FaucherSpiral#
- class gammapy.astro.population.FaucherSpiral[source]#
Bases:
gammapy.astro.population.spatial.LogSpiral
Milky way spiral arm used in Faucher et al (2006).
Reference: https://ui.adsabs.harvard.edu/abs/2006ApJ…643..332F
Attributes Summary
Methods Summary
__call__
(radius[, blur, random_state])Draw random position from spiral arm distribution.
radius
(theta, spiralarm_index)Radius for a given angle.
theta
(radius, spiralarm_index)Angle for a given radius.
xy_position
([theta, radius, spiralarm_index])Compute (x, y) position for a given angle or radius.
Attributes Documentation
- k = <Quantity [4.25, 4.25, 4.89, 4.89] rad>#
- r_0 = <Quantity [3.48, 3.48, 4.9 , 4.9 ] kpc>#
- spiralarms = array(['Norma', 'Carina Sagittarius', 'Perseus', 'Crux Scutum'], dtype='<U18')#
- theta_0 = <Quantity [1.57, 4.71, 4.09, 0.95] rad>#
Methods Documentation
- __call__(radius, blur=True, random_state='random-seed')[source]#
Draw random position from spiral arm distribution.
Returns the corresponding angle theta[rad] to a given radius[kpc] and number of spiral arm. Possible numbers are:
Norma = 0,
Carina Sagittarius = 1,
Perseus = 2
Crux Scutum = 3.
- Parameters
- random_state{int, ‘random-seed’, ‘global-rng’,
RandomState
} Defines random number generator initialisation. Passed to
get_random_state
. Default is ‘random-seed’.
- random_state{int, ‘random-seed’, ‘global-rng’,
- Returns
- Returns dx and dy, if blurring= true.
- radius(theta, spiralarm_index)#
Radius for a given angle.
- theta(radius, spiralarm_index)#
Angle for a given radius.
- xy_position(theta=None, radius=None, spiralarm_index=0)#
Compute (x, y) position for a given angle or radius.