/usr/lib/python/astrometry/sdss/dr8.py is in astrometry.net 0.46-0ubuntu2.
This file is owned by root:root, with mode 0o644.
The actual contents of the file can be viewed below.
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 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176 177 178 179 180 181 182 183 184 185 186 187 188 189 190 191 192 193 194 195 196 197 198 199 200 201 202 203 204 205 206 207 208 209 210 211 212 213 214 215 216 217 218 219 220 221 222 223 224 225 226 227 228 229 230 231 232 233 234 235 236 237 238 239 240 241 242 243 244 245 246 247 248 249 250 251 252 253 254 255 256 257 258 259 260 261 262 263 264 265 266 267 268 269 270 271 272 273 274 275 276 277 278 279 280 281 282 283 284 285 286 287 288 289 290 291 292 293 294 295 296 297 298 299 300 301 302 303 304 305 306 307 308 309 310 311 312 313 314 315 316 317 318 319 320 321 322 323 324 325 326 327 328 329 330 331 332 333 334 335 336 337 338 339 340 341 342 343 344 345 346 347 348 349 350 351 352 353 354 355 356 357 358 359 360 361 362 363 364 365 366 367 368 369 370 371 372 373 374 375 376 377 378 379 380 381 382 383 384 385 386 387 388 389 390 391 392 393 394 395 396 397 398 399 400 401 402 403 404 405 406 407 408 409 410 411 412 413 414 415 416 417 418 419 420 421 422 423 424 425 426 427 428 429 430 431 432 433 434 435 436 437 438 439 440 441 | import os
from astrometry.util.fits import fits_table
import numpy as np
import logging
import urlparse
import tempfile
fitsio = None
try:
import fitsio
except:
import pyfits
from common import *
from dr7 import *
from astrometry.util.yanny import *
from astrometry.util.run_command import run_command
class Frame(SdssFile):
def __init__(self, *args, **kwargs):
super(Frame, self).__init__(*args, **kwargs)
self.filetype = 'frame'
self.image = None
self.image_proxy = None
def getImageShape(self):
if self.image_proxy is not None:
# fitsio fits.FITSHDU object
H,W = self.image_proxy.get_info()['dims']
H = int(H)
W = int(W)
else:
H,W = self.image.shape
return H,W
def getImageSlice(self, slice):
if self.image_proxy is not None:
#print 'reading slice from image proxy:', slice
return self.image_proxy[slice]
return self.image[slice]
#def __str__(self):
def getImage(self):
if self.image is None and self.image_proxy is not None:
self.image = self.image_proxy.read()
self.image_proxy = None
return self.image
def getHeader(self):
return self.header
def getAsTrans(self):
return self.astrans
def getCalibVec(self):
return self.calib
def getSkyAt(self, x, y):
skyim = self.sky
(sh,sw) = skyim.shape
if sw != 256:
skyim = skyim.T
(sh,sw) = skyim.shape
xi = np.round(self.skyxi[x]).astype(int)
yi = np.round(self.skyyi[y]).astype(int)
yi = np.minimum(yi,sh-1)
return skyim[yi,xi]
def getSky(self):
skyim = self.sky
(sh,sw) = skyim.shape
if sw != 256:
skyim = skyim.T
(sh,sw) = skyim.shape
xi = np.round(self.skyxi).astype(int)
yi = np.round(self.skyyi).astype(int)
yi = np.minimum(yi,sh-1)
assert(all(xi >= 0) and all(xi < sw))
assert(all(yi >= 0) and all(yi < sh))
XI,YI = np.meshgrid(xi, yi)
# Nearest-neighbour interpolation -- we just need this
# for approximate invvar.
bigsky = skyim[YI,XI]
return bigsky
def getInvvar(self, psfield, bandnum, ignoreSourceFlux=False,
sourceFlux=None, constantSkyAt=None):
'''
If constantSkyAt = (x,y) (INTEGERS!),
returns a scalar (rather than a np.array) of the invvar at that point.
