def get_coord(targ_file, radec=None):
'''
radec: int (None)
None: Read from ASCII file
1: List of [Name, RA, DEC] with RA/DEC as : separated strings
2: List of [Name, RA, DEC] with RA/DEC as decimal degrees
'''
if not isinstance(targ_file, basestring):
raise IOError('Bad input to finder.get_coord!')
from astropy.io import ascii
# Import Tables
if radec == None:
# Read
ra_tab = ascii.read(targ_file) #, names=('Name','RA','DEC','Epoch'))
# Rename the columns
ra_tab.rename_column('col1', 'Name')
if isinstance(ra_tab['col2'][0], basestring):
ra_tab.rename_column('col2', 'RAS')
ra_tab.rename_column('col3', 'DECS')
else:
ra_tab.rename_column('col2', 'RA')
ra_tab.rename_column('col3', 'DEC')
elif radec == 1:
# Error check
if len(targ_file) != 3:
return -1
# Manipulate
arr = np.array(targ_file).reshape(1, 3)
# Generate the Table
ra_tab = QTable(arr, names=('Name', 'RAS', 'DECS'))
elif radec == 2:
# Error check
if len(targ_file) != 3:
return -1
# Manipulate
ras, decs = x_r.dtos1((targ_file[1], targ_file[2]))
# Generate the Table
ra_tab = QTable([[targ_file[0]], [ras], [decs]],
names=('Name', 'RA', 'DEC'))
else:
raise ValueError('get_coord: Bad flag')
# Add dummy columns for decimal degrees and EPOCH
nrow = len(ra_tab)
col_RAD = Column(name='RAD', data=np.zeros(nrow), unit=astrou.degree)
col_DECD = Column(name='DECD', data=np.zeros(nrow), unit=astrou.degree)
col_EPOCH = Column(name='EPOCH', data=np.zeros(nrow))
ra_tab.add_columns([col_RAD, col_DECD, col_EPOCH])
# Assume 2000 for now
ra_tab['EPOCH'] = 2000.
return ra_tab
def get_coord(targ_file, radec=None):
'''
radec: int (None)
None: Read from ASCII file
1: List of [Name, RA, DEC] with RA/DEC as : separated strings
2: List of [Name, RA, DEC] with RA/DEC as decimal degrees
'''
if not isinstance(targ_file,basestring):
raise IOError('Bad input to finder.get_coord!')
from astropy.io import ascii
# Import Tables
if radec == None:
# Read
ra_tab = ascii.read(targ_file) #, names=('Name','RA','DEC','Epoch'))
# Rename the columns
ra_tab.rename_column('col1','Name')
if isinstance(ra_tab['col2'][0],basestring):
ra_tab.rename_column('col2','RAS')
ra_tab.rename_column('col3','DECS')
else:
ra_tab.rename_column('col2','RA')
ra_tab.rename_column('col3','DEC')
elif radec == 1:
# Error check
if len(targ_file) != 3:
return -1
# Manipulate
arr = np.array(targ_file).reshape(1,3)
# Generate the Table
ra_tab = QTable( arr, names=('Name','RAS','DECS') )
elif radec == 2:
# Error check
if len(targ_file) != 3:
return -1
# Manipulate
ras, decs = x_r.dtos1((targ_file[1], targ_file[2]))
# Generate the Table
ra_tab = QTable( [ [targ_file[0]], [ras], [decs] ], names=('Name','RA','DEC') )
else:
raise ValueError('get_coord: Bad flag')
# Add dummy columns for decimal degrees and EPOCH
nrow = len(ra_tab)
col_RAD = Column(name='RAD', data=np.zeros(nrow), unit=astrou.degree)
col_DECD = Column(name='DECD', data=np.zeros(nrow), unit=astrou.degree)
col_EPOCH = Column(name='EPOCH', data=np.zeros(nrow))
ra_tab.add_columns( [col_RAD, col_DECD, col_EPOCH] )
# Assume 2000 for now
ra_tab['EPOCH'] = 2000.
return ra_tab
def starlist(targs, outfil=None):
'''
Generates a Keck approved starlist
FORMAT:
1-25: Name
Then: RA, DEC, EPOCH [WITH COLONS!]
