本文整理匯總了Python中MOSFIRE.IO.load_edges方法的典型用法代碼示例。如果您正苦於以下問題:Python IO.load_edges方法的具體用法?Python IO.load_edges怎麽用?Python IO.load_edges使用的例子?那麽, 這裏精選的方法代碼示例或許可以為您提供幫助。您也可以進一步了解該方法所在類MOSFIRE.IO
的用法示例。
在下文中一共展示了IO.load_edges方法的4個代碼示例,這些例子默認根據受歡迎程度排序。您可以為喜歡或者感覺有用的代碼點讚,您的評價將有助於係統推薦出更棒的Python代碼示例。
示例1: __init__
# 需要導入模塊: from MOSFIRE import IO [as 別名]
# 或者: from MOSFIRE.IO import load_edges [as 別名]
def __init__(self, maskname, bandname, options, fig):
self.fig = fig
self.flat = IO.read_drpfits(maskname, "combflat_2d_%s.fits" % bandname,
options)
self.edges, meta = IO.load_edges(maskname, bandname, options)
self.edgeno=2
self.cid = self.fig.canvas.mpl_connect('key_press_event', self)
self.draw()
示例2: rename_files
# 需要導入模塊: from MOSFIRE import IO [as 別名]
# 或者: from MOSFIRE.IO import load_edges [as 別名]
def rename_files(wavenames, maskname, band, wavops):
lamname = Wavelength.filelist_to_wavename(wavenames[0], band, maskname, wavops).rstrip(".fits")
suffix = lamname.lstrip("wave_stack_%s_" % band)
path = os.path.join(wavops["outdir"], maskname)
fnames = ["rectified_%s%s.fits", "rectified_ivar_%s%s.fits", "rectified_sn_%s%s.fits"]
for fname in fnames:
try:
a = get_path(os.path.join(path, fname % (band, "_" + suffix)))
b = os.path.join(path, fname % (band, "")) + gz(a)
os.rename(a, b)
except:
print "Ignoring renaming of: ", fname
pass
edges = IO.load_edges(maskname, band, wavops)
n_slits = len(edges[0])
for i in xrange(1, n_slits + 1):
S = "S%2.2i" % (i)
a = get_path(os.path.join(path, "eps_%s_%s_%s.fits" % (band, suffix, S)))
a_h = pf.open(a)[0].header
obj = a_h["object"]
b = os.path.join(path, "%s_%s_%s_eps.fits" % (maskname, band, obj)) + gz(a)
os.rename(a, b)
a = get_path(os.path.join(path, "ivar_%s_%s_%s.fits" % (band, suffix, S)))
a_h = pf.open(a)[0].header
obj = a_h["object"]
b = os.path.join(path, "%s_%s_%s_ivar.fits" % (maskname, band, obj)) + gz(a)
os.rename(a, b)
a = get_path(os.path.join(path, "eps_%s_%s_%s.fits" % (maskname, suffix, band)))
b = os.path.join(path, "%s_%s_eps.fits" % (maskname, band)) + gz(a)
os.rename(a, b)
a = get_path(os.path.join(path, "snrs_%s_%s_%s.fits" % (maskname, suffix, band)))
b = os.path.join(path, "%s_%s_snrs.fits" % (maskname, band)) + gz(a)
os.rename(a, b)
a = get_path(os.path.join(path, "ivars_%s_%s_%s.fits" % (maskname, suffix, band)))
b = os.path.join(path, "%s_%s_ivars.fits" % (maskname, band)) + gz(a)
os.rename(a, b)
示例3: handle_background
# 需要導入模塊: from MOSFIRE import IO [as 別名]
# 或者: from MOSFIRE.IO import load_edges [as 別名]
def handle_background(filelist, wavename, maskname, band_name, options, shifts=None, plan=None, extension=None):
'''
Perform difference imaging and subtract residual background.
The plan looks something like: [['A', 'B']]
In this case, the number of output files is equal to the length of the list (1).
If you choose to use an ABA'B' pattern then the plan will be: [["A", "B"], ["A'", "B'"]]
the background subtraction code will make and handle two files, "A-B" and "A'-B'".
'''
global header, bs, edges, data, Var, itime, lam, sky_sub_out, sky_model_out, band
band = band_name
flatname = "pixelflat_2d_%s.fits" % band_name
hdr, flat = IO.readfits("pixelflat_2d_%s.fits" % (band_name), options)
if np.abs(np.median(flat) - 1) > 0.1:
raise Exception("Flat seems poorly behaved.")
'''
This next section of the code figures out the observing plan
and then deals with the bookeeping of sending the plan
to the background subtracter.
