“Astropy”的版本间差异
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(→宇宙学) |
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==宇宙学== |
==宇宙学== |
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http://docs.astropy.org/en/stable/cosmology/ |
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*从红移到年龄 |
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>>>from astropy.cosmology import FlatLambdaCDM |
>>>from astropy.cosmology import FlatLambdaCDM |
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>>>cosmo = FlatLambdaCDM(H0=70, Om0=0.3) |
>>>cosmo = FlatLambdaCDM(H0=70, Om0=0.3) |
2017年9月15日 (五) 14:18的版本
astropy.io.fits
>>> hdulist = fits.open('input.fits') >>> hdulist.info()
- 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')
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)