NOTE that this does NOT blank out masked pixels; use, eg,
fpM = sdss.readFpM(run, camcol, field, bandname)
for plane in [ 'INTERP', 'SATUR', 'CR', 'GHOST' ]:
fpM.setMaskedPixels(plane, invvar, 0, roi=roi)
'''
calibvec = self.getCalibVec()
if constantSkyAt:
x,y = constantSkyAt
calibvec = calibvec[x]
sky = self.getSkyAt(x,y)
if ignoreSourceFlux:
dn = sky
elif sourceFlux is None:
image = self.getImage()
dn = (image[y,x] / calibvec) + sky
else:
dn = (sourceFlux / calibvec) + sky
else:
bigsky = self.getSky()
if ignoreSourceFlux:
dn = bigsky
elif sourceFlux is None:
image = self.getImage()
dn = (image / calibvec) + bigsky
else:
dn = (sourceFlux / calibvec) + bigsky
gain = psfield.getGain(bandnum)
# Note, "darkvar" includes dark current *and* read noise.
darkvar = psfield.getDarkVariance(bandnum)
dnvar = (dn / gain) + darkvar
invvar = 1./(dnvar * calibvec**2)
return invvar
class PhotoObj(SdssFile):
def __init__(self, *args, **kwargs):
super(PhotoObj, self).__init__(*args, **kwargs)
self.filetype = 'photoObj'
self.table = None
def getTable(self):
return self.table
class runlist(object):
pass
class DR8(DR7):
_lup_to_mag_b = np.array([1.4e-10, 0.9e-10, 1.2e-10, 1.8e-10, 7.4e-10])
_two_lup_to_mag_b = 2.*_lup_to_mag_b
_ln_lup_to_mag_b = np.log(_lup_to_mag_b)
'''
From
http://data.sdss3.org/datamodel/glossary.html#asinh
m = -(2.5/ln(10))*[asinh(f/2b)+ln(b)].
The parameter b is a softening parameter measured in maggies, and
for the [u, g, r, i, z] bands has the values
[1.4, 0.9, 1.2, 1.8, 7.4] x 1e-10
'''
@staticmethod
def luptitude_to_mag(Lmag, bandnum, badmag=25):
if bandnum is None:
# assume Lmag is broadcastable to a 5-vector
twobi = DR8._two_lup_to_mag_b
lnbi = DR8._ln_lup_to_mag_b
else:
twobi = DR8._two_lup_to_mag_b[bandnum]
lnbi = DR8._ln_lup_to_mag_b[bandnum]
# MAGIC -1.08.... = -2.5/np.log(10.)
f = np.sinh(Lmag/-1.0857362047581294 - lnbi) * twobi
# prevent log10(-flux)
mag = np.zeros_like(f) + badmag
I = (f > 0)
mag[I] = -2.5 * np.log10(f[I])
return mag
@staticmethod
def nmgy_to_mag(nmgy):
return 22.5 - 2.5 * np.log10(nmgy)
def getDRNumber(self):
return 8
def useLocalTree(self):
pobj = os.environ['BOSS_PHOTOOBJ']
redux = os.environ['PHOTO_REDUX']
self.filenames.update(
photoObj = os.path.join(pobj, '%(rerun)s', '%(run)i', '%(camcol)i',
'photoObj-%(run)06i-%(camcol)i-%(field)04i.fits'),
frame = os.path.join(pobj, 'frames', '%(rerun)s', '%(run)i', '%(camcol)i',
'frame-%(band)s-%(run)06i-%(camcol)i-%(field)04i.fits.bz2'),
psField = os.path.join(redux, '%(rerun)s', '%(run)i', 'objcs', '%(camcol)i',
'psField-%(run)06i-%(camcol)i-%(field)04i.fit'),
fpM = os.path.join(redux, '%(rerun)s', '%(run)i', 'objcs', '%(camcol)i',
'fpM-%(run)06i-%(band)s%(camcol)i-%(field)04i.fit.gz'),
)
def saveUnzippedFiles(self, basedir):
self.unzip_dir = basedir
def __init__(self, **kwargs):
'''
Useful kwargs:
basedir : (string) - local directory where data will be stored.
