コード例 #1
0
ファイル: test_coords.py プロジェクト: jls713/galpy
def test_cov_dvrpmllbb_to_vxyz():
    l,b,d= 90., 0., 2.
    e_d, e_vr= 0.2, 2.
    cov_pmllpmbb= numpy.array([[100.,0.],[0.,400.]])
    pmll,pmbb= 20.,30.
    cov_vxvyvz= bovy_coords.cov_dvrpmllbb_to_vxyz(d,e_d,e_vr,
                                                  pmll,pmbb,
                                                  cov_pmllpmbb,
                                                  l,b,
                                                  degree=True,
                                                  plx=False)
    assert numpy.fabs(numpy.sqrt(cov_vxvyvz[0,0])
                      -d*4.74047*pmll*numpy.sqrt((e_d/d)**2.+(10./pmll)**2.)) < 10.**-10., 'cov_dvrpmllbb_to_vxyz coversion did not work as expected'
    assert numpy.fabs(numpy.sqrt(cov_vxvyvz[1,1])-e_vr) < 10.**-10., 'cov_dvrpmllbb_to_vxyz coversion did not work as expected'
    assert numpy.fabs(numpy.sqrt(cov_vxvyvz[2,2])
                      -d*4.74047*pmbb*numpy.sqrt((e_d/d)**2.+(20./pmbb)**2.)) < 10.**-10., 'cov_dvrpmllbb_to_vxyz coversion did not work as expected'
    #Another one
    l,b,d= 180., 0., 1./2.
    e_d, e_vr= 0.05, 2.
    cov_pmllpmbb= numpy.array([[100.,0.],[0.,400.]])
    pmll,pmbb= 20.,30.
    cov_vxvyvz= bovy_coords.cov_dvrpmllbb_to_vxyz(d,e_d,e_vr,
                                                  pmll,pmbb,
                                                  cov_pmllpmbb,
                                                  l/180.*numpy.pi,
                                                  b/180.*numpy.pi,
                                                  degree=False,
                                                  plx=True)
    assert numpy.fabs(numpy.sqrt(cov_vxvyvz[0,0])-e_vr) < 10.**-10., 'cov_dvrpmllbb_to_vxyz coversion did not work as expected'
    assert numpy.fabs(numpy.sqrt(cov_vxvyvz[1,1])
                      -1./d*4.74047*pmll*numpy.sqrt((e_d/d)**2.+(10./pmll)**2.)) < 10.**-10., 'cov_dvrpmllbb_to_vxyz coversion did not work as expected'
    assert numpy.fabs(numpy.sqrt(cov_vxvyvz[2,2])
                      -1./d*4.74047*pmbb*numpy.sqrt((e_d/d)**2.+(20./pmbb)**2.)) < 10.**-10., 'cov_dvrpmllbb_to_vxyz coversion did not work as expected'
    #Another one, w/ arrays
    l,b,d= 90., 90., 2.
    e_d, e_vr= 0.2, 2.
    tcov_pmllpmbb= numpy.array([[100.,0.],[0.,400.]])
    cov_pmllpmbb= numpy.empty((3,2,2))
    for ii in range(3): cov_pmllpmbb[ii,:,:]= tcov_pmllpmbb
    pmll,pmbb= 20.,30.
    os= numpy.ones(3)
    cov_vxvyvz= bovy_coords.cov_dvrpmllbb_to_vxyz(os*d,os*e_d,os*e_vr,
                                                  os*pmll,os*pmbb,
                                                  cov_pmllpmbb,
                                                  os*l,os*b,
                                                  degree=True,
                                                  plx=False)
    for ii in range(3):
        assert numpy.fabs(numpy.sqrt(cov_vxvyvz[ii,0,0])
                          -d*4.74047*pmll*numpy.sqrt((e_d/d)**2.+(10./pmll)**2.)) < 10.**-10., 'cov_dvrpmllbb_to_vxyz coversion did not work as expected'
        assert numpy.fabs(numpy.sqrt(cov_vxvyvz[ii,1,1])
                          -d*4.74047*pmbb*numpy.sqrt((e_d/d)**2.+(20./pmbb)**2.)) < 10.**-10., 'cov_dvrpmllbb_to_vxyz coversion did not work as expected'
        assert numpy.fabs(numpy.sqrt(cov_vxvyvz[ii,2,2])-e_vr) < 10.**-10., 'cov_dvrpmllbb_to_vxyz coversion did not work as expected'
    return None
コード例 #2
0
def uvw_unc(req_dict, opt_dict):

    cov_radec = np.zeros((2, 2))
    cov_radec[0, 0] = opt_dict['epmra']**2
    cov_radec[1, 1] = opt_dict['epmdec']**2

    covar_pmllbb = b_c.cov_pmrapmdec_to_pmllpmbb(cov_radec,
                                                 req_dict['ra'],
                                                 req_dict['dec'],
                                                 degree=True,
                                                 epoch=2000.0)

