p-winds is a Python implementation of Parker wind models for planetary atmospheres. New in the 0.5-beta version: Transit simulation Radiative transfer to calculate the in-transit signal of the Helium triplet in 1.083 microns New in the 0.5.2-beta version: Added the necessary configuration to allow conda-forge and Travis CI routine
This is the final alpha release, where the steady-state population of helium was implemented. The ne...
Changelog: Added option to scale MUSCLES spectra to arbitrary stellar radii Implemented a v_guess r...
We have recently received the referee report of our manuscript submitted for peer-review on Astronom...
p-winds is a Python implementation of Parker wind models for planetary atmospheres. New in the 0.5-b...
p-winds is a Python implementation of Parker wind models for planetary atmospheres. New in the 0.5-b...
p-winds is an open-source Python implementation of Parker wind models for planetary atmospheres, mor...
p-winds is a Python implementation of Parker wind models for planetary atmospheres. New in the 0.6.4...
p-winds is a Python implementation of Parker wind models for planetary atmospheres. New in the 0.5.4...
p-winds is a Python implementation of Parker wind models for planetary atmospheres. New in the 0.6.2...
p-winds is a Python implementation of Parker wind models for planetary atmospheres. New in the 0.5.3...
This is a beta test of the version 1.3.0 of p-winds. Here is the changelog: parker.py was updated w...
After a long period of development, we are proud to release the first stable, production-level versi...
This is the pre-release version of p-winds 1.2. New in this version: hydrogen.py requires a first g...
This new version is an update based on the referee report of the manuscript submitted to Astronomy &...
This is a patch for the pre-release version of p-winds 1.2. New in this version: Corrected the impl...
This is the final alpha release, where the steady-state population of helium was implemented. The ne...
Changelog: Added option to scale MUSCLES spectra to arbitrary stellar radii Implemented a v_guess r...
We have recently received the referee report of our manuscript submitted for peer-review on Astronom...
p-winds is a Python implementation of Parker wind models for planetary atmospheres. New in the 0.5-b...
p-winds is a Python implementation of Parker wind models for planetary atmospheres. New in the 0.5-b...
p-winds is an open-source Python implementation of Parker wind models for planetary atmospheres, mor...
p-winds is a Python implementation of Parker wind models for planetary atmospheres. New in the 0.6.4...
p-winds is a Python implementation of Parker wind models for planetary atmospheres. New in the 0.5.4...
p-winds is a Python implementation of Parker wind models for planetary atmospheres. New in the 0.6.2...
p-winds is a Python implementation of Parker wind models for planetary atmospheres. New in the 0.5.3...
This is a beta test of the version 1.3.0 of p-winds. Here is the changelog: parker.py was updated w...
After a long period of development, we are proud to release the first stable, production-level versi...
This is the pre-release version of p-winds 1.2. New in this version: hydrogen.py requires a first g...
This new version is an update based on the referee report of the manuscript submitted to Astronomy &...
This is a patch for the pre-release version of p-winds 1.2. New in this version: Corrected the impl...
This is the final alpha release, where the steady-state population of helium was implemented. The ne...
Changelog: Added option to scale MUSCLES spectra to arbitrary stellar radii Implemented a v_guess r...
We have recently received the referee report of our manuscript submitted for peer-review on Astronom...
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