'''
DR7.__init__(self, **kwargs)
self.unzip_dir = None
# Local filenames
self.filenames.update({
'frame': 'frame-%(band)s-%(run)06i-%(camcol)i-%(field)04i.fits',
'idR': 'idR-%(run)06i-%(band)s-%(camcol)i-%(field)04i.fits',
'photoObj': 'photoObj-%(run)06i-%(camcol)i-%(field)04i.fits',
'photoField': 'photoField-%(run)06i-%(camcol)i.fits',
})
# URLs on DAS server
self.dasurl = 'http://data.sdss3.org/sas/dr8/groups/boss/'
self.daspaths = {
'idR': 'photo/data/%(run)i/fields/%(camcol)i/idR-%(run)06i-%(band)s%(camcol)i-%(field)04i.fit.Z',
'fpObjc': 'photo/redux/%(rerun)s/%(run)i/objcs/%(camcol)i/fpObjc-%(run)06i-%(camcol)i-%(field)04i.fit',
# DR8 frames are no longer available on DAS.
'frame': '/sas/dr9/boss/photoObj/frames/%(rerun)s/%(run)i/%(camcol)i/frame-%(band)s-%(run)06i-%(camcol)i-%(field)04i.fits.bz2',
#'frame': 'photoObj/frames/%(rerun)s/%(run)i/%(camcol)i/frame-%(band)s-%(run)06i-%(camcol)i-%(field)04i.fits.bz2',
'photoObj': 'photoObj/%(rerun)s/%(run)i/%(camcol)i/photoObj-%(run)06i-%(camcol)i-%(field)04i.fits',
'psField': 'photo/redux/%(rerun)s/%(run)i/objcs/%(camcol)i/psField-%(run)06i-%(camcol)i-%(field)04i.fit',
'photoField': 'photoObj/%(rerun)s/%(run)i/photoField-%(run)06i-%(camcol)i.fits',
'fpM': 'photo/redux/%(rerun)s/%(run)i/objcs/%(camcol)i/fpM-%(run)06i-%(band)s%(camcol)i-%(field)04i.fit.gz',
'fpAtlas': 'photo/redux/%(rerun)s/%(run)i/objcs/%(camcol)i/fpAtlas-%(run)06i-%(camcol)i-%(field)04i.fit',
}
self.dassuffix = {
'frame': '.bz2',
'fpM': '.gz',
'idR': '.Z',
}
self.processcmds = {
'frame': 'bunzip2 -cd %(input)s > %(output)s.tmp && mv %(output)s.tmp %(output)s',
'fpM': 'gunzip -cd %(input)s > %(output)s',
'idR': 'gunzip -cd %(input)s > %(output)s',
}
y = read_yanny(self._get_runlist_filename())
y = y['RUNDATA']
rl = runlist()
rl.run = np.array(y['run'])
rl.startfield = np.array(y['startfield'])
rl.endfield = np.array(y['endfield'])
rl.rerun = np.array(y['rerun'])
#print 'Rerun type:', type(rl.rerun), rl.rerun.dtype
self.runlist = rl
self.logger = logging.getLogger('astrometry.sdss.DR%i' %
self.getDRNumber())
#self.logger.debug('debug test')
#self.logger.info('info test')
#self.logger.warning('warning test')
def _get_runlist_filename(self):
return self._get_data_file('runList-dr8.par')
# read a data file describing the DR8 data
def _get_data_file(self, fn):
return os.path.join(os.path.dirname(__file__), fn)
def get_rerun(self, run, field=None):
I = (self.runlist.run == run)
if field is not None:
I *= (self.runlist.startfield <= field) * (self.runlist.endfield >= field)
I = np.flatnonzero(I)
reruns = np.unique(self.runlist.rerun[I])
#OBprint 'Reruns:', reruns
if len(reruns) == 0:
return None
return reruns[-1]
def get_url(self, filetype, run, camcol, field, band=None):
rerun = self.get_rerun(run, field)
path = self.daspaths[filetype]
url = urlparse.urljoin(self.dasurl, path % dict(
run=run, camcol=camcol, field=field, rerun=rerun, band=band))
return url
def retrieve(self, filetype, run, camcol, field=None, band=None, skipExisting=True,
tempsuffix='.tmp'):
outfn = self.getPath(filetype, run, camcol, field, band)
if outfn is None:
return None
if skipExisting and os.path.exists(outfn):
return outfn
print 'Did not find file:', outfn
url = self.get_url(filetype, run, camcol, field, band=band)
#print 'URL:', url
if self.curl:
cmd = "curl -o '%(outfn)s' '%(url)s'"
else:
cmd = "wget --continue -nv -O %(outfn)s '%(url)s'"
# suffix to add to the downloaded filename
suff = self.dassuffix.get(filetype, '')
oo = outfn + suff
if tempsuffix is not None:
oo += tempsuffix
cmd = cmd % dict(outfn=oo, url=url)
self.logger.debug('cmd: %s' % cmd)
(rtn,out,err) = run_command(cmd)
if rtn:
print 'Command failed: command', cmd
print 'Output:', out
print 'Error:', err
print 'Return val:', rtn
return None
if tempsuffix is not None:
#
os.rename(oo, outfn + suff)
if filetype in self.processcmds:
cmd = self.processcmds[filetype]
cmd = cmd % dict(input = outfn + suff, output = outfn)
self.logger.debug('cmd: %s' % cmd)
(rtn,out,err) = run_command(cmd)
if rtn:
print 'Command failed: command', cmd
print 'Output:', out
print 'Error:', err
print 'Return val:', rtn
return None
return outfn
def readPhotoObj(self, run, camcol, field, filename=None):
obj = PhotoObj(run, camcol, field)
if filename is None:
fn = self.getPath('photoObj', run, camcol, field)
else:
fn = filename
obj.table = fits_table(fn)
return obj
def readFrame(self, run, camcol, field, band, filename=None):
'''
http://data.sdss3.org/datamodel/files/BOSS_PHOTOOBJ/frames/RERUN/RUN/CAMCOL/frame.html
'''
f = Frame(run, camcol, field, band)
