgname in _SubgroupOrder:
if getattr(self, 'solve_%s' % sgname):
sg = subgroups[sgname] = []
subgroup_order.append(sgname)
# make Meow list
source_model = []
for src in sources:
is_null = src.name in nulls
# this will be True if this source has solvable parms
solvable = self.solvable_sources and not is_null and (
not self.lsm_solvable_tag
or getattr(src, self.lsm_solvable_tag, False))
if solvable:
# independent groups?
if self.lsm_solve_group_tag:
independent_sg = sgname = "%s:%s" % (
self.lsm_solve_group_tag,
getattr(src, self.lsm_solve_group_tag, "unknown"))
else:
independent_sg = ""
sgname = 'source:%s' % src.name
if sgname in subgroups:
sgsource = subgroups[sgname]
else:
sgsource = subgroups[sgname] = []
subgroup_order.append(sgname)
# make dict of source parametrs: for each parameter we have a value,subgroup pair
if is_null:
attrs = dict(ra=src.pos.ra,
dec=src.pos.dec,
I=0,
Q=None,
U=None,
V=None,
RM=None,
spi=None,
freq0=None)
else:
attrs = dict(
ra=src.pos.ra,
dec=src.pos.dec,
I=src.flux.I,
Q=getattr(src.flux, 'Q', None),
U=getattr(src.flux, 'U', None),
V=getattr(src.flux, 'V', None),
RM=getattr(src.flux, 'rm', None),
freq0=getattr(src.flux, 'freq0', None)
or (src.spectrum and getattr(src.spectrum, 'freq0', None)),
spi=src.spectrum and getattr(src.spectrum, 'spi', None))
if not is_null and isinstance(src.shape, ModelClasses.Gaussian):
attrs['lproj'] = src.shape.ex * math.sin(src.shape.pa)
attrs['mproj'] = src.shape.ex * math.cos(src.shape.pa)
attrs['ratio'] = src.shape.ey / src.shape.ex
# construct parms or constants for source attributes, depending on whether the source is solvable or not
# If source is solvable and this particular attribute is solvable, replace
# value in attrs dict with a Meq.Parm.
if solvable:
for parmname, value in list(attrs.items()):
sgname = _Subgroups.get(parmname, None)
if sgname in subgroups:
solvable = True
parm = attrs[parmname] = ns[src.name](
parmname) << Meq.Parm(value or 0,
tags=["solvable", sgname],
solve_group=independent_sg)
subgroups[sgname].append(parm)
sgsource.append(parm)
parms.append(parm)
# construct a direction
direction = Meow.Direction(ns,
src.name,
attrs['ra'],
attrs['dec'],
static=not solvable
or not self.solve_pos)
# construct a point source or gaussian or FITS image, depending on source shape class
if src.shape is None or is_null:
msrc = Meow.PointSource(ns,
name=src.name,
I=attrs['I'],
Q=attrs['Q'],
U=attrs['U'],
V=attrs['V'],
direction=direction,
spi=attrs['spi'],
freq0=attrs['freq0'],
RM=attrs['RM'])
elif isinstance(src.shape, ModelClasses.Gaussian):
msrc = Meow.GaussianSource(ns,
name=src.name,
I=attrs['I'],
Q=attrs['Q'],
U=attrs['U'],
V=attrs['V'],
direction=direction,
spi=attrs['spi'],
freq0=attrs['freq0'],
lproj=attrs['lproj'],
mproj=attrs['mproj'],
ratio=attrs['ratio'])
if solvable and 'shape' in subgroups:
subgroups['pos'] += direction.get_solvables()
elif isinstance(src.shape, ModelClasses.FITSImage):
msrc = Meow.FITSImageComponent(ns,
name=src.name,
filename=src.shape.filename,
direction=direction)
msrc.set_options(fft_pad_factor=(src.shape.pad or 2))
msrc.solvable = solvable
# copy standard attributes from sub-objects
for subobj in src.flux, src.shape, src.spectrum:
if subobj:
for attr, val in src.flux.getAttributes():
msrc.set_attr(attr, val)
# copy all extra attrs from source object
for attr, val in src.getExtraAttributes():
msrc.set_attr(attr, val)
# make sure Iapp exists (init with I if it doesn't)
if msrc.get_attr('Iapp', None) is None:
msrc.set_attr('Iapp', src.flux.I)
source_model.append(msrc)
# if any solvable parms were made, make a parmgroup and solve job for them
if parms:
if os.path.isdir(self.filename):
table_name = os.path.join(self.filename, "sources.fmep")
else:
table_name = os.path.splitext(self.filename)[0] + ".fmep"
# make list of Subgroup objects for every non-empty subgroup
sgs = []
for sgname in subgroup_order:
sglist = subgroups.get(sgname, None)
if sglist:
sgs.append(Meow.ParmGroup.Subgroup(sgname, sglist))
# make main parm group
pg_src = Meow.ParmGroup.ParmGroup("source parameters",
parms,
subgroups=sgs,
table_name=table_name,
table_in_ms=False,
bookmark=True)
# now make a solvejobs for the source
Meow.ParmGroup.SolveJob("cal_source",
"Solve for source parameters", pg_src)
return source_model