REVIEW 5 cited by
Probabilistic Programming in Python using PyMC
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
Probabilistic programming (PP) allows flexible specification of Bayesian statistical models in code. PyMC3 is a new, open-source PP framework with an intutive and readable, yet powerful, syntax that is close to the natural syntax statisticians use to describe models. It features next-generation Markov chain Monte Carlo (MCMC) sampling algorithms such as the No-U-Turn Sampler (NUTS; Hoffman, 2014), a self-tuning variant of Hamiltonian Monte Carlo (HMC; Duane, 1987). Probabilistic programming in Python confers a number of advantages including multi-platform compatibility, an expressive yet clean and readable syntax, easy integration with other scientific libraries, and extensibility via C, C++, Fortran or Cython. These features make it relatively straightforward to write and use custom statistical distributions, samplers and transformation functions, as required by Bayesian analysis.
Forward citations
Cited by 5 Pith papers
-
Requirements for Joint Orbital Characterization of Cold Giants and Habitable Worlds with Habitable Worlds Observatory
Simulations of 164 nearby target stars set HWO design requirements: an outer working angle of 1440 milliarcseconds, 40 precursor radial velocity measurements, and 6-8 astrometric epochs to pin down cold giant orbits.
-
The TOI-1117 Multi-planetary System: 3 sub-Neptunes, 1 in both the Neptunian Desert and Radius Valley
Three sub-Neptune planets orbit TOI-1117; the transiting inner planet sits in both the Neptunian Desert and Radius Valley, and its photoevaporation history favors a water-rich interior.
-
Statistics on the population of distant substellar companions to nearby stars
Wide substellar companions around nearby stars follow power-law mass and separation distributions consistent with stellar binaries, with an occurrence rate of about 1% at 1,000–20,000 AU.
-
In Search of Decay: An Analysis of Transit Times of Hot Jupiters in Main Sequence and Post-Main Sequence Systems
A TESS transit-timing survey of 54 hot Jupiter systems finds 8 candidates with orbital decay at three-sigma significance and derives lower limits on the stellar tidal quality factor Q*'.
-
Searching for GEMS: TOI-5916 b & TOI-6158 b are two Saturn-density planets orbiting M2 dwarfs
TOI-5916 b and TOI-6158 b are confirmed gas giants around M2 dwarfs with Saturn-like densities, on 2.37- and 3.04-day orbits.
Discussion (0). Continue with ORCID to comment.