    cov_vxvyvz = b_c.cov_dvrpmllbb_to_vxyz(req_dict['dist'],
                                           opt_dict['edist'],
                                           opt_dict['erv'],
                                           req_dict['pml'],
                                           req_dict['pmb'],
                                           covar_pmllbb,
                                           req_dict['l'],
                                           req_dict['b'],
                                           plx=False,
                                           degree=True)

    du = vx_e = m.sqrt(cov_vxvyvz[0, 0])
    dv = vy_e = m.sqrt(cov_vxvyvz[1, 1])
    dw = vz_e = m.sqrt(cov_vxvyvz[2, 2])

    return du, dv, dw
コード例 #3
0
 def calc_spacevel_uncer_var_tensor(self):
     """
     Using vscatter for error in RV (km/s) and 2.5% distance errors
     """
     dist_uncer = 0.025 * self.get_col('RC_DIST')
     uncer_tensor = bcoords.cov_dvrpmllbb_to_vxyz(self.get_col('RC_DIST'),
                            dist_uncer,
                            self.get_col('VSCATTER'),
                            self.pmll_pmbb[:, 0], self.pmll_pmbb[:, 1],
                            self.covar_pmllpmbb, self.get_col('GLON'),
                            self.get_col('GLAT'), degree=self.degree)
     self.spacevel_uncer_var_tensor = uncer_tensor
コード例 #4
0
def obs_to_galcen(ra,
                  dec,
                  dist,
                  pmra,
                  pmdec,
                  rv,
                  pmra_err,
                  pmdec_err,
                  pmra_pmdec_corr,
                  dist_err,
                  rv_err,
                  return_cov=True,
                  verbose=True,
                  return_rphiz=True,
                  ro=8.,
                  vo=220.,
                  zo=0.025,
                  parallax=False):
    vxvv = np.dstack([ra, dec, dist, pmra, pmdec, rv])[0]
    ra, dec = vxvv[:, 0], vxvv[:, 1]
    lb = bovy_coords.radec_to_lb(ra, dec, degree=True)
    pmra, pmdec = vxvv[:, 3], vxvv[:, 4]
    pmllpmbb = bovy_coords.pmrapmdec_to_pmllpmbb(pmra,
                                                 pmdec,
                                                 ra,
                                                 dec,
                                                 degree=True)
    d, vlos = vxvv[:, 2], vxvv[:, 5]
    if parallax:
        d = 1. / d
    rectgal = bovy_coords.sphergal_to_rectgal(lb[:, 0],
                                              lb[:, 1],
                                              d,
                                              vlos,
                                              pmllpmbb[:, 0],
                                              pmllpmbb[:, 1],
                                              degree=True)
    vsolar = np.array([-10.1, 4.0, 6.7])
    vsun = np.array([
        0.,
        1.,
        0.,
    ]) + vsolar / vo
    X = rectgal[:, 0] / ro
    Y = rectgal[:, 1] / ro
    Z = rectgal[:, 2] / ro
    vx = rectgal[:, 3] / vo
    vy = rectgal[:, 4] / vo
    vz = rectgal[:, 5] / vo
    XYZ = np.dstack([X, Y, Z])[0]
    vxyz = np.dstack([vx, vy, vz])[0]
    if return_rphiz:
        Rpz = bovy_coords.XYZ_to_galcencyl(XYZ[:, 0],
                                           XYZ[:, 1],
                                           XYZ[:, 2],
                                           Zsun=zo / ro)
        vRvTvz = bovy_coords.vxvyvz_to_galcencyl(vxyz[:, 0],
                                                 vxyz[:, 1],
                                                 vxyz[:, 2],
                                                 Rpz[:, 0],
                                                 Rpz[:, 1],
                                                 Rpz[:, 2],
                                                 vsun=vsun,
                                                 Xsun=1.,
                                                 Zsun=zo / ro,
                                                 galcen=True)
    if return_cov == True:
        cov_pmradec = np.empty([len(pmra_err), 2, 2])
        cov_pmradec[:, 0, 0] = pmra_err**2
        cov_pmradec[:, 1, 1] = pmdec_err**2
        cov_pmradec[:, 0, 1] = pmra_pmdec_corr * pmra_err * pmdec_err
        cov_pmradec[:, 1, 0] = pmra_pmdec_corr * pmra_err * pmdec_err
        if verbose:
            print('propagating covariance in pmra pmdec -> pmll pmbb')
        cov_pmllbb = bovy_coords.cov_pmrapmdec_to_pmllpmbb(cov_pmradec,
                                                           vxvv[:, 0],
                                                           vxvv[:, 1],
                                                           degree=True,
                                                           epoch='J2015')
        if verbose:
            print('propagating covariance in pmll pmbb -> vx vy vz')
        cov_vxyz = bovy_coords.cov_dvrpmllbb_to_vxyz(vxvv[:, 2], dist_err,
                                                     rv_err, pmllpmbb[:, 0],
                                                     pmllpmbb[:,
                                                              1], cov_pmllbb,
                                                     lb[:, 0], lb[:, 1])
        if not return_rphiz:
            return XYZ, vxyz, cov_vxyz