Parameters:
----------
targs: Table (targets with RA, DEC)
outfil: string (None)
'''
reload(x_rad)
# Init
if outfil is None:
outfil = 'starlist.txt'
# Open
f = open(outfil, 'w')
# Name tag
name_tag = get_name_tag(targs.dtype.names)
# Loop
for jj, targ in enumerate(targs):
ras, decs = x_rad.dtos1((targ['RA'], targ['DEC']))
#decs = targ['DEC'].replace(':',' ')
if not decs[0] in ['+', '-']:
decs = '+' + decs
# Name
mask = []
while type(targ[name_tag]) is MaskedConstant:
mask.append(name_tag)
name_tag = get_name_tag(targs.dtype.names, mask=mask)
lin = targ[name_tag][0:3] + '_J' + ras.replace(
':', '')[0:4] + decs.replace(':', '')[0:5]
#xdb.set_trace()
# RA
lin = lin + ' ' + ras
# DEC
lin = lin + ' ' + decs
# EPOCH
lin = lin + ' 2000.'
# Write
f.write(str(lin + '\n'))
# Close
print('lick.wiki: Wrote starlist -- {:s}'.format(outfil))
f.close()
def starlist(targs, outfil=None):
'''
Generates a Keck approved starlist
FORMAT:
1-25: Name
Then: RA, DEC, EPOCH [WITH COLONS!]
Parameters:
----------
targs: Table (targets with RA, DEC)
outfil: string (None)
'''
reload(x_rad)
# Init
if outfil is None:
outfil = 'starlist.txt'
# Open
f = open(outfil, 'w')
# Name tag
name_tag = get_name_tag(targs.dtype.names)
# Loop
for jj,targ in enumerate(targs):
ras,decs = x_rad.dtos1((targ['RA'], targ['DEC']))
#decs = targ['DEC'].replace(':',' ')
if not decs[0] in ['+','-']:
decs = '+'+decs
# Name
mask = []
while type(targ[name_tag]) is MaskedConstant:
mask.append(name_tag)
name_tag = get_name_tag(targs.dtype.names,mask=mask)
lin = targ[name_tag][0:3]+'_J'+ras.replace(':','')[0:4]+decs.replace(':','')[0:5]
#xdb.set_trace()
# RA
lin = lin + ' ' + ras
# DEC
lin = lin + ' ' + decs
# EPOCH
lin = lin + ' 2000.'
# Write
f.write(str(lin+'\n'))
# Close
print('lick.wiki: Wrote starlist -- {:s}'.format(outfil))
f.close()
def mmt_targets(field, path=None):
'''Read files related to MMT targets
Parameters:
-----------
field: tuple
(Name, ra, dec)
Returns:
----------
Target and observing info
'''
if path is None:
path = '/Galx_Spectra/MMT/'
# Targets
targ_path = field[0] + path
# Target file
targ_file = glob.glob(targ_path + '*.targ')
if len(targ_file) != 1:
raise ValueError('Wrong number of MMT target files')
else:
targ_file = targ_file[0]
# Read PI, program info [NOT IMPLEMENTED]
#f = open(msk_file, 'r')
#lines = f.readlines()
#f.close()
# Read target table
tab = ascii.read(targ_file, comment='#')
# Restrict to targets
itarg = np.where(tab['type'] == 'TARGET')
targs = tab[itarg]
# Polish
nrow = len(targs)
targs.rename_column('ra', 'RAS')
targs.rename_column('dec', 'DECS')
targs.add_column(Column([0.] * nrow, name='TARG_RA'))
targs.add_column(Column([0.] * nrow, name='TARG_DEC'))
# Get RA/DEC in degrees
for k, row in enumerate(targs):
rad, decd = xra.stod1((row['RAS'], row['DECS']))
targs[k]['TARG_RA'] = rad.value
targs[k]['TARG_DEC'] = decd.value
targs.rename_column('objid', 'TARG_ID')
targs.rename_column('mag', 'TARG_MAG')
targs.add_column(Column([0.] * nrow, name='EPOCH'))
targs.add_column(Column(['SDSS'] * nrow, name='TARG_IMG'))
targs.add_column(Column(['HECTOSPEC'] * nrow, name='INSTR'))
targ_mask = {}
cnames = ['MASK_NAME', 'MASK_ID']
smsk = '--'
msk_val = [smsk] * len(cnames)
for kk, cname in enumerate(cnames):
targ_mask[cname] = [msk_val[kk]] * nrow
# Now the 'mask' files
mask_files = glob.glob(targ_path + '*.cat')
all_obs = []
all_masks = []
for mask_file in mask_files:
print('Reading MMT mask file: {:s}'.format(mask_file))
i0 = mask_file.rfind('/')
mask_nm = mask_file[i0 + 1:mask_file.find('.cat')]
# Grab info from spectrum file
#xdb.set_trace()
spec_fil = glob.glob(mask_file[:i0 + 1] + 'spHect-' + mask_nm +
'*.fits.gz')
if len(spec_fil) != 1:
print('spec_fil -- Not found!'.format(spec_fil))
ras, decs = xra.dtos1((field[1], field[2]))
pa = 0.
