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1 |
| -# PyLDTk |
| 1 | +# LDTk |
2 | 2 |
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3 | 3 | [](http://www.gnu.org/licenses/gpl-2.0.html)
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4 | 4 | [](http://mnras.oxfordjournals.org/content/453/4/3821.abstract)
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7 | 7 | [](https://zenodo.org/badge/latestdoi/5871/hpparvi/ldtk)
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8 | 8 | [](http://www.astropy.org/)
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9 | 9 |
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10 |
| -**Py**thon **L**imb **D**arkening **T**ool**k**it - a Python toolkit for calculating stellar limb darkening profiles and model-specific coefficients for arbitrary passbands using the stellar spectrum model library by Husser et al (2013). |
| 10 | +Python **L**imb **D**arkening **T**ool**k**it - a Python toolkit for calculating stellar limb darkening profiles and model-specific coefficients for arbitrary passbands using the stellar spectrum model library by Husser et al (2013). |
11 | 11 |
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12 | 12 | ```python
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13 | 13 | from ldtk import LDPSetCreator, BoxcarFilter
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@@ -40,7 +40,7 @@ lnlike = ps.lnlike_qd([0.25,0.05],flt=0) # Quad. law log L for the first filter
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40 | 40 |
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41 | 41 | ## Overview
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42 | 42 |
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43 |
| -PyLDTk automates the calculation of custom stellar limb darkening (LD) profiles and model-specific limb darkening coefficients (LDC) using the library of PHOENIX-generated specific intensity spectra by Husser et al. (2013). |
| 43 | +LDTk automates the calculation of custom stellar limb darkening (LD) profiles and model-specific limb darkening coefficients (LDC) using the library of PHOENIX-generated specific intensity spectra by Husser et al. (2013). |
44 | 44 |
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45 | 45 | The aim of the package is to facilitate exoplanet transit light curve modeling, especially transmission
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46 | 46 | spectroscopy where the modeling is carried out for custom narrow passbands. The package can be
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@@ -150,11 +150,11 @@ The limb darkening profiles can be resampled to a desired sampling in ``mu`` usi
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150 | 150 |
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151 | 151 | ## Citing
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152 | 152 |
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153 |
| -If you use PyLDTk in your research, please cite the PyLDTk paper |
| 153 | +If you use LDTk in your research, please cite the LDTk paper |
154 | 154 |
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155 | 155 | Parviainen, H. & Aigrain, S. MNRAS 453, 3821–3826 (2015) (DOI:10.1093/mnras/stv1857).
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156 | 156 |
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157 |
| -and the paper describing the spectrum library without which PyLDTk would be rather useless |
| 157 | +and the paper describing the spectrum library without which LDTk would be rather useless |
158 | 158 |
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159 | 159 | Husser, T.-O. et al. A&A 553, A6 (2013) (DOI:10.1051/0004-6361/201219058).
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160 | 160 |
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