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Releases: nanograv/PINT

1.0

26 Apr 18:08
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Full Changelog: 0.9.8...1.0

v0.9.8

04 Dec 19:09
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Full Changelog: 0.9.7...0.9.8

v0.9.7

24 Aug 21:50
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0.9.6

22 Jun 23:59
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v0.9.5

01 May 14:20
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[0.9.5] 2023-05-01

Changed

  • Changed minimum supported version of scipy to 1.4.1
  • Moved DMconst from pint.models.dispersion_model to pint to avoid circular imports
  • Removed references to astropy._erfa (removed since astropy 4.2)
  • Refactor Dre method, fix expressions for Einstein delay and post-Keplerian parameters in DD model
  • Updated contributor list (AUTHORS.rst)
  • Emit an informative warning for "MODE" statement in TOA file; Ignore "MODE 1" silently
  • Version of sphinx-rtd-theme updated in requirements_dev.txt
  • Updated black version to 23.x
  • Older event loading functions now use newer functions to create TOAs and then convert to list of TOA objects
  • Limited hypothesis to <= 6.72.0 to avoid numpy problems in oldestdeps

Added

  • Documentation: Explanation for DM
  • Methods to compute dispersion slope and to convert DM using the CODATA value of DMconst
  • TimingModel.total_dispersion_slope method
  • Explicit discussion of DT92 convention to DDK model
  • HAWC, HESS and ORT telescopes to the list of known observatories
  • Documentation: making TOAs from array of times added to HowTo
  • Method to make TOAs from an array of times
  • Clock correction for LEAP
  • Wideband TOA simulation feature in pint.simulation and zima
  • ELL1k timing model
  • Test for MCMCFitter
  • Added multiprocessing capability to event_optimize
  • Can merge TOAs using '+' operator; in-place merge using '+=' operator
  • funcParameters defined as functions operating on other parameters
  • Option to save emcee backend chains in event_optimize
  • Documentation on how to extract a covariance matrix
  • DDS and DDGR models
  • Second-order corrections included in ELL1
  • Module for converting between binary models also included in convert_parfile
  • Method to get a parameter as a uncertainties.ufloat for doing math
  • Method to get current binary period and uncertainty at a given time regardless of binary model
  • TCB to TDB conversion on read, and conversion script (tcb2tdb)
  • Functions to get TOAs objects from satellite data (Fermi and otherwise)
  • Methods to convert a TOAs object into a list of TOA objects

Fixed

  • Syntax error in README.rst
  • Broken notebooks CI test
  • BIPM correction for simulated TOAs
  • Added try/except to test_pldmnoise.py/test_PLRedNoise_recovery to avoid exceptions during CI
  • Import for longdouble2str in get_tempo_result
  • Plotting orbital phase in pintk when FB0 is used instead of PB
  • Selection of BIPM for random models
  • Added 1 sigma errors to update the postfit parfile errors in event_optimize
  • Fixed DDS CI testing failures
  • Add SolarSystemShapiro to the timing model only if an Astrometry component is present.

Full Changelog: 0.9.3...0.9.5

v0.9.3

16 Dec 23:45
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v0.9.2

30 Nov 18:16
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Full Changelog: 0.9.1...0.9.2

v0.9.1

12 Aug 18:33
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PINT Release version 0.9.1

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Full Changelog: 0.9.0...0.9.1

v0.9.0

24 Jun 16:25
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Major changes in this release include dropping support for Python version less than 3.8 and use of the global clock file repository instead of distributing clock files with PINT or relying on TEMPO/Tempo2.

v0.8.8

02 Jun 12:00
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Version 0.8.8 of PINT. Contains many improvements to the GUI as well as many other fixes.

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Full Changelog: 0.8.7...0.8.8