v1.0.31

update

1.0.29

Thanks to @lgbouma for adding a parameter verbose=True for a silent run.

1.0.28

• Relaxed constraints on minimum stellar mass, stellar radius and planetary period. TLS can now be used to search for periods shorter than 0.6 days. Example usage:

model = transitleastsquares(t, y)
results = model.power(
    R_star_min=0.05,
    M_star_min=0.05,
    R_star_max=0.2,
    M_star_max=0.2,
    M_star=0.1,
    R_star=0.1,
    period_min=0.1,
    period_max=1,
    )

This will generate a grid of 698842 periods from 0.1 to 1.0 days. Attention: short periods require dense grid, which are computationally expensive.

• Added compatibility with Python 3.9

1.0.26

Fixed a bug in oversampling_factor which now also accepts floating point values

1.0.25

Fixed a bug reported by @MNGuenther which prevented the check of shortest transit durations for short-period planets around low-mass stars.

1.0.24

Thanks to Thanks to @keatonb for bugfix: mass reassignment outside of allowed bounds #78

1.0.23

Fixed: A bug in the post-detection statistics which caused a delay in large dataset (e.g., Kepler K1)

1.0.21

• Fixed: A bug in cleaned_array which caused an error in case invalid dy values were supplied. Relevant for TESS FITS files. These should now run including uncertainties.
• Added: New statistics: before_transit_count, in_transit_count, after_transit_count yield the number of data points in a bin of length transit duration before, in and after the phase-folded transit.
• Added: New parameter show_progress_bar (bool, default: True) When set to False, no progress bar (using tqdm) will be shown
• Added: Python 2 compatibility. For now, it is only single-core.

1.0.20

• Fixed: A bug which erroneously interchanged power and power_raw

1.0.19

• Fixed: A bug in the calculation of statistics which caused TLS to stall in some cases