Python coordinates.FK5屬性代碼示例

# 需要導入模塊: from astropy import coordinates [as 別名]
# 或者: from astropy.coordinates import FK5 [as 別名]
def test_parse_coord_system():

    frame = parse_coord_system(Galactic())
    assert isinstance(frame, Galactic)

    frame = parse_coord_system('fk5')
    assert isinstance(frame, FK5)

    with pytest.raises(ValueError) as exc:
        frame = parse_coord_system('e')
    assert exc.value.args[0] == "Ecliptic coordinate frame not yet supported"

    frame = parse_coord_system('g')
    assert isinstance(frame, Galactic)

    with pytest.raises(ValueError) as exc:
        frame = parse_coord_system('spam')
    assert exc.value.args[0] == "Could not determine frame for system=spam" 

# 需要導入模塊: from astropy import coordinates [as 別名]
# 或者: from astropy.coordinates import FK5 [as 別名]
def test_caching_components_and_classes():

    # Make sure that when we change the WCS object, the classes and components
    # are updated (we use a cache internally, so we need to make sure the cache
    # is invalidated if needed)

    wcs = WCS_SIMPLE_CELESTIAL

    assert wcs.world_axis_object_components == [('celestial', 0, 'spherical.lon.degree'),
                                                ('celestial', 1, 'spherical.lat.degree')]

    assert wcs.world_axis_object_classes['celestial'][0] is SkyCoord
    assert wcs.world_axis_object_classes['celestial'][1] == ()
    assert isinstance(wcs.world_axis_object_classes['celestial'][2]['frame'], ICRS)
    assert wcs.world_axis_object_classes['celestial'][2]['unit'] is u.deg

    wcs.wcs.radesys = 'FK5'

    frame = wcs.world_axis_object_classes['celestial'][2]['frame']
    assert isinstance(frame, FK5)
    assert frame.equinox.jyear == 2000.

    wcs.wcs.equinox = 2010

    frame = wcs.world_axis_object_classes['celestial'][2]['frame']
    assert isinstance(frame, FK5)
    assert frame.equinox.jyear == 2010. 

# 需要導入模塊: from astropy import coordinates [as 別名]
# 或者: from astropy.coordinates import FK5 [as 別名]
def _celestial_frame_to_wcs_builtin(frame, projection='TAN'):

    # Import astropy.coordinates here to avoid circular imports
    from astropy.coordinates import BaseRADecFrame, FK4, FK4NoETerms, FK5, ICRS, ITRS, Galactic

    # Create a 2-dimensional WCS
    wcs = WCS(naxis=2)

    if isinstance(frame, BaseRADecFrame):

        xcoord = 'RA--'
        ycoord = 'DEC-'
        if isinstance(frame, ICRS):
            wcs.wcs.radesys = 'ICRS'
        elif isinstance(frame, FK4NoETerms):
            wcs.wcs.radesys = 'FK4-NO-E'
            wcs.wcs.equinox = frame.equinox.byear
        elif isinstance(frame, FK4):
            wcs.wcs.radesys = 'FK4'
            wcs.wcs.equinox = frame.equinox.byear
        elif isinstance(frame, FK5):
            wcs.wcs.radesys = 'FK5'
            wcs.wcs.equinox = frame.equinox.jyear
        else:
            return None
    elif isinstance(frame, Galactic):
        xcoord = 'GLON'
        ycoord = 'GLAT'
    elif isinstance(frame, ITRS):
        xcoord = 'TLON'
        ycoord = 'TLAT'
        wcs.wcs.radesys = 'ITRS'
        wcs.wcs.dateobs = frame.obstime.utc.isot
    else:
        return None

    wcs.wcs.ctype = [xcoord + '-' + projection, ycoord + '-' + projection]

    return wcs 

# 需要導入模塊: from astropy import coordinates [as 別名]
# 或者: from astropy.coordinates import FK5 [as 別名]
def test_skycoord_to_pixel(mode):

    # Import astropy.coordinates here to avoid circular imports
    from astropy.coordinates import SkyCoord

    header = get_pkg_data_contents('data/maps/1904-66_TAN.hdr', encoding='binary')
    wcs = WCS(header)

    ref = SkyCoord(0.1 * u.deg, -89. * u.deg, frame='icrs')

    xp, yp = skycoord_to_pixel(ref, wcs, mode=mode)

    # WCS is in FK5 so we need to transform back to ICRS
    new = pixel_to_skycoord(xp, yp, wcs, mode=mode).transform_to('icrs')

    assert_allclose(new.ra.degree, ref.ra.degree)
    assert_allclose(new.dec.degree, ref.dec.degree)

    # Make sure you can specify a different class using ``cls`` keyword
    class SkyCoord2(SkyCoord):
        pass

    new2 = pixel_to_skycoord(xp, yp, wcs, mode=mode,
                             cls=SkyCoord2).transform_to('icrs')

    assert new2.__class__ is SkyCoord2
    assert_allclose(new2.ra.degree, ref.ra.degree)
    assert_allclose(new2.dec.degree, ref.dec.degree) 

# 需要導入模塊: from astropy import coordinates [as 別名]
# 或者: from astropy.coordinates import FK5 [as 別名]
def test_skycoord_to_pixel_swapped():

    # Regression test for a bug that caused skycoord_to_pixel and
    # pixel_to_skycoord to not work correctly if the axes were swapped in the
    # WCS.