'''
hdrs = []
epss = {}
vars = {}
bss = []
times = {}
Nframes = []
i = 0
header = pf.Header()
for i in xrange(len(filelist)):
fl = filelist[i]
files = IO.list_file_to_strings(fl)
print "Combining"
if shifts is None: shift = None
else: shift = shifts[i]
hdr, electron, var, bs, time, Nframe = imcombine(files, maskname,
options, flat, outname="%s.fits" % (fl),
shifts=shift, extension=extension)
hdrs.append(hdr)
header = merge_headers(header, hdr)
epss[hdr['FRAMEID']] = electron/time
vars[hdr['FRAMEID']] = var
times[hdr['FRAMEID']] = time
bss.append(bs)
Nframes.append(Nframe)
positions = {}
i = 0
for h in hdrs:
positions[h['FRAMEID']] = i
i += 1
posnames = set(positions.keys())
if plan is None:
plan = guess_plan_from_positions(posnames)
num_outputs = len(plan)
edges, meta = IO.load_edges(maskname, band, options)
lam = IO.readfits(wavename, options)
bs = bss[0]
for i in xrange(num_outputs):
posname0 = plan[i][0]
posname1 = plan[i][1]
print "Handling %s - %s" % (posname0, posname1)
data = epss[posname0] - epss[posname1]
Var = vars[posname0] + vars[posname1]
itime = np.mean([times[posname0], times[posname1]], axis=0)
p = Pool()
solutions = p.map(background_subtract_helper, xrange(len(bs.ssl)))
p.close()
write_outputs(solutions, itime, header, maskname, band, plan[i], options)
示例4: handle_rectification
# 需要導入模塊: from MOSFIRE import IO [as 別名]
# 或者: from MOSFIRE.IO import load_edges [as 別名]
def handle_rectification(maskname, in_files, wavename, band_pass, barset_file, options,
commissioning_shift=3.0):
'''Handle slit rectification and coaddition.
Args:
maskname: The mask name string
in_files: List of stacked spectra in electron per second. Will look
like ['electrons_Offset_1.5.txt.fits', 'electrons_Offset_-1.5.txt.fits']
wavename: path (relative or full) to the wavelength stack file, string
band_pass: Band pass name, string
barset_file: Path to a mosfire fits file containing the full set of
FITS extensions for the barset. It can be any file in the list
of science files.
Returns:
None
Writes files:
[maskname]_[band]_[object name]_eps.fits --
The rectified, background subtracted, stacked eps spectrum
[maskname]_[band]_[object name]_sig.fits --
Rectified, background subtracted, stacked weight spectrum (STD/itime)
[maskname]_[band]_[object_name]_itime.fits
Rectified, CRR stacked integration time spectrum
[maskname]_[band]_[object_name]_snrs.fits
Rectified signal to noise spectrum
'''
global edges, dats, vars, itimes, shifts, lambdas, band, fidl, all_shifts
band = band_pass
dlambda = Wavelength.grating_results(band)
hpp = Filters.hpp[band]
fidl = np.arange(hpp[0], hpp[1], dlambda)
lambdas = IO.readfits(wavename, options)
if np.any(lambdas[1].data < 0) or np.any(lambdas[1].data > 29000):
print "***********WARNING ***********"
print "The file {0} may not be a wavelength file.".format(wavename)
print "Check before proceeding."
print "***********WARNING ***********"
edges, meta = IO.load_edges(maskname, band, options)
shifts = []
posnames = []
postoshift = {}
for file in in_files:
print ":: ", file
II = IO.read_drpfits(maskname, file, options)
off = np.array((II[0]["decoff"], II[0]["raoff"]),dtype=np.float64)
if "yoffset" in II[0]:
off = -II[0]["yoffset"]
else:
# Deal with data taken during commissioning
if II[0]["frameid"] == 'A': off = 0.0
else: off = commissioning_shift
try: off0
except: off0 = off
shift = off - off0
shifts.append(shift)
posnames.append(II[0]["frameid"])
postoshift[II[0]['frameid']] = shift
print "Position {0} shift: {1:2.2f} as".format(off, shift)
plans = Background.guess_plan_from_positions(set(posnames))
all_shifts = []
for plan in plans:
to_append = []
for pos in plan:
to_append.append(postoshift[pos])
all_shifts.append(to_append)
# Reverse the elements in all_shifts to deal with an inversion
all_shifts.reverse()
theBPM = IO.badpixelmask()
all_solutions = []
cntr = 0
for plan in plans:
p0 = plan[0].replace("'", "p")
p1 = plan[1].replace("'", "p")
suffix = "%s-%s" % (p0,p1)
print "Handling plan %s" % suffix
fname = "bsub_{0}_{1}_{2}.fits".format(maskname,band,suffix)
EPS = IO.read_drpfits(maskname, fname, options)
EPS[1] = np.ma.masked_array(EPS[1], theBPM, fill_value=0)
#.........這裏部分代碼省略.........