else:
header = fits.open(spec_fil[0])[0].header
if header['APERTURE'] != mask_nm:
raise ValueError('Mask doesnt match!')
pa = header['POSANGLE']
ras = header['CAT-RA']
decs = header['CAT-DEC']
# Continuing
mask_dict = dict(
INSTR='HECTOSPEC',
MASK_NAME=mask_nm,
MASK_RA=ras,
MASK_DEC=decs,
MASK_EPOCH=2000.,
MASK_PA=pa) # SHOULD GRAB PA, RA, DEC FROM SPECTRA FITS HEADER
all_masks.append(mask_dict)
# Read obs
f = open(mask_file, 'r')
lines = f.readlines()
f.close()
iall_obs = []
for line in lines:
if 'OBS' in line:
prs = line.strip().split(' ')
gdprs = [iprs for iprs in prs if len(iprs) > 0]
obs_dict = {}
obs_dict['DATE'] = gdprs[2]
obs_dict['TEXP'] = float(gdprs[3])
obs_dict['DISPERSER'] = gdprs[4]
obs_dict['CONDITIONS'] = gdprs[5]
#
iall_obs.append(obs_dict)
obs_tab = xxul.dict_list_to_table(iall_obs)
obs_tab['TEXP'].unit = u.s
# Read observed targets
obs_targ = ascii.read(mask_file, comment='#')
gdt = np.where(obs_targ['flag'] == 1)[0]
for gdi in gdt:
mtt = np.where(targs['TARG_ID'] == int(obs_targ['objid'][gdi]))[0]
if len(mtt) != 1:
raise ValueError('Multiple matches?!')
targ_mask['MASK_NAME'][mtt[0]] = mask_nm
all_obs.append(obs_tab)
# Finish
mask = np.array([False] * len(targs))
bad = np.where(np.array(targ_mask['names']) == '--')[0]
if len(bad) > 0:
mask[bad] = True
#
clm = MaskedColumn(targ_mask['names'], name='MASK_NAME', mask=mask)
targs.add_column(clm)
return all_masks, all_obs, targs
def main(inp, survey='2r', radec=None, deci=None, fpath=None, show_circ=True,
EPOCH=0., DSS=None, BW=False, imsize=5.*astrou.arcmin, show_spec=False,
OUT_TYPE='PDF'):
'''
Parameters:
---------
inp: Input
string or List of strings or List of several items
'ra_dec_list.txt' -- ASCII file with columns of Name,RA,DEC and RA,DEC are string or float (deg)
['NAME_OF_TARG', '10:31:38.87', '+25:59:02.3']
['NAME_OF_TARG', 124.24*u.deg, -23.244*u.deg]
['NAME_OF_TARG', SkyCoord]
radec: integer (0) [DEPRECATED!]
Flag indicating type of input
0 = ASCII file with columns of Name,RA,DEC and RA,DEC are string or float (deg)
1 = List of string ['Name', 'RA', 'DEC']
2 = ['Name', ra_deg, dec_deg]
BW: bool (False)
B&W image?
show_circ: bool (True)
Show a yellow circle on the target
show_spec: bool (False)
Try to grab and show an SDSS spectrum
imsize: Quantity, optional
Image size
OUT_TYPE: str, optional
File type -- 'PDF', 'PNG'
'''
reload(x_r)
reload(xgs)
import matplotlib.pyplot as plt
import matplotlib.cm as cm
# Init
if fpath is None:
fpath = './'
try:
imsize=imsize.to('arcmin').value
except AttributeError:
raise AttributeError('finder: Input imsize needs to be an Angle')
cradius = imsize / 50.
# Read in the Target list
if isinstance(inp,basestring):
ra_tab = get_coord(targ_file, radec=radec)
else:
ira_tab = {}
ira_tab['Name'] = inp[0]
if isinstance(inp[1],basestring):
ra, dec = x_r.stod1((inp[1],inp[2]))
ira_tab['RA'] = ra
ira_tab['DEC'] = dec
elif isinstance(inp[1],float):
ira_tab['RA'] = inp[1] * astrou.deg
ira_tab['DEC'] = inp[2]* astrou.deg
elif isinstance(inp[1],SkyCoord):
ira_tab['RA'] = inp[1].ra.deg
ira_tab['DEC'] = inp[1].dec.deg
else: # Should check it is a Quantity
ira_tab['RA'] = inp[1]
ira_tab['DEC'] = inp[2]
# Strings
ras,decs = x_r.dtos1((ira_tab['RA'],ira_tab['DEC']))
ira_tab['RAS'] = ras
ira_tab['DECS'] = decs
# Make a list
ra_tab = [ira_tab]
# Grab ra, dec in decimal degrees
if deci is not None:
return
#xdb.set_trace()
#x_r.stod(ra_tab) #ra_tab['RA'][q], ra_tab['DEC'][q], TABL)
# Precess (as necessary)
if EPOCH > 1000.:
