Hey everyone,
> Alexandre, something that I want to emphasise right now is that I
>
would like to consider the next ~12-24 months a sprint to 1.0.
>
Therefore, I want to avoid as much as possible taking on new
> technical
debt and focus on fixing/cleaning everything we have so
> far, according
to our (as yet not ratified) values. [1]
We're in the same page, Juan :) Thinking on that, it would be
interesting to have something on our model close to Debian Linux's
release cycle. We'd work on and receive major contributions up to a
certain point (let's say, the next 6-12 months). Then, we clean and
debug everything we can, not accepting new major code for that release;
it'll be something like Debian's frozen cycle. But I'm digressing.
Kind regards,
Alex
On Wed, 2019-08-07 at 00:24 -0500, Juan Nunez-Iglesias wrote:
> Thanks Mark for raising this and Lars and Alex for weighing in.
>
> On Mon, 5 Aug 2019, at 5:40 AM, Alexandre de Siqueira wrote:
> > > > I think what is important is to keep the API forward looking
> > > > for
> > > > ND. We can do things like accept tuples for parameters, instead
> > > > of
> > > > "x_center", "y_center", or "r_center", "c_center". We can also
> > > > just throw errors when people pass in higher dimensions images
> > > > saying that it isn't implemented and contributions are welcome.
> > >
> > > I think this is critical and really like this compromise. Don't
> > > do
> > > more work than is actually needed while not making future work
> > > harder. Equally critical to me is that whether a function
> > > supports
> > > ND or only 2D is clearly documented. Maybe after a parameter's
> > > type
> > > declaration in the docstring?
> >
> > I guess these are all good solutions for us right now. I'm sure
> > that
> > we'll break, fix and clean lots of stuff/code/API until we reach
> > 1.0
> > (and that is okay™). This problems will be tackled naturally on the
> > way.
>
> I agree with Lars, keeping the *API* nD-compatible is already a very
> good step towards keeping the Guardian of the Dimensions happy. =P
> Great suggestion, Mark!
>
> Alexandre, something that I want to emphasise right now is that I
> would like to consider the next ~12-24 months a sprint to 1.0.
> Therefore, I want to avoid as much as possible taking on new
> technical debt and focus on fixing/cleaning everything we have so
> far, according to our (as yet not ratified) values. [1]
>
> > > > Optimizing for the different use cases is just tricky, and
> > > > won't
> > > > be done correctly if contributors are asked to include
> > > > something
> > > > they have no immediate need for.
> >
> > We can help in some of these cases. If we (core group) can't, we
> > can:
> > 1. discuss if the algorithm is ready as-is to be included and
> > upgraded
> > from there; 2. ask for external community help.
>
> My main idea is that I am happy to jump in and make things nD at the
> PR stage. However, I don't have the bandwidth to do this for *all*
> contributions and help is always appreciated. This is why it's
> important to be on the same page.
>
> Additionally, as I raised in the SEEDS PR [2], a contribution might
> be worthwhile in nD but not worthwhile in 2D, because 2D
> implementations in Python already exist. (And in this case they have
> a good chance of being faster than ours!) We are having enough
> trouble keeping up with the maintenance burden as it is, so the value
> of new contributions to the community should be weighed against the
> maintenance burden.
>
> It might be time to revisit the idea of skimage-contrib, a repo in
> which functions that don't quite meet this benchmark can live, until
> they are ready to graduate.
>
> > > In that vein, wasn't there a discussion about writing a guide on
> > > ND-algorithms (e.g. the raveled approach used in watershed,
> > > local_maxima, flood_fill)? Was there any progress on this? I
> > > think
> > > this could be really useful to the community and a good resource
> > > for new contributors regardless of how skimage's policy on this
> > > turns out.
> >
> > +1. Or even, contributors aiming to enhance our 3D/nD
> > possibilities,
> > only :)
>
> Yes, I mentioned that I should write a guide and here we are, no
> further along. Apologies for that. I'll prioritise this work for the
> summer/fall. If we have an easy guide, including pointing to PRs or
> commits that convert code to nD, that will make things a lot easier.
>
> Juan.
>
> .. [1] https://github.com/scikit-image/scikit-image/pull/3585
> .. [2] https://github.com/scikit-image/scikit-image/pull/1557
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--
--------------------------------------------------
Dr. Alexandre de Siqueira
Berkeley Institute for Data Science - BIDS
190 Doe Library
University of California, Berkeley
Berkeley, CA 94720
United States
Lattes CV: 3936721630855880
ORCID: 0000-0003-1320-4347
Github: alexdesiqueira
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