“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)  | 
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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)