from astropy import units as u
from astropy.coordinates import FK5
from astropy.time import Time
# Precess to 2000.
tEPOCH = Time(EPOCH, format='jyear', scale='utc')
# Load into astropy
fk5c = FK5(ra=ra_tab['RA'], dec=ra_tab['DEC'], equinox=tEPOCH, unit=(u.degree,u.degree))
# Precess
newEPOCH = Time(2000., format='jyear', scale='utc')
newfk5 = fk5c.precess_to(newEPOCH)
# Save
ra_tab['RA'] = newfk5.ra.degree
ra_tab['DEC'] = newfk5.dec.degree
# Strings too?
ra_tab['RAS'] = str(newfk5.ra.to_string(unit=u.hour,sep=':'))
ra_tab['DECS'] = str(newfk5.dec.to_string(unit=u.hour,sep=':'))
##
# Main Loop
for obj in ra_tab:
# Outfil
nm = "".join(obj['Name'].split())
if OUT_TYPE=='PNG':
outfil = fpath+ nm + '.png'
else:
outfil = fpath+ nm + '.pdf'
print(outfil)
# Grab the Image
reload(xgs)
img, oBW = xgs.getimg(obj['RA'], obj['DEC'], imsize, BW=BW,DSS=DSS)
# Generate the plot
plt.clf()
fig = plt.figure(dpi=1200)
fig.set_size_inches(8.0,10.5)
# Font
plt.rcParams['font.family']= 'times new roman'
ticks_font = matplotlib.font_manager.FontProperties(family='times new roman',
style='normal', size=16, weight='normal', stretch='normal')
ax = plt.gca()
for label in ax.get_yticklabels() :
label.set_fontproperties(ticks_font)
for label in ax.get_xticklabels() :
label.set_fontproperties(ticks_font)
# Image
if oBW == 1:
cmm = cm.Greys_r
else:
cmm = None
plt.imshow(img,cmap=cmm,aspect='equal',extent=(-imsize/2., imsize/2, -imsize/2.,imsize/2))
# Axes
plt.xlim(-imsize/2., imsize/2.)
plt.ylim(-imsize/2., imsize/2.)
# Label
plt.xlabel('Relative ArcMin', fontsize=20)
xpos = 0.12*imsize
ypos = 0.02*imsize
plt.text(-imsize/2.-xpos, 0., 'EAST', rotation=90.,fontsize=20)
plt.text(0.,imsize/2.+ypos, 'NORTH', fontsize=20, horizontalalignment='center')
# Title
plt.text(0.5,1.24, str(nm), fontsize=32,
horizontalalignment='center',transform=ax.transAxes)
plt.text(0.5,1.16, 'RA (J2000) = '+str(obj['RAS']), fontsize=28,
horizontalalignment='center',transform=ax.transAxes)
plt.text(0.5,1.10, 'DEC (J2000) = '+str(obj['DECS']), fontsize=28,
horizontalalignment='center',transform=ax.transAxes)
#import pdb; pdb.set_trace()
# Circle
if show_circ:
circle=plt.Circle((0,0),cradius,color='y', fill=False)
plt.gca().add_artist(circle)
# Spectrum??
if show_spec:
spec_img = xgs.get_spec_img(obj['RA'], obj['DEC'])
plt.imshow(spec_img,extent=(-imsize/2.1, imsize*(-0.1), -imsize/2.1, imsize*(-0.2)))
# Write
if show_spec:
plt.savefig(outfil, dpi=300)
else:
plt.savefig(outfil)
print 'finder: Wrote '+outfil
plt.close()
#xdb.set_trace()
print 'finder: All done.'
return oBW
def main(inp,
survey='2r',
radec=None,
deci=None,
fpath=None,
show_circ=True,
EPOCH=0.,
DSS=None,
BW=False,
imsize=5. * astrou.arcmin,
show_spec=False,
OUT_TYPE='PDF',
show_another=None):
'''
Parameters:
---------
inp: Input
string or List of strings or List of several items
'ra_dec_list.txt' -- ASCII file with columns of Name,RA,DEC and RA,DEC are string or float (deg)
['NAME_OF_TARG', '10:31:38.87', '+25:59:02.3']
['NAME_OF_TARG', 124.24*u.deg, -23.244*u.deg]
['NAME_OF_TARG', SkyCoord]
radec: integer (0) [DEPRECATED!]
