phoebe
Advanced tools
| Metadata-Version: 2.4 | ||
| Name: phoebe | ||
| Version: 2.4.21 | ||
| Version: 2.4.22 | ||
| Summary: PHOEBE: modeling and analysis of eclipsing binary stars | ||
@@ -127,2 +127,10 @@ Author-email: Andrej Prša <aprsa@villanova.edu>, Kyle Conroy <kyle.conroy@villanova.edu>, Angela Kochoska <angela.kochoska@villanova.edu>, Martin Horvat <martin.horvat@fmf.uni-lj.si>, Dave Jones <djones@iac.es>, Michael Abdul-Masih <michael.abdul-masih@eso.org>, Bert Pablo <hpablo@aavso.org>, Joe Giammarco <giammarc@eastern.edu> | ||
| ### 2.4.22 | ||
| * Fixes bug where LS periodogram was returning frequency instead of period [#1089] | ||
| * Fixes passband luminosity computation for the dataset-scaled mode. [#1091] | ||
| * Fixes third light computation when multiple passbands are used. [#1091] | ||
| * Argument order for compute_l3s() changed to explicitly provide the model as it is required for correct scaling. [#1091] | ||
| * Fixes support for newer releases of scipy. [#1102] | ||
| ### 2.4.21 | ||
@@ -129,0 +137,0 @@ |
@@ -20,3 +20,3 @@ """ | ||
| __version__ = '2.4.21' | ||
| __version__ = '2.4.22' | ||
@@ -23,0 +23,0 @@ import os as _os |
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| Metadata-Version: 2.4 | ||
| Name: phoebe | ||
| Version: 2.4.21 | ||
| Version: 2.4.22 | ||
| Summary: PHOEBE: modeling and analysis of eclipsing binary stars | ||
@@ -127,2 +127,10 @@ Author-email: Andrej Prša <aprsa@villanova.edu>, Kyle Conroy <kyle.conroy@villanova.edu>, Angela Kochoska <angela.kochoska@villanova.edu>, Martin Horvat <martin.horvat@fmf.uni-lj.si>, Dave Jones <djones@iac.es>, Michael Abdul-Masih <michael.abdul-masih@eso.org>, Bert Pablo <hpablo@aavso.org>, Joe Giammarco <giammarc@eastern.edu> | ||
| ### 2.4.22 | ||
| * Fixes bug where LS periodogram was returning frequency instead of period [#1089] | ||
| * Fixes passband luminosity computation for the dataset-scaled mode. [#1091] | ||
| * Fixes third light computation when multiple passbands are used. [#1091] | ||
| * Argument order for compute_l3s() changed to explicitly provide the model as it is required for correct scaling. [#1091] | ||
| * Fixes support for newer releases of scipy. [#1102] | ||
| ### 2.4.21 | ||
@@ -129,0 +137,0 @@ |
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-1
@@ -14,3 +14,3 @@ # PHOEBE build specification | ||
| name = "phoebe" | ||
| version = "2.4.21" | ||
| version = "2.4.22" | ||
| description = "PHOEBE: modeling and analysis of eclipsing binary stars" | ||
@@ -17,0 +17,0 @@ readme = "README.md" |
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@@ -81,2 +81,10 @@ PHOEBE 2.4 | ||
| ### 2.4.22 | ||
| * Fixes bug where LS periodogram was returning frequency instead of period [#1089] | ||
| * Fixes passband luminosity computation for the dataset-scaled mode. [#1091] | ||
| * Fixes third light computation when multiple passbands are used. [#1091] | ||
| * Argument order for compute_l3s() changed to explicitly provide the model as it is required for correct scaling. [#1091] | ||
| * Fixes support for newer releases of scipy. [#1102] | ||
| ### 2.4.21 | ||
@@ -83,0 +91,0 @@ |
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