# Third-party
import astropy.coordinates as coord
import astropy.units as u

__all__ = ['get_galactocentric2019']


def get_galactocentric2019():
    """
    References
    ----------
    Galactic center sky position:
    - `Reid & Brunthaler (2004) <https://ui.adsabs.harvard.edu/abs/2004ApJ...616..872R/abstract>`_

    Galactic center distance:
    - `GRAVITY collaboration (2018) <https://ui.adsabs.harvard.edu/abs/2018A%26A...615L..15G/abstract>`_

    Solar velocity:
    - `Drimmel & Poggio (2018) <https://ui.adsabs.harvard.edu/abs/2018RNAAS...2d.210D/abstract>`_
    - `Reid & Brunthaler (2004) <https://ui.adsabs.harvard.edu/abs/2004ApJ...616..872R/abstract>`_
    - `GRAVITY collaboration (2018) <https://ui.adsabs.harvard.edu/abs/2018A%26A...615L..15G/abstract>`_

    Solar height above midplane:
    - `Bennett & Bovy (2019) <https://ui.adsabs.harvard.edu/abs/2019MNRAS.482.1417B/abstract>`_

    Returns
    -------
    galcen_frame : `~astropy.coordinates.Galactocentric`
        The modern (2019) Galactocentric reference frame.

    """
    rsun = 8.122 * u.kpc
    vsun = coord.CartesianDifferential([12.9, 245.6, 7.78] * u.km/u.s)
    zsun = 20.8 * u.pc

    return coord.Galactocentric(galcen_distance=rsun,
                                galcen_v_sun=vsun,
                                z_sun=zsun)

e8839c5429848fe15cc1c475354b0242ef1a75e6
<mask token>

<mask token>


def get_galactocentric2019():
    """
    References
    ----------
    Galactic center sky position:
    - `Reid & Brunthaler (2004) <https://ui.adsabs.harvard.edu/abs/2004ApJ...616..872R/abstract>`_

    Galactic center distance:
    - `GRAVITY collaboration (2018) <https://ui.adsabs.harvard.edu/abs/2018A%26A...615L..15G/abstract>`_

    Solar velocity:
    - `Drimmel & Poggio (2018) <https://ui.adsabs.harvard.edu/abs/2018RNAAS...2d.210D/abstract>`_
    - `Reid & Brunthaler (2004) <https://ui.adsabs.harvard.edu/abs/2004ApJ...616..872R/abstract>`_
    - `GRAVITY collaboration (2018) <https://ui.adsabs.harvard.edu/abs/2018A%26A...615L..15G/abstract>`_

    Solar height above midplane:
    - `Bennett & Bovy (2019) <https://ui.adsabs.harvard.edu/abs/2019MNRAS.482.1417B/abstract>`_

    Returns
    -------
    galcen_frame : `~astropy.coordinates.Galactocentric`
        The modern (2019) Galactocentric reference frame.

    """
    rsun = 8.122 * u.kpc
    vsun = coord.CartesianDifferential([12.9, 245.6, 7.78] * u.km / u.s)
    zsun = 20.8 * u.pc
    return coord.Galactocentric(galcen_distance=rsun, galcen_v_sun=vsun,
        z_sun=zsun)

<mask token>
__all__ = ['get_galactocentric2019']


def get_galactocentric2019():
    """
    References
    ----------
    Galactic center sky position:
    - `Reid & Brunthaler (2004) <https://ui.adsabs.harvard.edu/abs/2004ApJ...616..872R/abstract>`_

    Galactic center distance:
    - `GRAVITY collaboration (2018) <https://ui.adsabs.harvard.edu/abs/2018A%26A...615L..15G/abstract>`_

    Solar velocity:
    - `Drimmel & Poggio (2018) <https://ui.adsabs.harvard.edu/abs/2018RNAAS...2d.210D/abstract>`_
    - `Reid & Brunthaler (2004) <https://ui.adsabs.harvard.edu/abs/2004ApJ...616..872R/abstract>`_
    - `GRAVITY collaboration (2018) <https://ui.adsabs.harvard.edu/abs/2018A%26A...615L..15G/abstract>`_

    Solar height above midplane:
    - `Bennett & Bovy (2019) <https://ui.adsabs.harvard.edu/abs/2019MNRAS.482.1417B/abstract>`_

    Returns
    -------
    galcen_frame : `~astropy.coordinates.Galactocentric`
        The modern (2019) Galactocentric reference frame.

