Parallax Class Family

class model.BSPL_noParallax

Bases: PSPL_noParallax

Methods

`get_amplification`(t)	noParallax: Get the photometric amplification term at a set of times, t.
`get_astrometry`(t_obs[, ast_filt_idx])	noParallax: Position of the observed source position in arcsec.
`get_astrometry_unlensed`(t_obs)	noParallax: Get the astrometry of the source if the lens didn't exist.
`get_centroid_shift`(t)	noParallax: Get the centroid shift (in mas) for a list of observation times (in MJD).
`get_lens_astrometry`(t_obs)	Equation of motion for just the foreground lens.
`get_resolved_amplification`(t)	Get the photometric amplification term at a set of times, t for both the plus and minus images.
`get_resolved_astrometry`(t_obs)	Get the x, y astrometry for each of the two source images, which we label plus and minus.

calc_piE_ecliptic

get_amplification(t)

noParallax: Get the photometric amplification term at a set of times, t.

Parameters

t:: Array of times in MJD.DDD

get_astrometry(t_obs, ast_filt_idx=0): noParallax: Position of the observed source position in arcsec.

get_astrometry_unlensed(t_obs)

noParallax: Get the astrometry of the source if the lens didn’t exist.

Returns

xS_unlensednumpy array, dtype=float, shape = len(t_obs) x 2: The unlensed positions of the source in arcseconds.

get_centroid_shift(t): noParallax: Get the centroid shift (in mas) for a list of observation times (in MJD).

get_lens_astrometry(t_obs)

Equation of motion for just the foreground lens.

Parameters

t_obsarray_like: Time (in MJD).

get_resolved_amplification(t)

Get the photometric amplification term at a set of times, t for both the plus and minus images.

Parameters

t:: Array of times in MJD.DDD

get_resolved_astrometry(t_obs)

Get the x, y astrometry for each of the two source images, which we label plus and minus.

Returns

[xS_plus, xS_minus]list of numpy arrays

xS_plus is the vector position of the plus image in arcsec
xS_minus is the vector position of the plus image in arcsec

class model.BSPL_Parallax

Bases: PSPL_Parallax

Methods

`calc_piE_ecliptic`()	Parallax: Get piE_ecliptic
`get_amplification`(t)	Parallax: Get the photometric amplification term at a set of times, t.
`get_astrometry`(t_obs[, ast_filt_idx])	Parallax: Get astrometry
`get_astrometry_unlensed`(t_obs)	Get the astrometry of the source if the lens didn't exist.
`get_centroid_shift`(t[, ast_filt_idx])	Parallax: Get the centroid shift (in mas) for a list of observation times (in MJD).
`get_geoproj_ast_params`(t0par)
`get_geoproj_params`(t0par)
`get_lens_astrometry`(t_obs)	Parallax: Get lens astrometry
`get_resolved_amplification`(t)	Parallax: Get the photometric amplification term at a set of times, t for both the plus and minus images.
`get_resolved_astrometry`(t_obs)	Parallax: Get the x, y astrometry for each of the two source images, which we label plus and minus.

start

calc_piE_ecliptic(): Parallax: Get piE_ecliptic

get_amplification(t)

Parallax: Get the photometric amplification term at a set of times, t.

Parameters

t:: Array of times in MJD.DDD

get_astrometry(t_obs, ast_filt_idx=0): Parallax: Get astrometry

get_astrometry_unlensed(t_obs)

Get the astrometry of the source if the lens didn’t exist.

Returns

xS_unlensednumpy array, dtype=float, shape = len(t_obs) x 2: The unlensed positions of the source in arcseconds.

get_centroid_shift(t, ast_filt_idx=0): Parallax: Get the centroid shift (in mas) for a list of observation times (in MJD).

get_lens_astrometry(t_obs): Parallax: Get lens astrometry

get_resolved_amplification(t)

Parallax: Get the photometric amplification term at a set of times, t for both the plus and minus images.

Parameters

t:: Array of times in MJD.DDD

get_resolved_astrometry(t_obs)

Parallax: Get the x, y astrometry for each of the two source images, which we label plus and minus.

Returns

[xS_plus, xS_minus]list of numpy arrays

xS_plus is the vector position of the plus image.
xS_minus is the vector position of the plus image.