diff --git a/.DS_Store b/.DS_Store
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diff --git a/build/lib/reflected_light_sim/__init__.py b/build/lib/reflected_light_sim/__init__.py
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+__version__ = "0.1"
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diff --git a/build/lib/reflected_light_sim/reflectance.py b/build/lib/reflected_light_sim/reflectance.py
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+++ b/build/lib/reflected_light_sim/reflectance.py
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+import astropy.io.fits as fits
+import glob
+import os
+import numpy as np
+import astropy.units as u
+import astropy.constants as cons
+
+class Spectrum():
+    '''
+    A class for spectra manipulation (based on PSI Sim's spectrum.py class).
+
+    The main properties will be: 
+    wvs    - sampled wavelengths (np.array of floats, in microns)
+    spectrum    - current flux values of the spectrum (np.array of floats, [photons/s/cm^2/A])
+    R   - spectral resolution (float)
+
+    The main functions will be: 
+    load_phoenix_model      - load a PHOENIX model 
+    calculate_reflected_light  -calculate the reflected light from a planet
+
+
+    '''
+
+    def __init__(self, wvs, spectrum, R):
+
+        self.wvs = wvs
+        self.spectrum = spectrum
+        self.R = R
+
+        return
+    
+    # def load_phoenix_model(self, )
+        
+
+    def load_phoenix_model(lambda_start, lambda_end,steff,path=None):
+        '''
+        Read in a phoenix spectrum
+        '''
+       
+        # Prompt the user to specify a path if none is given
+        if path is None:
+            path = input('Specify a path to your PHOENIX model (directory containing wavels + fluxes): \n')
+        teff =str(int(steff)).zfill(5)
+        path_use = path + 'lte%s-4.50-0.0.PHOENIX-ACES-AGSS-COND-2011-HiRes.fits'%(teff)
+        f = fits.open(path_use)
+        spec = f[0].data / (1e8) # ergs/s/cm2/cm to ergs/s/cm2/Angstrom for conversion
+        f.close()
+        
+        f = fits.open(path + 'WAVE_PHOENIX-ACES-AGSS-COND-2011.fits')
+        lam = f[0].data # angstroms
+        f.close()
+        
+        # Convert
+        conversion_factor = 5.03*10**7 * lam #lam in angstrom here
+        spec *= conversion_factor # phot/cm2/s/angstrom
+        
+        # Take subarray requested
+        isub = np.where( (lam > lambda_start*10.0) & (lam < lambda_end*10.0))[0]
+
+        # Convert 
+        return lam[isub]/10.0,spec[isub] * 10 * 100**2 #nm, phot/m2/s/nm
+
+    def cal_refflux_pl(d_star_earth,host_spec,r_star,r_planet,a_planet, albedo,wvl):
+        '''
+        Calculation about reflected flux from planet
+        '''
+        wvl *= u.nm
+        ph_energy = ((cons.h * cons.c / (wvl) ) /u.ph).to(u.J / u.ph)
+
+        host_spec_J = (host_spec* u.ph / (u.m**2 * u.s * u.nm) * ph_energy).to(u.J / (u.m**2 * u.s * u.nm))
+
+        lum_star = host_spec_J * 4 * np.pi * r_star**2
+
+        # flux of star on planet
+        flux_sp = lum_star / (4 * np.pi * a_planet**2)
+
+        lum_planet = flux_sp * r_planet**2 * np.pi * albedo
+
+        flux_planet = lum_planet / (4 * np.pi * d_star_earth**2)
+
+        flux_planet_ph = (flux_planet / ph_energy).to(u.ph / (u.m**2 * u.s * u.nm))
+
+        # Convert 
+        return flux_planet_ph #nm, phot/m2/s/nm
+        
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diff --git a/dist/reflected_light_sim-0.1-py3-none-any.whl b/dist/reflected_light_sim-0.1-py3-none-any.whl
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diff --git a/dist/reflected_light_sim-0.1.tar.gz b/dist/reflected_light_sim-0.1.tar.gz
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