Flag indicating type of input
0 = ASCII file with columns of Name,RA,DEC and RA,DEC are string or float (deg)
1 = List of string ['Name', 'RA', 'DEC']
2 = ['Name', ra_deg, dec_deg]
BW: bool (False)
B&W image?
show_circ: bool (True)
Show a yellow circle on the target
show_another : tuple, optional
RA,DEC for another target to circle (e.g. offset star)
show_spec: bool (False)
Try to grab and show an SDSS spectrum
imsize: Quantity, optional
Image size
OUT_TYPE: str, optional
File type -- 'PDF', 'PNG'
'''
reload(x_r)
reload(xgs)
import matplotlib.pyplot as plt
import matplotlib.cm as cm
# Init
if fpath is None:
fpath = './'
try:
imsize = imsize.to('arcmin').value
except AttributeError:
raise AttributeError('finder: Input imsize needs to be an Angle')
cradius = imsize / 50.
# Read in the Target list
if isinstance(inp, basestring):
raise NotImplementedError("No longer implemented")
#ra_tab = get_coord(targ_file, radec=radec)
else:
ira_tab = {}
ira_tab['Name'] = inp[0]
if isinstance(inp[1], basestring):
ra, dec = x_r.stod1((inp[1], inp[2]))
ira_tab['RA'] = ra
ira_tab['DEC'] = dec
elif isinstance(inp[1], float):
ira_tab['RA'] = inp[1] * astrou.deg
ira_tab['DEC'] = inp[2] * astrou.deg
elif isinstance(inp[1], SkyCoord):
ira_tab['RA'] = inp[1].ra.deg
ira_tab['DEC'] = inp[1].dec.deg
else: # Should check it is a Quantity
ira_tab['RA'] = inp[1]
ira_tab['DEC'] = inp[2]
# Strings
ras, decs = x_r.dtos1((ira_tab['RA'], ira_tab['DEC']))
ira_tab['RAS'] = ras
ira_tab['DECS'] = decs
# Make a list
ra_tab = [ira_tab]
# Grab ra, dec in decimal degrees
if deci is not None:
return
#xdb.set_trace()
#x_r.stod(ra_tab) #ra_tab['RA'][q], ra_tab['DEC'][q], TABL)
# Precess (as necessary)
if EPOCH > 1000.:
from astropy import units as u
from astropy.coordinates import FK5
from astropy.time import Time
# Precess to 2000.
tEPOCH = Time(EPOCH, format='jyear', scale='utc')
# Load into astropy
fk5c = FK5(ra=ra_tab['RA'],
dec=ra_tab['DEC'],
equinox=tEPOCH,
unit=(u.degree, u.degree))
# Precess
newEPOCH = Time(2000., format='jyear', scale='utc')
newfk5 = fk5c.precess_to(newEPOCH)
# Save
ra_tab['RA'] = newfk5.ra.degree
ra_tab['DEC'] = newfk5.dec.degree
# Strings too?
ra_tab['RAS'] = str(newfk5.ra.to_string(unit=u.hour, sep=':'))
ra_tab['DECS'] = str(newfk5.dec.to_string(unit=u.hour, sep=':'))
##
# Main Loop
for obj in ra_tab:
# Outfil
nm = "".join(obj['Name'].split())
if OUT_TYPE == 'PNG':
outfil = fpath + nm + '.png'
else:
outfil = fpath + nm + '.pdf'
print(outfil)
# Grab the Image
reload(xgs)
img, oBW = xgs.getimg(obj['RA'], obj['DEC'], imsize, BW=BW, DSS=DSS)
# Generate the plot
plt.clf()
fig = plt.figure(dpi=1200)
fig.set_size_inches(8.0, 10.5)
# Font
plt.rcParams['font.family'] = 'times new roman'
ticks_font = matplotlib.font_manager.FontProperties(
family='times new roman',
style='normal',
size=16,
weight='normal',
stretch='normal')
ax = plt.gca()
for label in ax.get_yticklabels():
label.set_fontproperties(ticks_font)
for label in ax.get_xticklabels():
label.set_fontproperties(ticks_font)
# Image
if oBW == 1:
cmm = cm.Greys_r
else:
cmm = None
plt.imshow(img,
cmap=cmm,
aspect='equal',
extent=(-imsize / 2., imsize / 2, -imsize / 2., imsize / 2))
# Axes
plt.xlim(-imsize / 2., imsize / 2.)
plt.ylim(-imsize / 2., imsize / 2.)
