Astropy

astropy.io.fits

[1]

>>> hdulist = fits.open('input.fits')
>>> hdulist.info()

header

• each element of an HDUList is an HDU object with .header and .data attributes, which can be used to access the header and data portions of the HDU.

>>> hdulist[0].header['targname']

• To see the entire header as it appears in the FITS file (with the END card and padding stripped), simply enter the header object by itself, or print(repr(header)):
• It’s also possible to view a slice of the header:

>>> header[:2]

• Another way to either update an existing card or append a new one is to use the Header.set() method:

>>> prihdr.set('observer', 'Edwin Hubble')

fits table 的读与写

• 写

from astropy.table import Table
t=Table([Bage,fzbin,Age_weight2],names=('Age','z','weights'))
t.write('SFH_LMC3_out.fits',format='fits')

• 读

hdu = fits.open('SFH_LMC3_out.fits')
hdu.info() #看看哪些hdu
data=hdu[1].data
data.columns #看看有那些列
Bage=data.field('Age')

astrometry

>>> from astropy.coordinates import SkyCoord >>> from astropy import units as u >>> c = SkyCoord(ra=ra1*u.degree, dec=dec1*u.degree) >>> catalog = SkyCoord(ra=ra2*u.degree, dec=dec2*u.degree) >>> idx, d2d, d3d = c.match_to_catalog_sky(catalog)

宇宙学

http://docs.astropy.org/en/stable/cosmology/

• 从红移到年龄

>>>from astropy.cosmology import FlatLambdaCDM 
>>>cosmo = FlatLambdaCDM(H0=70, Om0=0.3)

• 从年龄到红移

>>> import astropy.units as u
>>> from astropy.cosmology import  z_at_value
>>> z_at_value(cosmos.age, 2 * u.Gyr)