    # Import astropy.coordinates here to avoid circular imports
    from astropy.coordinates import SkyCoord

    header = get_pkg_data_contents('data/maps/1904-66_TAN.hdr', encoding='binary')
    wcs = WCS(header)

    wcs_swapped = wcs.sub([WCSSUB_LATITUDE, WCSSUB_LONGITUDE])

    ref = SkyCoord(0.1 * u.deg, -89. * u.deg, frame='icrs')

    xp1, yp1 = skycoord_to_pixel(ref, wcs)
    xp2, yp2 = skycoord_to_pixel(ref, wcs_swapped)

    assert_allclose(xp1, xp2)
    assert_allclose(yp1, yp2)

    # WCS is in FK5 so we need to transform back to ICRS
    new1 = pixel_to_skycoord(xp1, yp1, wcs).transform_to('icrs')
    new2 = pixel_to_skycoord(xp1, yp1, wcs_swapped).transform_to('icrs')

    assert_allclose(new1.ra.degree, new2.ra.degree)
    assert_allclose(new1.dec.degree, new2.dec.degree) 

# 需要導入模塊: from astropy import coordinates [as 別名]
# 或者: from astropy.coordinates import FK5 [as 別名]
def test_constellations(recwarn):
    from astropy.coordinates import ICRS, FK5, SkyCoord
    from astropy.coordinates.funcs import get_constellation

    inuma = ICRS(9*u.hour, 65*u.deg)

    n_prewarn = len(recwarn)
    res = get_constellation(inuma)
    res_short = get_constellation(inuma, short_name=True)
    assert len(recwarn) == n_prewarn  # neither version should not make warnings

    assert res == 'Ursa Major'
    assert res_short == 'UMa'
    assert isinstance(res, str) or getattr(res, 'shape', None) == tuple()

    # these are taken from the ReadMe for Roman 1987
    ras = [9, 23.5, 5.12, 9.4555, 12.8888, 15.6687, 19, 6.2222]
    decs = [65, -20, 9.12, -19.9, 22, -12.1234, -40, -81.1234]
    shortnames = ['UMa', 'Aqr', 'Ori', 'Hya', 'Com', 'Lib', 'CrA', 'Men']

    testcoos = FK5(ras*u.hour, decs*u.deg, equinox='B1950')
    npt.assert_equal(get_constellation(testcoos, short_name=True), shortnames)

    # test on a SkyCoord, *and* test Boötes, which is special in that it has a
    # non-ASCII character
    bootest = SkyCoord(15*u.hour, 30*u.deg, frame='icrs')
    boores = get_constellation(bootest)
    assert boores == 'Boötes'
    assert isinstance(boores, str) or getattr(boores, 'shape', None) == tuple() 

# 需要導入模塊: from astropy import coordinates [as 別名]
# 或者: from astropy.coordinates import FK5 [as 別名]
def test_concatenate():
    from astropy.coordinates import FK5, SkyCoord, ICRS
    from astropy.coordinates.funcs import concatenate

    # Just positions
    fk5 = FK5(1*u.deg, 2*u.deg)
    sc = SkyCoord(3*u.deg, 4*u.deg, frame='fk5')

    res = concatenate([fk5, sc])
    np.testing.assert_allclose(res.ra, [1, 3]*u.deg)
    np.testing.assert_allclose(res.dec, [2, 4]*u.deg)

    with pytest.raises(TypeError):
        concatenate(fk5)

    with pytest.raises(TypeError):
        concatenate(1*u.deg)

    # positions and velocities
    fr = ICRS(ra=10*u.deg, dec=11.*u.deg,
              pm_ra_cosdec=12*u.mas/u.yr,
              pm_dec=13*u.mas/u.yr)
    sc = SkyCoord(ra=20*u.deg, dec=21.*u.deg,
                  pm_ra_cosdec=22*u.mas/u.yr,
                  pm_dec=23*u.mas/u.yr)

    res = concatenate([fr, sc])

    with pytest.raises(ValueError):
        concatenate([fr, fk5])

    fr2 = ICRS(ra=10*u.deg, dec=11.*u.deg)
    with pytest.raises(ValueError):
        concatenate([fr, fr2]) 

# 需要導入模塊: from astropy import coordinates [as 別名]
# 或者: from astropy.coordinates import FK5 [as 別名]
def test_fk5_time(tmpdir):

    tree = {'coord': FK5(equinox="2011-01-01T00:00:00")}

    assert_roundtrip_tree(tree, tmpdir) 