# Label
plt.xlabel('Relative ArcMin', fontsize=20)
xpos = 0.12 * imsize
ypos = 0.02 * imsize
plt.text(-imsize / 2. - xpos, 0., 'EAST', rotation=90., fontsize=20)
plt.text(0.,
imsize / 2. + ypos,
'NORTH',
fontsize=20,
horizontalalignment='center')
#import pdb; pdb.set_trace()
# Circle
if show_circ:
circle = plt.Circle((0, 0), cradius, color='y', fill=False)
plt.gca().add_artist(circle)
# Second Circle
if show_another is not None:
# Coordinates
cobj = x_r.to_coord((obj['RA'], obj['DEC']))
canother = x_r.to_coord(show_another)
# Offsets
off, PA = x_r.offsets(cobj, canother)
xanother = -1 * off[0].to('arcmin').value
yanother = off[1].to('arcmin').value
square = matplotlib.patches.Rectangle(
(xanother - cradius, yanother - cradius),
cradius * 2,
cradius * 2,
color='cyan',
fill=False)
plt.gca().add_artist(square)
plt.text(0.5,
1.24,
str(nm),
fontsize=32,
horizontalalignment='center',
transform=ax.transAxes)
plt.text(0.5,
1.18,
'RA (J2000) = ' + str(obj['RAS']) + ' DEC (J2000) = ' +
str(obj['DECS']),
fontsize=22,
horizontalalignment='center',
transform=ax.transAxes)
plt.text(0.5,
1.12,
'RA(offset) = {:s} DEC(offset) = {:s}'.format(
canother.ra.to_string(unit=astrou.hour,
pad=True,
sep=':',
precision=2),
canother.dec.to_string(pad=True,
alwayssign=True,
sep=':',
precision=1)),
fontsize=22,
horizontalalignment='center',
transform=ax.transAxes,
color='blue')
plt.text(
0.5,
1.06,
'RA(offset to obj) = {:g} DEC(offset to obj) = {:g}'.format(
-1 * off[0].to('arcsec'), -1 * off[1].to('arcsec')),
fontsize=18,
horizontalalignment='center',
transform=ax.transAxes)
else:
# Title
plt.text(0.5,
1.24,
str(nm),
fontsize=32,
horizontalalignment='center',
transform=ax.transAxes)
plt.text(0.5,
1.16,
'RA (J2000) = ' + str(obj['RAS']),
fontsize=28,
horizontalalignment='center',
transform=ax.transAxes)
plt.text(0.5,
1.10,
'DEC (J2000) = ' + str(obj['DECS']),
fontsize=28,
horizontalalignment='center',
transform=ax.transAxes)
# Spectrum??
if show_spec:
spec_img = xgs.get_spec_img(obj['RA'], obj['DEC'])
plt.imshow(spec_img,
extent=(-imsize / 2.1, imsize * (-0.1), -imsize / 2.1,
imsize * (-0.2)))
# Write
if show_spec:
plt.savefig(outfil, dpi=300)
else:
plt.savefig(outfil)
print 'finder: Wrote ' + outfil
plt.close()
#xdb.set_trace()
print 'finder: All done.'
return oBW
def mmt_targets(field, path=None):
"""Read files related to MMT targets
Parameters:
-----------
field: tuple
(Name, ra, dec)
Returns:
----------
Target and observing info
"""
if path is None:
path = "/Galx_Spectra/MMT/"
# Targets
targ_path = field[0] + path
# Target file
targ_file = glob.glob(targ_path + "*.targ")
if len(targ_file) != 1:
raise ValueError("Wrong number of MMT target files")
else:
targ_file = targ_file[0]
# Read PI, program info [NOT IMPLEMENTED]
# f = open(msk_file, 'r')
# lines = f.readlines()
# f.close()
# Read target table
tab = ascii.read(targ_file, comment="#")
# Restrict to targets
itarg = np.where(tab["type"] == "TARGET")
targs = tab[itarg]
# Polish
nrow = len(targs)
targs.rename_column("ra", "RAS")
targs.rename_column("dec", "DECS")
targs.add_column(Column([0.0] * nrow, name="TARG_RA"))
targs.add_column(Column([0.0] * nrow, name="TARG_DEC"))
# Get RA/DEC in degrees
for k, row in enumerate(targs):
rad, decd = xra.stod1((row["RAS"], row["DECS"]))
targs[k]["TARG_RA"] = rad.value
targs[k]["TARG_DEC"] = decd.value
targs.rename_column("objid", "TARG_ID")
targs.rename_column("mag", "TARG_MAG")
targs.add_column(Column([0.0] * nrow, name="EPOCH"))
targs.add_column(Column(["SDSS"] * nrow, name="TARG_IMG"))
targs.add_column(Column(["HECTOSPEC"] * nrow, name="INSTR"))
targ_mask = {}
cnames = ["MASK_NAME", "MASK_ID"]
smsk = "--"
msk_val = [smsk] * len(cnames)
for kk, cname in enumerate(cnames):
targ_mask[cname] = [msk_val[kk]] * nrow
# Now the 'mask' files
mask_files = glob.glob(targ_path + "*.cat")
all_obs = []
all_masks = []
for mask_file in mask_files:
print("Reading MMT mask file: {:s}".format(mask_file))
i0 = mask_file.rfind("/")
mask_nm = mask_file[i0 + 1 : mask_file.find(".cat")]
# Grab info from spectrum file
# xdb.set_trace()
spec_fil = glob.glob(mask_file[: i0 + 1] + "spHect-" + mask_nm + "*.fits.gz")
if len(spec_fil) != 1:
print("spec_fil -- Not found!".format(spec_fil))
ras, decs = xra.dtos1((field[1], field[2]))
pa = 0.0
else:
header = fits.open(spec_fil[0])[0].header
if header["APERTURE"] != mask_nm:
raise ValueError("Mask doesnt match!")
