コード例 #1
0
    def _calculate_pos_crs(self, source):
        """Calculate position for a source

        Args:
            source (String):    Key saying which source to calculate position for.

        Returns:
            Array:  Positions, one 2-vector
        """

        ga = 0.0058 * Unit.mas2rad  # Aberration constant (mas/yr)
        mjd_2015 = 57023.0  # # Reference epoch of aberration model

        # Galactic center
        gc = Direction(ra=Unit.hms_to_rad(17, 45, 40.04),
                       dec=Unit.dms_to_rad(-29, 0, 28.1))

        # Radio source
        src = Direction(ra=self.data[source]["ra"],
                        dec=self.data[source]["dec"])

        # Compute correction
        dra = ga * gc.unit_vector @ src.dsrc_dra
        ddec = ga * gc.unit_vector @ src.dsrc_ddec
        dt = (self.time.mean.mjd - mjd_2015) * Unit.day2julian_year

        ra = src.right_ascension + dra * dt
        dec = src.declination + ddec * dt

        return np.squeeze(Direction(ra=ra, dec=dec, time=self.time))
コード例 #2
0
ファイル: icrf3.py プロジェクト: priyatharsan/where
    def _calculate_pos_crs(self, source):
        """Calculate position for a source

        Args:
            source (String):    Key saying which source to calculate position for.

        Returns:
            Array:  Positions, one 2-vector
        """

        ga = 0.0058 * Unit.mas2rad  # Aberration constant (mas/yr)
        mjd_2015 = 57023.0  # # Reference epoch of aberration model

        # Galactic center
        gc_ra = Unit.hms_to_rad(17, 45, 40.04)
        gc_dec = Unit.dms_to_rad(-29, 0, 28.1)
        gc = radec2unitvector(gc_ra, gc_dec)

        source_info = self.data[source]

        # Compute correction
        dra = ga * gc @ dsrc_dra(source_info["ra"], source_info["dec"])
        ddec = ga * gc @ dsrc_ddec(source_info["ra"], source_info["dec"])
        dt = (self.time.mean.mjd - mjd_2015) * Unit.day2julian_year

        return np.array(
            [source_info["ra"] + dra * dt, source_info["dec"] + ddec * dt])
コード例 #3
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    def _convert_dms2rad(self, field: bytes) -> float:
        """Convert DMS (degrees, minutes, seconds) to radians

        Args:
            field:  Original field with degrees, minutes, seconds separated by whitespace.

        Returns:
            Field converted to radians.
        """
        degrees, minutes, seconds = [float(f) for f in field.split()]
        return Unit.dms_to_rad(degrees, minutes, seconds)
コード例 #4
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ファイル: vlbi_ngs_sources.py プロジェクト: yxw027/where
    def parse_radio_source(self, line, _):
        """Read station position

        Reads the station position from the NGS file.

        Args:
            line:  Input data from NGS file
        """
        src_name = line["name"]
        self.data[src_name] = dict()
        self.data[src_name]["ra"] = Unit.hms_to_rad(float(line["ra_hrs"]),
                                                    int(line["ra_mins"]),
                                                    float(line["ra_secs"]))
        self.data[src_name]["dec"] = Unit.dms_to_rad(
            float(line["dec_degs"].replace(" ", "")), int(line["dec_mins"]),
            float(line["dec_secs"]))
コード例 #5
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    def structure_data(self):
        ra = Unit.hms_to_rad(self._array["ra_h"], self._array["ra_m"],
                             self._array["ra_s"])
        dec = Unit.dms_to_rad(self._array["dec_deg"], self._array["dec_m"],
                              self._array["dec_s"])

        src_type = dict(vcs=False, non_vcs=True, undefined=False)
        self.data = {
            src["iers_name"]: dict(icrf_name=src["icrf_name"],
                                   defining=src["defining"],
                                   special=src["special"],
                                   ra=ra[i],
                                   dec=dec[i],
                                   **src_type)
            for i, src in enumerate(self._array)
        }