Checking in.

Author: mkelley

docs/sbpy/calib.rst

@@ -41,6 +41,9 @@ The names of the built-in sources are stored as an internal array.  They can be
     >>> print(sun)
     <Sun: E490-00a (2014) low resolution reference solar spectrum (Table 4)>
 
+
+.. _sbpy-spectroscopic-calibration:
+
 Controlling the default spectra
 -------------------------------
 
@@ -92,6 +95,8 @@ An example showing how to change the default Vega spectrum:
     ...   # vega.txt in effect
 
 
+.. _sbpy-photometric-calibration:
+
 Photometric calibration (without spectra or `synphot`)
 ------------------------------------------------------
 

sbpy/photometry/hb/data/filter.ecsv

@@ -6,7 +6,7 @@
 # - {name: cwave, unit: AA, datatype: float64, description: center wavelength}
 # - {name: width, unit: AA, datatype: string, subtype: 'float64[4]', description: full-width power points at 80%, 50%, 10%, and 1% of the peak transmission}
 # - {name: Flam0, unit: erg / (cm2 s AA), datatype: float64, description: flux of 0 magnitude star}
-# - {name: XXmBCsun, unit: mag, datatype: float64, description: "solar color, XX-BC"}
+# - {name: XXmBCsun, datatype: float64, description: "solar color, XX-BC"}
 # - {name: gamma_XX_XX, unit: 1 / AA, datatype: float64, description: "fraction of gas emission band captured by filter, normalized by the filter's equivalent width and transmission properties"}
 # - {name: gamma_prime_XX_XX, datatype: float64, description: fraction of gas emission band captured by filter}
 # meta: !!omap

sbpy/photometry/hb/filter.py

@@ -106,9 +106,9 @@ def fluxd0(self) -> u.Quantity[u.Unit("erg / (cm2 s AA)")]:
         return filter_data[self.value]["Flam0"]
 
     @property
-    def solar_color(self) -> u.mag:
+    def solar_color(self) -> u.Magnitude:
         """Solar color: [filter]-BC."""
-        return filter_data[self.value]["XXmBCsun"]
+        return u.Magnitude(filter_data[self.value]["XXmBCsun"])
 
     def gamma(self, molecule: str) -> u.Quantity[1 / u.AA]:
         """Fraction of molecule present in this filter, normalized by filter equivalent width.

sbpy/photometry/hb/tests/test_filter.py

@@ -35,7 +35,7 @@ def test_fluxd0(self):
         assert HBFilterSet.H2Oplus.fluxd0 == 1.380e-9 * u.erg / u.cm**2 / u.s / u.AA
 
     def test_solar_color(self):
-        assert HBFilterSet.C3.solar_color == 0.497 * u.mag
+        assert HBFilterSet.C3.solar_color == u.Magnitude(0.497)
 
     def test_gamma(self):
         assert HBFilterSet.C2.gamma("C2") == 5.433e-3 / u.AA

sbpy/spectroscopy/core.py

@@ -8,7 +8,6 @@
 import numpy as np
 import astropy.units as u
 
-
 __all__ = ["Spectrum", "SpectralModel", "SpectralGradient"]
 
 __doctest_requires__ = {