pa = header["POSANGLE"]
ras = header["CAT-RA"]
decs = header["CAT-DEC"]
# Continuing
mask_dict = dict(
INSTR="HECTOSPEC", MASK_NAME=mask_nm, MASK_RA=ras, MASK_DEC=decs, MASK_EPOCH=2000.0, MASK_PA=pa
) # SHOULD GRAB PA, RA, DEC FROM SPECTRA FITS HEADER
all_masks.append(mask_dict)
# Read obs
f = open(mask_file, "r")
lines = f.readlines()
f.close()
iall_obs = []
for line in lines:
if "OBS" in line:
prs = line.strip().split(" ")
gdprs = [iprs for iprs in prs if len(iprs) > 0]
obs_dict = {}
obs_dict["DATE"] = gdprs[2]
obs_dict["TEXP"] = float(gdprs[3])
obs_dict["DISPERSER"] = gdprs[4]
obs_dict["CONDITIONS"] = gdprs[5]
#
iall_obs.append(obs_dict)
obs_tab = xxul.dict_list_to_table(iall_obs)
obs_tab["TEXP"].unit = u.s
# Read observed targets
obs_targ = ascii.read(mask_file, comment="#")
gdt = np.where(obs_targ["flag"] == 1)[0]
for gdi in gdt:
mtt = np.where(targs["TARG_ID"] == int(obs_targ["objid"][gdi]))[0]
if len(mtt) != 1:
raise ValueError("Multiple matches?!")
targ_mask["MASK_NAME"][mtt[0]] = mask_nm
all_obs.append(obs_tab)
# Finish
mask = np.array([False] * len(targs))
bad = np.where(np.array(targ_mask["names"]) == "--")[0]
if len(bad) > 0:
mask[bad] = True
#
clm = MaskedColumn(targ_mask["names"], name="MASK_NAME", mask=mask)
targs.add_column(clm)
return all_masks, all_obs, targs
def main(inp,
survey='2r',
radec=None,
deci=None,
fpath=None,
EPOCH=0.,
DSS=None,
BW=False,
imsize=5.,
show_spec=False):
'''
Parameters:
---------
inp: Input
string or List of strings or List of several items
'ra_dec_list.txt' -- ASCII file with columns of Name,RA,DEC and RA,DEC are string or float (deg)
['NAME_OF_TARG', '10:31:38.87', '+25:59:02.3']
['NAME_OF_TARG', 124.24*u.deg, -23.244*u.deg]
radec: integer (0) [DEPRECATED!]
Flag indicating type of input
0 = ASCII file with columns of Name,RA,DEC and RA,DEC are string or float (deg)
1 = List of string ['Name', 'RA', 'DEC']
2 = ['Name', ra_deg, dec_deg]
BW: bool (False)
B&W image?
show_spec: bool (False)
Try to grab and show an SDSS spectrum
imsize: float
Image size in arcmin
'''
reload(x_r)
reload(xgs)
import matplotlib.pyplot as plt
import matplotlib.cm as cm
# Init
if fpath is None:
fpath = './'
cradius = imsize / 50.