# ...
if filename is None:
fn = self.getPath('frame', run, camcol, field, band)
else:
fn = filename
#print 'reading file', fn
if fitsio:
print 'Frame filename', fn
# eg /clusterfs/riemann/raid006/dr10/boss/photoObj/frames/301/2825/1/frame-u-002825-1-0126.fits.bz2
tempfn = None
keep = False
cmd = None
# bunzip2
filetype = 'frame'
if filetype in self.processcmds:
cmd = self.processcmds[filetype]
if cmd is not None and self.unzip_dir is not None:
udir = os.path.join(self.unzip_dir, '%i' % run, '%i' % camcol)
if not os.path.exists(udir):
try:
os.makedirs(udir)
except:
pass
tempfn = os.path.join(udir, os.path.basename(fn).replace('.bz2', ''))
#print 'Checking', tempfn
if os.path.exists(tempfn):
print 'File exists:', tempfn
fn = tempfn
cmd = None
else:
print 'Saving to', tempfn
keep = True
elif cmd is not None and self.unzip_dir is None:
fid,tempfn = tempfile.mkstemp()
os.close(fid)
if cmd is not None:
cmd = cmd % dict(input = fn, output = tempfn)
self.logger.debug('cmd: %s' % cmd)
(rtn,out,err) = run_command(cmd)
if rtn:
print 'Command failed: command', cmd
print 'Output:', out
print 'Error:', err
print 'Return val:', rtn
return None
fn = tempfn
#f.image, f.header = fitsio.read(fn, header=True)
#print 'Reading header...'
f.header = fitsio.read_header(fn, 0)
#print 'Reading image HDU...'
# Allow later reading of just the ROI slice...
f.image_proxy = fitsio.FITS(fn)[0]
f.calib = fitsio.read(fn, ext=1)
sky = fitsio.read(fn, ext=2, columns=['allsky', 'xinterp', 'yinterp'])
#print 'sky', type(sky)
# ... supposed to be a recarray, but it's not...
f.sky, f.skyxi, f.skyyi = sky.tolist()[0]
tab = fits_table(fn, hdu=3)
if not keep and tempfn is not None:
os.remove(tempfn)
else:
p = pyfits.open(fn)
# in nanomaggies
f.image = p[0].data
f.header = p[0].header
# converts counts -> nanomaggies
f.calib = p[1].data
# table with val,x,y -- binned; use bilinear interpolation to expand
sky = p[2].data
# table -- asTrans structure
tab = fits_table(p[3].data)
f.sky = sky.field('allsky')[0]
f.skyxi = sky.field('xinterp')[0]
f.skyyi = sky.field('yinterp')[0]
#print 'sky shape', f.sky.shape
if len(f.sky.shape) != 2:
f.sky = f.sky.reshape((-1, 256))
assert(len(tab) == 1)
tab = tab[0]
# DR7 has NODE, INCL in radians...
f.astrans = AsTrans(run, camcol, field, band,
node=np.deg2rad(tab.node), incl=np.deg2rad(tab.incl),
astrans=tab, cut_to_band=False)
return f
|