        if verbose:
            print('propagating covariance in vx vy vz -> vR vT vz')
        cov_galcencyl = bovy_coords.cov_vxyz_to_galcencyl(cov_vxyz,
                                                          Rpz[:, 1],
                                                          Xsun=1.,
                                                          Zsun=zo / ro)
        return XYZ, vxyz, cov_vxyz, Rpz, vRvTvz, cov_galcencyl
    if not return_rphiz:
        return XYZ, vxyz
    return XYZ, vxyz, Rpz, vRvTvz
コード例 #5
0
def dat_to_galcen(
        dat,
        return_cov=True,
        return_rphiz=True,
        verbose=False,
        ro=8.,
        vo=220.,
        zo=0.025,
        keys=['ra', 'dec', 'BPG_meandist', 'pmra', 'pmdec', 'VHELIO_AVG'],
        cov_keys=[
            'pmra_error', 'pmdec_error', 'pmra_pmdec_corr', 'BPG_diststd',
            'VERR'
        ],
        parallax=False):
    vxvv = np.dstack([dat[keys[i]] for i in range(len(keys))])[0]
    ra, dec = vxvv[:, 0], vxvv[:, 1]
    lb = bovy_coords.radec_to_lb(ra, dec, degree=True)
    pmra, pmdec = vxvv[:, 3], vxvv[:, 4]
    pmllpmbb = bovy_coords.pmrapmdec_to_pmllpmbb(pmra,
                                                 pmdec,
                                                 ra,
                                                 dec,
                                                 degree=True)
    d, vlos = vxvv[:, 2], vxvv[:, 5]
    if parallax:
        d = 1. / d
    rectgal = bovy_coords.sphergal_to_rectgal(lb[:, 0],
                                              lb[:, 1],
                                              d,
                                              vlos,
                                              pmllpmbb[:, 0],
                                              pmllpmbb[:, 1],
                                              degree=True)
    vsolar = np.array([-11.1, 245.6,
                       7.25])  #use SBD10 vR and vZ and SGR proper motion vT
    vsun = np.array([
        0.,
        0.,
        0.,
    ]) + vsolar / vo
    X = rectgal[:, 0] / ro
    Y = rectgal[:, 1] / ro
    Z = rectgal[:, 2] / ro
    vx = rectgal[:, 3] / vo
    vy = rectgal[:, 4] / vo
    vz = rectgal[:, 5] / vo
    XYZ = np.dstack([X, Y, Z])[0]
    vxyz = np.dstack([vx, vy, vz])[0]
    if return_rphiz:
        Rpz = bovy_coords.XYZ_to_galcencyl(XYZ[:, 0],
                                           XYZ[:, 1],
                                           XYZ[:, 2],
                                           Zsun=zo / ro)
        vRvTvz = bovy_coords.vxvyvz_to_galcencyl(vxyz[:, 0],
                                                 vxyz[:, 1],
                                                 vxyz[:, 2],
                                                 Rpz[:, 0],
                                                 Rpz[:, 1],
                                                 Rpz[:, 2],
                                                 vsun=vsun,
                                                 Xsun=1.,
                                                 Zsun=zo / ro,
                                                 galcen=True)
    if return_cov == True:
        cov_pmradec = np.array([[[
            dat[cov_keys[0]][i]**2,
            dat[cov_keys[2]][i] * dat[cov_keys[0]][i] * dat[cov_keys[1]][i]
        ],
                                 [
                                     dat[cov_keys[2]][i] *
                                     dat[cov_keys[0]][i] * dat[cov_keys[1]][i],
                                     dat[cov_keys[1]][i]**2
                                 ]] for i in range(len(dat))])
        if verbose:
            print('propagating covariance in pmra pmdec -> pmll pmbb')
        cov_pmllbb = bovy_coords.cov_pmrapmdec_to_pmllpmbb(cov_pmradec,
                                                           vxvv[:, 0],
                                                           vxvv[:, 1],
                                                           degree=True,
                                                           epoch='J2015')
        if verbose:
            print('propagating covariance in pmll pmbb -> vx vy vz')
        cov_vxyz = bovy_coords.cov_dvrpmllbb_to_vxyz(vxvv[:,
                                                          2], dat[cov_keys[3]],
                                                     dat[cov_keys[4]],
                                                     pmllpmbb[:,
                                                              0], pmllpmbb[:,
                                                                           1],
                                                     cov_pmllbb, lb[:,
                                                                    0], lb[:,
                                                                           1])
        if not return_rphiz:
            return XYZ, vxyz, cov_vxyz

        if verbose:
            print('propagating covariance in vx vy vz -> vR vT vz')
        cov_galcencyl = bovy_coords.cov_vxyz_to_galcencyl(cov_vxyz,
                                                          Rpz[:, 1],
                                                          Xsun=1.,
                                                          Zsun=zo / ro)
        return XYZ, vxyz, cov_vxyz, Rpz, vRvTvz, cov_galcencyl
    if not return_rphiz:
        return XYZ, vxyz
    return XYZ, vxyz, Rpz, vRvTvz