Docs: performance

docs/index.rst

@@ -36,6 +36,7 @@ Learn more about contributing to this repository in our :doc:`Contribution Guide
    Installation <installation>
    Getting Started <tutorials/quickstart>
    Tutorials <tutorials>
+   Performance <performance>
 
 .. toctree::
    :hidden:

docs/performance.rst

@@ -0,0 +1,76 @@
+Performance
+===========
+
+LSDB is a high-performance package built to support the analysis of large-scale astronomical datasets.
+One of the performance goals of LSDB is to add as little overhead over the input-output operations as possible.
+We achieve this aim for catalog cross-matching, spatial and data filtering operations by using
+the `HiPSCat <https://github.com/astronomy-commons/hipscat>`_ data format,
+efficient algorithms,
+and `Dask <https://dask.org/>`_ framework for parallel computing.
+
+Here we demonstrate the results of the performance tests of LSDB for the cross-matching operations,
+performed on `Bridges2 cluster at Pittsburgh Supercomputing Center <https://www.psc.edu/resources/bridges-2/>`_ using single node with 128 cores and 256 GB of memory.
+
+Cross-matching performance overhead
+-----------------------------------
+
+We compare I/O speed and cross-matching performance of LSDB on an example of cross-matching of
+ZTF DR14 (metadata only, 1.2B rows, 60GB)
+and Gaia DR3 (1.8B rows, 972GB) catalogs.
+The cross-matching took 46 minutes and produced a catalog of 498GB.
+While the cross-matching optimized reading of Gaia and didn't load southern part of the Gaia which doesn't overlap with ZTF,
+we would judge the performance by the output size, which gives us 185MB/s of the cross-matching speed.
+
+We compare it to just copying both catalogs with `cp -r` command, which took 86 minutes and produced 1030GB of data,
+which corresponds to 204MB/s of the copy speed.
+These allow us to conclude that LSDB cross-matching overhead is 5-15% compared to the I/O operations.
+
+The details of this analysis are given in
+`this note <https://github.com/lincc-frameworks/notebooks_lf/blob/ac5f91e3100aeaff5a5028b357dce08489dcab5b/sprints/2024/02_22/banch-vs-cp.md>`_.
+
+LSDB's cross-matching algorithm performance versus other tools
+--------------------------------------------------------------
+
+We compare the performance of LSDB's default cross-matching algorithm with
+`astropy`'s `match_coordinates_sky <https://docs.astropy.org/en/stable/api/astropy.coordinates.match_coordinates_sky.html>`_
+and `smatch <https://github.com/esheldon/smatch>`_ package.
+
+We use the same ZTF DR14 and Gaia DR3 catalogs as in the previous test, but we only use coordinate columns for the cross-matching.
+With each algorithm, we perform the cross-matching of the catalogs within a 1 arcsecond radius, selecting the closest match.
+To compare the performance on different scales,
+we select subsets of the catalogs with cone search around an arbitrary point,
+ranging the radius from 1 arcminute to 25 degrees.
+
+The analysis has the following steps:
+
+* Load the data from the HiPSCat format, selecting the subset of the data with ``lsdb.read_hipscat(PATH, columns=[RA_COL, DEC_COL]).cone_search(ra, dec, radius).compute()``.
+* Perform the cross-matching with the selected algorithm
+
+  * LSDB: ``ztf.crossmatch(gaia, radius_arcsec=1, n_neighbors=1).compute()``
+  * Astropy analysis is two-step:
+
+    * Initialize the ``SkyCoord`` objects for both catalogs
+    * Perform the cross-matching with ``match_coordinates_sky(ztf, gaia, nthneighbor=1)``, filter the results by 1-arcsencod radius, and compute distances
+
+  * Smatch: ``smatch.match(ztf_ra, ztf_dec, 1/3600, gaia_ra, gaia_dec)``, and convert distances from cosines of the angles to arcseconds
+
+The results of the analysis are shown in the following plot:
+
+.. figure:: _static/crossmatching-performance.png
+   :class: no-scaled-link
+   :scale: 100 %
+   :align: center
+   :alt: Cross-matching performance comparison between LSDB, astropy, and smatch
+
+Some observations from the plot:
+
+* Construction of the ``SkyCoord`` objects in astropy is the most time-consuming step, on this step spherical coordinates are converted to Cartesian, so `match_coordinates_sky` has less work to do comparing to other algorithms. So if your analysis doesn't require the ``SkyCoord`` objects anywhere else, it would be more fair to add up the time of the `SkyCoord` objects construction and the `match_coordinates_sky` execution.
+* All algorithms but LSDB have a nearly linear dependency on the number of rows in the input catalogs starting from a small number of rows. LSDB has a constant overhead associated with the graph construction and Dask overhead, which is negligible for large catalogs, where the time starts to grow linearly.
+* LSDB is the only method allowing to parallelize the cross-matching operation, so we run it with 1, 4, 16, and 64 workers.
+* 16 and 64-worker cases show the same performance, which shows the limits of the parallelization, at least with the hardware setup used in the analysis.
+* Despite the fact that LSDB's crossmatching algorithm does more job converting spherical coordinates to Cartesian, it's getting faster than astropy's algorithm for the large catalogs, even with a single worker. This is probably due to the fact that LSDB utilises batching approach, which allows to grow less deep k-D trees for each partition of the data, and thus less time is spent on the tree traversal.
+
+Summarizing, the cross-matching approach implemented in LSDB is competitive with the existing tools and is more efficient for large catalogs, starting with roughly one million rows.
+Also, LSDB allows to work with out-of-memory datasets, which is not possible with astropy and smatch, and not demonstrated in the analysis.
+
+The complete code of the analysis is available `here <https://github.com/lincc-frameworks/notebooks_lf/tree/main/sprints/2024/05_30/xmatch_bench>`_.