    """
    rsun = 8.122 * u.kpc
    vsun = coord.CartesianDifferential([12.9, 245.6, 7.78] * u.km / u.s)
    zsun = 20.8 * u.pc
    return coord.Galactocentric(galcen_distance=rsun, galcen_v_sun=vsun,
        z_sun=zsun)

import astropy.coordinates as coord
import astropy.units as u
__all__ = ['get_galactocentric2019']


def get_galactocentric2019():
    """
    References
    ----------
    Galactic center sky position:
    - `Reid & Brunthaler (2004) <https://ui.adsabs.harvard.edu/abs/2004ApJ...616..872R/abstract>`_

    Galactic center distance:
    - `GRAVITY collaboration (2018) <https://ui.adsabs.harvard.edu/abs/2018A%26A...615L..15G/abstract>`_

    Solar velocity:
    - `Drimmel & Poggio (2018) <https://ui.adsabs.harvard.edu/abs/2018RNAAS...2d.210D/abstract>`_
    - `Reid & Brunthaler (2004) <https://ui.adsabs.harvard.edu/abs/2004ApJ...616..872R/abstract>`_
    - `GRAVITY collaboration (2018) <https://ui.adsabs.harvard.edu/abs/2018A%26A...615L..15G/abstract>`_

    Solar height above midplane:
    - `Bennett & Bovy (2019) <https://ui.adsabs.harvard.edu/abs/2019MNRAS.482.1417B/abstract>`_

    Returns
    -------
    galcen_frame : `~astropy.coordinates.Galactocentric`
        The modern (2019) Galactocentric reference frame.

    """
    rsun = 8.122 * u.kpc
    vsun = coord.CartesianDifferential([12.9, 245.6, 7.78] * u.km / u.s)
    zsun = 20.8 * u.pc
    return coord.Galactocentric(galcen_distance=rsun, galcen_v_sun=vsun,
        z_sun=zsun)

# Third-party
import astropy.coordinates as coord
import astropy.units as u

__all__ = ['get_galactocentric2019']


def get_galactocentric2019():
    """
    References
    ----------
    Galactic center sky position:
    - `Reid & Brunthaler (2004) <https://ui.adsabs.harvard.edu/abs/2004ApJ...616..872R/abstract>`_

    Galactic center distance:
    - `GRAVITY collaboration (2018) <https://ui.adsabs.harvard.edu/abs/2018A%26A...615L..15G/abstract>`_

    Solar velocity:
    - `Drimmel & Poggio (2018) <https://ui.adsabs.harvard.edu/abs/2018RNAAS...2d.210D/abstract>`_
    - `Reid & Brunthaler (2004) <https://ui.adsabs.harvard.edu/abs/2004ApJ...616..872R/abstract>`_
    - `GRAVITY collaboration (2018) <https://ui.adsabs.harvard.edu/abs/2018A%26A...615L..15G/abstract>`_

    Solar height above midplane:
    - `Bennett & Bovy (2019) <https://ui.adsabs.harvard.edu/abs/2019MNRAS.482.1417B/abstract>`_

    Returns
    -------
    galcen_frame : `~astropy.coordinates.Galactocentric`
        The modern (2019) Galactocentric reference frame.

    """
    rsun = 8.122 * u.kpc
    vsun = coord.CartesianDifferential([12.9, 245.6, 7.78] * u.km/u.s)
    zsun = 20.8 * u.pc

    return coord.Galactocentric(galcen_distance=rsun,
                                galcen_v_sun=vsun,
                                z_sun=zsun)