# Read in the Target list
if isinstance(inp, basestring):
ra_tab = get_coord(targ_file, radec=radec)
else:
ira_tab = {}
ira_tab['Name'] = inp[0]
if isinstance(inp[1], basestring):
ra, dec = x_r.stod1((inp[1], inp[2]))
ira_tab['RA'] = ra
ira_tab['DEC'] = dec
elif isinstance(inp[1], float):
ira_tab['RA'] = inp[1] * astrou.deg
ira_tab['DEC'] = inp[2] * astrou.deg
else: # Should check it is a Quantity
ira_tab['RA'] = inp[1]
ira_tab['DEC'] = inp[2]
# Strings
ras, decs = x_r.dtos1((ira_tab['RA'], ira_tab['DEC']))
ira_tab['RAS'] = ras
ira_tab['DECS'] = decs
# Make a list
ra_tab = [ira_tab]
# Grab ra, dec in decimal degrees
if deci is not None:
return
#xdb.set_trace()
#x_r.stod(ra_tab) #ra_tab['RA'][q], ra_tab['DEC'][q], TABL)
# Precess (as necessary)
if EPOCH > 1000.:
from astropy import units as u
from astropy.coordinates import FK5
from astropy.time import Time
# Precess to 2000.
tEPOCH = Time(EPOCH, format='jyear', scale='utc')
# Load into astropy
fk5c = FK5(ra=ra_tab['RA'],
dec=ra_tab['DEC'],
equinox=tEPOCH,
unit=(u.degree, u.degree))
# Precess
newEPOCH = Time(2000., format='jyear', scale='utc')
newfk5 = fk5c.precess_to(newEPOCH)
# Save
ra_tab['RA'] = newfk5.ra.degree
ra_tab['DEC'] = newfk5.dec.degree
# Strings too?
ra_tab['RAS'] = str(newfk5.ra.to_string(unit=u.hour, sep=':'))
ra_tab['DECS'] = str(newfk5.dec.to_string(unit=u.hour, sep=':'))
##
# Main Loop
for obj in ra_tab:
# Outfil
nm = "".join(obj['Name'].split())
outfil = fpath + nm + '.pdf'
print(outfil)
# Grab the Image
reload(xgs)
img, oBW = xgs.getimg(obj['RA'], obj['DEC'], imsize, BW=BW, DSS=DSS)
# Generate the plot
plt.clf()
fig = plt.figure(dpi=1200)
fig.set_size_inches(8.0, 10.5)
# Font
plt.rcParams['font.family'] = 'times new roman'
ticks_font = matplotlib.font_manager.FontProperties(
family='times new roman',
style='normal',
size=16,
weight='normal',
stretch='normal')
ax = plt.gca()
for label in ax.get_yticklabels():
label.set_fontproperties(ticks_font)
for label in ax.get_xticklabels():
label.set_fontproperties(ticks_font)
# Image
if oBW == 1:
cmm = cm.Greys_r
else:
cmm = None
plt.imshow(img,
cmap=cmm,
aspect='equal',
extent=(-imsize / 2., imsize / 2, -imsize / 2., imsize / 2))
# Axes
plt.xlim(-imsize / 2., imsize / 2.)
plt.ylim(-imsize / 2., imsize / 2.)
# Label
plt.xlabel('Relative ArcMin', fontsize=20)
xpos = 0.12 * imsize
ypos = 0.02 * imsize
plt.text(-imsize / 2. - xpos, 0., 'EAST', rotation=90., fontsize=20)
plt.text(0.,
imsize / 2. + ypos,
'NORTH',
fontsize=20,
horizontalalignment='center')
# Title
plt.text(0.5,
1.24,
str(nm),
fontsize=32,
horizontalalignment='center',
transform=ax.transAxes)
plt.text(0.5,
1.16,
'RA (J2000) = ' + str(obj['RAS']),
fontsize=28,
horizontalalignment='center',
transform=ax.transAxes)
plt.text(0.5,
1.10,
'DEC (J2000) = ' + str(obj['DECS']),
fontsize=28,
horizontalalignment='center',
transform=ax.transAxes)
#import pdb; pdb.set_trace()
# Circle
circle = plt.Circle((0, 0), cradius, color='y', fill=False)
plt.gca().add_artist(circle)
# Spectrum??
if show_spec:
spec_img = xgs.get_spec_img(obj['RA'], obj['DEC'])
plt.imshow(spec_img,
extent=(-imsize / 2.1, imsize * (-0.1), -imsize / 2.1,
imsize * (-0.2)))
# Write
if show_spec:
plt.savefig(outfil, dpi=300)
else:
plt.savefig(outfil)
print 'finder: Wrote ' + outfil
#xdb.set_trace()
print 'finder: All done.'
return oBW