# 需要導入模塊: from astropy import coordinates [as 別名]
# 或者: from astropy.coordinates import FK5 [as 別名]
def _wcs_to_celestial_frame_builtin(wcs):

    # Import astropy.coordinates here to avoid circular imports
    from astropy.coordinates import (FK4, FK4NoETerms, FK5, ICRS, ITRS,
                                     Galactic, SphericalRepresentation)

    # Import astropy.time here otherwise setup.py fails before extensions are compiled
    from astropy.time import Time

    if wcs.wcs.lng == -1 or wcs.wcs.lat == -1:
        return None

    radesys = wcs.wcs.radesys

    if np.isnan(wcs.wcs.equinox):
        equinox = None
    else:
        equinox = wcs.wcs.equinox

    xcoord = wcs.wcs.ctype[wcs.wcs.lng][:4]
    ycoord = wcs.wcs.ctype[wcs.wcs.lat][:4]

    # Apply logic from FITS standard to determine the default radesys
    if radesys == '' and xcoord == 'RA--' and ycoord == 'DEC-':
        if equinox is None:
            radesys = "ICRS"
        elif equinox < 1984.:
            radesys = "FK4"
        else:
            radesys = "FK5"

    if radesys == 'FK4':
        if equinox is not None:
            equinox = Time(equinox, format='byear')
        frame = FK4(equinox=equinox)
    elif radesys == 'FK4-NO-E':
        if equinox is not None:
            equinox = Time(equinox, format='byear')
        frame = FK4NoETerms(equinox=equinox)
    elif radesys == 'FK5':
        if equinox is not None:
            equinox = Time(equinox, format='jyear')
        frame = FK5(equinox=equinox)
    elif radesys == 'ICRS':
        frame = ICRS()
    else:
        if xcoord == 'GLON' and ycoord == 'GLAT':
            frame = Galactic()
        elif xcoord == 'TLON' and ycoord == 'TLAT':
            # The default representation for ITRS is cartesian, but for WCS
            # purposes, we need the spherical representation.
            frame = ITRS(representation_type=SphericalRepresentation,
                         obstime=wcs.wcs.dateobs or None)
        else:
            frame = None

    return frame 

# 需要導入模塊: from astropy import coordinates [as 別名]
# 或者: from astropy.coordinates import FK5 [as 別名]
def compute_paral_angles(header, latitude, ra_key, dec_key, lst_key, 
                         acqtime_key, date_key='DATE-OBS'):
    """Calculates the parallactic angle for a frame, taking coordinates and
    local sidereal time from fits-headers (frames taken in an alt-az telescope 
    with the image rotator off).
    
    The coordinates in the header are assumed to be J2000 FK5 coordinates.
    The spherical trigonometry formula for calculating the parallactic angle
    is taken from Astronomical Algorithms (Meeus, 1998).
    
    Parameters
    ----------
    header : dictionary
        Header of current frame.
    latitude : float
        Latitude of the observatory in degrees. The dictionaries in 
        vip_hci/conf/param.py can be used like: latitude=LBT['latitude'].
    ra_key, dec_key, lst_key, acqtime_key, date_key : strings
        Keywords where the values are stored in the header.
        
    Returns
    -------
    pa.value : float
        Parallactic angle in degrees for current header (frame).
    """                                    
    obs_epoch = Time(header[date_key], format='iso', scale='utc')
       
    # equatorial coordinates in J2000
    ra = header[ra_key]                                                         
    dec = header[dec_key]   
    coor = sky_coordinate.SkyCoord(ra=ra, dec=dec, unit=(hourangle,degree),
                                   frame=FK5, equinox='J2000.0')
    # recalculate for DATE-OBS (precession)
    coor_curr = coor.transform_to(FK5(equinox=obs_epoch))
    
    # new ra and dec in radians
    ra_curr = coor_curr.ra                                                      
    dec_curr = coor_curr.dec
        
    lst_split = header[lst_key].split(':')
    lst = float(lst_split[0])+float(lst_split[1])/60+float(lst_split[2])/3600
    exp_delay = (header[acqtime_key] * 0.5) / 3600
    # solar to sidereal time
    exp_delay = exp_delay*1.0027                                                
    
    # hour angle in degrees
    hour_angle = (lst + exp_delay) * 15 - ra_curr.deg                           
    hour_angle = np.deg2rad(hour_angle)                                         
    latitude = np.deg2rad(latitude)                                             
    
    # PA formula from Astronomical Algorithms 
    pa = -np.rad2deg(np.arctan2(-np.sin(hour_angle), np.cos(dec_curr) * \
                 np.tan(latitude) - np.sin(dec_curr) * np.cos(hour_angle)))     
  
    #if dec_curr.value > latitude:  pa = (pa.value + 360) % 360
    
    return pa.value