本文整理汇总了Python中astrodata.AstroData.detector_y_bin方法的典型用法代码示例。如果您正苦于以下问题:Python AstroData.detector_y_bin方法的具体用法?Python AstroData.detector_y_bin怎么用?Python AstroData.detector_y_bin使用的例子?那么恭喜您, 这里精选的方法代码示例或许可以为您提供帮助。您也可以进一步了解该方法所在类astrodata.AstroData
的用法示例。
在下文中一共展示了AstroData.detector_y_bin方法的3个代码示例,这些例子默认根据受欢迎程度排序。您可以为喜欢或者感觉有用的代码点赞,您的评价将有助于系统推荐出更棒的Python代码示例。
示例1: AstroData
# 需要导入模块: from astrodata import AstroData [as 别名]
# 或者: from astrodata.AstroData import detector_y_bin [as 别名]
import sys
sys.path.append("/opt/gemini_python")
from astrodata import AstroData
import urllib2, urllib
# This is a GMOS_N imaging science dataset
ad = AstroData("/home/callen/SVN-AD/gemini_python/test_data/calsearch/N20110531S0114.fits")
desc_dict = {'instrument':ad.instrument().for_db(),
'observation_type': ad.observation_type().for_db(),
'data_label':ad.data_label().for_db(),
'detector_x_bin':ad.detector_x_bin().for_db(),
'detector_y_bin':ad.detector_y_bin().for_db(),
'read_speed_setting':ad.read_speed_setting().for_db(),
'gain_setting':ad.gain_setting().for_db(),
'amp_read_area':ad.amp_read_area().for_db(),
'ut_datetime':ad.ut_datetime().for_db(),
'exposure_time':ad.exposure_time().for_db(),
'object': ad.object().for_db(),
'filter_name':ad.filter_name().for_db(),
'focal_plane_mask':ad.focal_plane_mask().for_db(),
}
print repr(desc_dict)
type_list = ad.types
ad.close()
sequence = [('descriptors', desc_dict), ('types', type_list)]
postdata = urllib.urlencode(sequence)
#postdata = urllib.urlencode({"hello":1.})
示例2: AcquisitionImage
# 需要导入模块: from astrodata import AstroData [as 别名]
# 或者: from astrodata.AstroData import detector_y_bin [as 别名]
class AcquisitionImage(object):
def __init__(self, filename, mosmask=None, mdfdir=None):
self.ad = AstroData(filename)
self.mosmask = mosmask
self.mdfdir = mdfdir
# Determine extension
nsci = len(self.ad)
debug("...nsci = ", nsci)
if nsci > 1:
l_sci_ext = 1
else:
l_sci_ext = 0
debug("...using extension [" + str(l_sci_ext) + "]")
overscan_dv = self.ad[l_sci_ext].overscan_section()
if self.is_mos_mode():
self.box_coords = parse_box_coords(self, self.get_mdf_filename())
self.box_mosaic = BoxMosaic(self, self.box_coords)
self.scidata = self.box_mosaic.get_science_data()
elif self.is_new_gmosn_ccd():
# tile the 2 center parts of the new GMOS image
self.scidata = gmultiamp(self.ad)
elif not overscan_dv.is_none():
# remove the overscan so we don't have to take it into account when guessing the slit location
self.scidata = subtract_overscan(self.ad[l_sci_ext])
# it still affects the center of rotation however
ox1, ox2, oy1, oy2 = overscan_dv.as_list()
correction = np.array([ox2 - ox1, 0])
center = self.get_binned_data_center() - correction
self.fieldcenter = center * self.detector_y_bin()
else:
self.scidata = self.ad[l_sci_ext].data
@cache
def instrument(self):
return str(self.ad.instrument())
def is_new_gmosn_ccd(self):
header = self.ad.phu.header
if "DETECTOR" not in header:
return False
if header["DETECTOR"] == "GMOS + e2v DD CCD42-90":
return True
return False
def get_science_data(self):
assert self.scidata is not None
return self.scidata
@cache
def unbinned_pixel_scale(self):
return float(self.ad.pixel_scale()) / self.detector_y_bin()
@cache
def binned_pixel_scale(self):
return float(self.ad.pixel_scale())
def _check_binning(self):
if int(self.ad.detector_x_bin()) != int(self.ad.detector_y_bin()):
error("ERROR: incorrect binning!")
error("Sorry about that, better luck next time.")
sys.exit(1)
@cache
def detector_x_bin(self):
self._check_binning()
return int(self.ad.detector_x_bin())
@cache
def detector_y_bin(self):
self._check_binning()
return int(self.ad.detector_y_bin())
@cache
def program_id(self):
return str(self.ad.program_id())
@cache
def observation_id(self):
return str(self.ad.observation_id())
@cache
def saturation_level(self):
dv = self.ad.saturation_level()
return min(dv.as_list())
@cache
def focal_plane_mask(self):
return str(self.ad.focal_plane_mask())
@cache
def grating(self):
return str(self.ad.grating())
#.........这里部分代码省略.........
示例3: AstroData
# 需要导入模块: from astrodata import AstroData [as 别名]
# 或者: from astrodata.AstroData import detector_y_bin [as 别名]
import sys, os
from astrodata import AstroData
from astrodata import Errors
import re
ad = AstroData("../../../test_data/recipedata/N20090703S0163.fits")
ybin = ad.detector_y_bin()
xbin = ad.detector_x_bin()
disp = ad.disperser()
descripts = ["airmass", "amp_read_area", "azimuth", "camera", "cass_rotator_pa",
"central_wavelength", "coadds", "data_label", "data_section", "dec", "decker",
"detector_section", "detector_x_bin", "detector_y_bin", "disperser",
"dispersion", "dispersion_axis", "elevation", "exposure_time", "filter_name",
"focal_plane_mask", "gain", "gain_setting", "grating", "instrument",
"local_time", "mdf_row_id", "nod_count", "nod_pixels", "non_linear_level",
"object", "observation_class", "observation_epoch", "observation_id",
"observation_type", "pixel_scale", "prism", "program_id", "pupil_mask",
"qa_state", "ra", "raw_bg", "raw_cc", "raw_iq", "raw_wv", "read_mode",
"read_noise", "read_speed_setting", "saturation_level", "slit", "telescope",
"ut_date", "ut_datetime", "ut_time", "wavefront_sensor",
"wavelength_reference_pixel", "well_depth_setting", "x_offset", "y_offset"]
descripts = ["detector_x_bin","exposure_time", "raw_cc"]
if True:
ops = ["+","-","*","/","//", "%", "**", "<<",">>", "^", "<", "<=", ">",">=","==",]
#ops = ["<", "<=", ">",">=","==",]
exprs = []
operands = ["'hello'", 10., 10]