# FRETBursts Release Notes¶

## Version 0.6.3 (Apr. 2017)¶

A few more small fixes in this release. If you have any installation issue please report it on github.

• Import OpenFileDialog when FRETBursts is imported (as in versions < 0.6.2)
• Use phconvert to decode SM files

## Version 0.6.2 (Apr. 2017)¶

This is a technical release that removes the hard dependency on QT and solves some installation issues due to QT pinning on conda-forge.

## Version 0.6.1 (Apr. 2017)¶

For this version of FRETBursts, conda packages are distributed for python 2.7, 3.5, 3.6 and numpy 1.11 and 1.12. FRETBursts still works with python 3.4 but conda packages are not provided anymore. Python 2.7 is now deprecated. Support for python 2.7 will be removed in a future version.

The current release includes the following changes:

• SangYoon Chung (@chungjjang80) found that the L argument in burst search was ignored and submitted a fix to the problem in PR #57. Tests were added to avoid future regressions.
• Fix access to the deprecated background attributes (introduced in 0.6). See b850a5.
• Add plot wrapper for 16-ch data.
• Improved example notebook showing how to export burst data. See Exporting Burst Data.
• Re-enable background rate caching. See PR #53.
• Support Path objects as filename in loader.photon_hdf5(). See 201b5c.
• Improve Ph_sel string representation, added factory method Ph_sel.from_str and added new tests. See 3dc5f0.

## Version 0.6 (Jan. 2017)¶

• Improvements to the layout of 48-spot plots.
• Simplify background computation avoiding useless recomputations. This results in 3x speed increase in background computation for measurement loaded with ondisk=True and 30% speed increase when using ondisk=False. Now all background rates are stored in the dictionary Data.bg, while the mean background rate in the dictionary Data.bg_mean. The old attributes Data.bg_* and Data.rate_* have been deprecated and will be removed in a future release (see below).
• Fix loading files with ondisk=True. With this option timestamps are not kept in RAM but loaded spot-by-spot when needed. This option has no effect on single-spot measurements but will save RAM in multi-spot measurements.
• Add new plot functions hist_interphoton and hist_interphoton_single to plot the interphoton delay distribution. In previous versions the function hist_bg (and hist_bg_single) did the same plot but required the background to be fitted. hist_interphoton* do not require any prior background fit and also have a cleaner and improved API.
• Detect and handle smFRET files (no ALEX) with counts not only in D or A channels (f0e33d).
• Better error message when a burst filtering function fails (c7826d).

### Backward-incompatible changes¶

#### Details of auto-threshold changes¶

The refactor included a change in how the background is computed when using tail_min_us='auto'. As before, with this setting, the background is estimated iteratively in two steps. A first raw estimation with a fixed threshold (250us), and second estimation with a threshold function of the rate computed in the first step. Before version 0.6, the first step estimated a single rate for the whole measurement. Now the first-step estimation is performed in each background period separately. As before, the second step computes the background separately in each background period. This change was motivated by the need to simplify the internal logic of background estimation, and to increase the computation efficiency and accuracy.

#### Background attributes¶

The background refactor resulted in an incompatible change in the Data.bg attribute. Users upgrading to version 0.6, may need to replace Data.bg with Data.bg[Ph_sel('all')] in their notebooks. Note that no official FRETBursts notebook was using Data.bg, so most users will not be affected.

#### Compatibility layer¶

All the old background-related attributes (bg_dd, bg_ad, bg_da, bg_aa, rate_dd, rate_ad, rate_da, rate_aa, rate_m) are still present but deprecated. The same data is now contained in the dictionaries Data.bg and Data.bg_mean. When using the deprecated attributes, a message will indicate the new syntax. If you see the deprecation warning, please update the notebook to avoid future errors.

#### Details of changed attributes¶

Before version 0.6, Data.bg contained background rates fitted for all-photons stream. Data.bg was a list of arrays: one array per spot, one array element per background period. In version 0.6+, Data.bg contains the background rates for all the fitted photon streams. Data.bg is now a dict using Ph_sel objects as keys. Each dict entry is a list of array, one array per spot and one array element per background period. For more details please refer to the following documentation Data.bg and Data.bg_mean.

## Version 0.5.9 (Sep. 2016)¶

• Added support for pyqt and qt 5+.
• Fix burst selection with multispot data. See this commit.

There may still be some glitches when using the QT5 GUIs from the notebook, but installing (and importing) FRETBursts does not require QT4 anymore (QT5 is the current default in anaconda). Please report any issue.

## Version 0.5.7 (Sep. 2016)¶

Refactoring and expansion of gamma and beta corrections. Briefly, in all the places where corrected burst sizes are being computed, we removed the gamma1 argument and added a flag donor_ref. Additionally, the values Data.S are now beta corrected.

These changes affected several components as described below.

### Data Class¶

• Methods Data.burst_sizes_ich and Data.burst_sizes now accept the arguments gamma, beta and donor_ref. The argument gamma1 was removed. The two conventions of corrected burst sizes are chosen with the boolean flag donor_ref. See the burst_sizes_ich docs for details.
• New method get_naa_corrected returns the array of naa burst counts corrected with the passed gamma and beta values. Like for the burst size, the argument donor_ref selects the convention for the correction. See the get_naa_corrected docs for details.
• A new Data attribute beta (default: 1) stores a beta value that is used to compute the corrected S. This value is never implicitly used to compute corrected burst sizes or naa (for these a beta arguments needs to be passed explicitly).

### Plot functions¶

Plot functions hist_size and hist_brightness accept the new arguments for corrected burst size (gamma, beta and donor_ref).

### Burst selection¶

Burst selection by size and naa accept the new arguments for corrected burst size (gamma, beta and donor_ref).

### Burst Weights¶

Functions that accept weights don’t accept the gamma1 argument anymore, but they don’t (yet) support the arguments donor_ref and beta. As a result, for the purpose of weighting, there is only one expression for corrected burst size (na + gamma*nd), with the option to add naa but without beta correction.

All these changes are covered by unit tests.

### Installation via conda-forge¶

Since version 0.5.6 we started distributing conda packages for FRETBursts through the conda-forge channel (a community supported repository, as opposed to a private channel we were using before). To install or update FRETBursts you should now use:

conda install fretbursts -c conda-forge


Using the conda-forge channel simplifies our release process since their infrastructure automatically builds packages for multiple platforms and python versions. Please report any issues in installing or upgrading FRETBursts on the GitHub Issues page.

For more detailed installation instructions see the Getting Started documentation.

## Version 0.5.6¶

For older release notes see GitHub Releases Page.