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Ruth Angus

Login: RuthAngus

Company: Columbia University

Location: Brooklyn, NY

Bio: null

Blog:

Member of

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Repositories

acf: Code for calculating autocorrelation functions.
action-time: Comparing kinematic ages with gyrochronal ages.
agemap: An age map of the Milkyway
alphacen: null
arxiv-alerts: null
asteroseismology: null
astrobites: Cos I need version control for everything I write
astro-viz: Astronomical data visualizations
beetchips: Modelling star spots
BlackHoleGP: Black hole GP stuff
celerite: Scalable 1D Gaussian Processes in C++, Python, and Julia
celerotation: Inferring rotation periods at light-speed
CfAML: Collaborative repository for the Machine Learning Reading group at CfA
chronometer: A coherent and comprehensive dating system for the stars in the Milky Way.
codebox: Code snippets
collabeat: Collaborative Beatz
CUWiP: null
datarecipes: Exercises from Hogg's paper
detrending: Light curves and detrending at #exosamsi
dfm.github.com: null
dotvim: my dotvim
emcee: The Python ensemble sampling toolkit for affine-invariant MCMC
EPRV: Codez written for the #EPRVmtg
exoplanet_travel: null
exopop: Inferring the population of exoplanets
extragalactic: Extragalactic planets
Fakespeare: Shakespeare lives
far-out: Things with wavelets
fgkcupid: A dating service for stars.
flicker: HBM with flicker
Fruitcake: Let's weight Phil!
gaia_astero: A catalogue of Gaia stars with asteroseismic parameters.
gaia-binaries: Identifying and exploring wide and close binaries in Gaia DR1
GAIA-sprints: Comparing gyro-iso-astero ages for stars in the first GAIA data release
gaia-wide-binaries: Measuring rotation periods for wide binaries and co-moving groups in TGAS
G-bomb: Gaia sprints
george: Fast Gaussian Processes for regression
GP_examples: null
GProtation: Measuring stellar rotation periods with Gaussian processes
GPtutorial: Gaussian process tutorial materials
granola: Calibrating MS ages using galactic dynamics with Gaia, Kepler and APOGEE
Gyro: Calibrating Gyrochronology using Kepler Asteroseismic targets
Gyro_demo: Demonstrating gyro useage
gyroscope: Mapping out (scoping) the future and potential of gyrochronology
habitablezoning: null
HotStarsInc: Do the exoplanets orbiting F stars have larger inclinations?
interwebz: Experiments with websites
ischrones: null
isochrone_viz: Online isochrone visualisation
K2rotation: Measuring K2 rotation periods
K-ACF: Auto-correlation functions for Kepler data
kalesalad: Measuring K2 rotation periods.
KeplerGP: Detrending Kepler data using Gaussian Processes
KeplerMusic: More Kepler Sonification
KeplerPORTs: Kepler Planet Occurrence Rate Tools
keplerstars: Playing around with the Kepler catalogue and light curve properties
kpm: null
lightcurvecannon: null
lightcurvecannon-1: null
LSSTease: Asteroseismology with LSST
LSST-max: Maximising science in the LSST era
M35: Measuring rotation periods in M35
Mdwarfs: M dwarfs are cool
myCV: my CV, copied from DFM.
nestle: Python implementation of nested sampling algorithms for evaluating Bayesian evidence
ngc6791: Extracting photometry from a cluster superstamp
ObservingStrategy: A community white paper about LSST observing strategy, with quantifications via the the Metric Analysis Framework.
outreach: Codes for outreach
plotstuff: null
Prob-tools: null
Python-Labs: Tim Morton's python labs
RandomForestEB: null
ruthangus.github.io: null
sassenach: A catalogue of rotation periods for K2 stars
SaveKepler: a whitepaper in response to the "repurpose Kepler" call
Sigourney: The systematics-insensitive Gaussian process periodogram
SIPK2: Systematics-Insensitive Periodograms for K2
smugness: Delivering smugness around the globe
Subgiants: Investigating the population of planets around subgiants
SweetPotato: null
teacups: Testing gyrochronology with Gaia comoving pairs
TESSproposal: A TESS proposal
thesis: My PhD thesis on stellar ages and stellar rotation.
trollbot: null
turnip: Exoplanet ages
wdf: Finding white dwarf companions in TGAS
wfirst_stars: null
yobot3k: Yo-ing the astronomy facts!

Commits To

Repository	Most Recent Commit	# Commits

This work is supported by the National Institutes of Health's National Center for Advancing Translational Sciences, Grant Number U24TR002306. This work is solely the responsibility of the creators and does not necessarily represent the official views of the National Institutes of Health.