我目前对 fit 文件有一点问题。数据是表格格式,这是我以前没有使用过的格式。我是一个 python 用户,并且严重依赖 astropy.fits 来操作 fit 图像。信息的快速输出给出:
No. Name Type Cards Dimensions Format
0 PRIMARY PrimaryHDU 60 ()
1 BinTableHDU 29 3072R x 2C [1024E, 1024E]
BinTableHDU 的标头如下:
XTENSION= 'BINTABLE' /Written by IDL: Mon Jun 22 23:28:21 2015
BITPIX = 8 /
NAXIS = 2 /Binary table
NAXIS1 = 8192 /Number of bytes per row
NAXIS2 = 3072 /Number of rows
PCOUNT = 0 /Random parameter count
GCOUNT = 1 /Group count
TFIELDS = 2 /Number of columns
TFORM1 = '1024E ' /Real*4 (floating point)
TFORM2 = '1024E ' /Real*4 (floating point)
TTYPE1 = 'COUNT_RATE' /
TUNIT1 = '1e-6cts/s/arcmin^2' /
TTYPE2 = 'UNCERTAINTY' /
TUNIT2 = '1e-6cts/s/arcmin^2' /
HISTORY g000m90r1b120pm.fits created on 10/08/97. PI channel range: 8: 19
PIXTYPE = 'HEALPIX ' / HEALPIX pixelisation
ORDERING= 'NESTED ' / Pixel ordering scheme, either RING or NESTED
NSIDE = 512 / Healpix resolution parameter
NPIX = 3145728 / Total number of pixels
OBJECT = 'FULLSKY ' / Sky coverage, either FULLSKY or PARTIAL
FIRSTPIX= 0 / First pixel # (0 based)
LASTPIX = 3145727 / Last pixel # (zero based)
INDXSCHM= 'IMPLICIT' / indexing : IMPLICIT or EXPLICIT
GRAIN = 0 / GRAIN = 0: No index,
COMMENT GRAIN =1: 1 pixel index for each pixel,
COMMENT GRAIN >1: 1 pixel index for Grain consecutive pixels
BAD_DATA= -1.63750E+30 / Sentinel value given to bad pixels
COORDSYS= 'G ' / Pixelization coordinate system
COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial
END
我想访问存储在标记为“计数率”的 TTYPE 中的拟合图像,然后将其设置为一种格式,然后我可以将其添加到具有相同尺寸的其他计数率数组中。
我从打开 fit 文件的常用程序开始:
hdulist_RASS_SXRB_R1 = fits.open('/Users/.../RASS_SXRB_R1.fits')
hdulist_RASS_SXRB_R1.info()
image_XRAY_SKYVIEW_R1 = hdulist_RASS_SXRB_R1[1].data
image_XRAY_SKYVIEW_R1 = numpy.array(image_XRAY_SKYVIEW_R1)
image_XRAY_SKYVIEW_header_R1 = hdulist_RASS_SXRB_R1[1].header
但这又回来了IndexError: too many indices for array
。我在此处的 astropy 文档中查看了访问表数据(Accessing data stored as a table in a multi-extension FITS (MEF) file)
如果有人有一种经过验证的方法可以从适合表中访问此类图像,我将不胜感激!非常感谢。