Keaton Bell
@astrokeat.bsky.social
180 followers 210 following 37 posts
astronomer to the stars
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astrokeat.bsky.social
My Python environment.
astrokeat.bsky.social
Great to revisit this photo! Many people I now know in the field whom I don't recall meeting at this, one of my first real science meetings.
astrokeat.bsky.social
RIP to Bill Paxton, lead developer of MESA. I feel privileged to have learned from the man himself at the 2012 MESA Summer School. #stellarastro #astrocode
astrokeat.bsky.social
A minor update to Pyriod is now available (v0.3.3), addressing some pesky depreciation warnings that would crop up. pypi.org/project/Pyri...
astrokeat.bsky.social
Also another notebook showing how to automate prewhitening analysis (I will try to build more convenience functions into Pyriod for this soon). github.com/keatonb/Pyri...
astrokeat.bsky.social
For this presentation, I have also uploaded a demonstration of how to use Pyriod to measure O-C diagrams to track timing variations of a signal. github.com/keatonb/Pyri...
astrokeat.bsky.social
At the 9th TESS/16th Kepler Asteroseismic Science Consortium Workshop this week in Vienna. I'm presenting this poster on my code Pyriod for pre-whitening frequency analysis of astronomical time series data. #astromethods
Reposted by Keaton Bell
vrubinobs.bsky.social
Here it is: the first set of riches from Rubin's Cosmic Treasure Chest!

Introducing NSF–DOE Rubin Observatory's first wide and deep view of the cosmos, the southern region of the Virgo Cluster.

Rubin produced this image in just 10.5 hours over parts of 7 nights! 🔭🧪

youtu.be/Gitit3LwQ20
astrokeat.bsky.social
I present the #astrocode Pyriod for interactive or scripted pre-whitening frequency analysis of astronomical time series data. See the demo of #stellarastro #TESS data analysis of a pulsating white dwarf star. Check it out at github.com/keatonb/Pyriod/.
astrokeat.bsky.social
Had to withdraw my #AAS246 poster due to COVID, but let me demo "Pyriod: Interactive Pre-Whitening Frequency Analysis in Python." Here is a quick guide to reproducing the analysis of TESS data on a pulsating white dwarf from Bell et al. (2019, ui.adsabs.harvard.edu/abs/2019A%26A...632A..42B).
astrokeat.bsky.social
Check out the #AAS246 iPoster "White Dwarf Asteroseismology in the Age of Gaia Astrometry" from Andrew Dublin, Agnes Bischoff-Kim and myself: aas246-aas.ipostersessions.com/Default.aspx...

#stellarastro
aas (iPosterSessions - an aMuze! Interactive system)
aas246-aas.ipostersessions.com
astrokeat.bsky.social
Check out the #AAS246 iPoster "TESS CROWDSAP Errors from White Dwarf Observations" from Nikoo Hosseininezhad and myself: aas246-aas.ipostersessions.com/default.aspx...

#stellarastro
aas (iPosterSessions - an aMuze! Interactive system)
aas246-aas.ipostersessions.com
astrokeat.bsky.social
The development of Pyriod is supported by the National Science Foundation under Grant No. AST-2406917.
astrokeat.bsky.social
The interface works in Jupyter, and it can also be scripted for automated analysis. We are grateful to lightkurve, astropy, lmfit, qgrid, and qgridnext, which make Pyriod work. I am working to improve tutorials and documentation. Submit issues/feature requests at github.com/keatonb/Pyriod
GitHub - keatonb/Pyriod: Python implementation of basic period detection and fitting routines for astronomical time series.
Python implementation of basic period detection and fitting routines for astronomical time series. - keatonb/Pyriod
github.com
astrokeat.bsky.social
Pyriod is inspired by Period04 (www.period04.net), aiming to provide a similar interactive data analysis experience for the modern Python workflow, with open-source code, and with a faster periodogram better-suited for the big data era.
Period04 - Homepage
www.period04.net
astrokeat.bsky.social
Our reward for completing this process is a table of signal frequencies, amplitudes, and phases, with estimated uncertainties. These measurements of resonant frequencies of a white dwarf star are published and interpreted in Bell et al. (2019, ui.adsabs.harvard.edu/abs/2019A%26A...632A..42B).
astrokeat.bsky.social
The fit to the light curve reveals the complex variability that we otherwise couldn't visibly see for all the measurement noise, shown here for one day of the TESS light curve.
astrokeat.bsky.social
Pyriod can enforce strict relationships between combination frequencies and independent frequencies when they are identified by their arithmetic relations. We proceed to pre-whiten all significant signals, with combinations marked with gold diamonds.
astrokeat.bsky.social
Three signals down, but the next three are "combination frequencies" that appear at precise sums, multiples, and differences of frequencies. If the first three signals are f0, f1, and f2, this next cluster of peaks are f0+f1, 2*f0, and f0+f2.
astrokeat.bsky.social
We then identify additional signals from the periodogram of fit residuals (the "pre-whitened" data). Pyriod displays the periodogram of the residuals in blue (highest peak marked). The model is displayed in green. In practice, we move significant peaks from blue to green.
astrokeat.bsky.social
We "pre-whiten" signals by fitting and subtracting sinusoids from the light curve. We currently fit the frequency, amplitude, and phase of one sinusoidal signal. The data may be noisy, but TESS collected enough that we detect this signal to high significance.
astrokeat.bsky.social
The periodogram displays the frequency content of the light curve, and we identify significant signals as having amplitudes well above the noise floor. The red curve gives an approximate significance threshold, and Pyriod marks the highest peak for inclusion in the model. Let's add it.
astrokeat.bsky.social
The pre-whitening algorithm is a method for measuring sinusoidal signals in time series data. It is best suited for signals that are coherent for the duration of the observations. We start with the periodogram of the TESS Sector 3 light curve of the pulsating white dwarf WD 0158-160.
astrokeat.bsky.social
Had to withdraw my #AAS246 poster due to COVID, but let me demo "Pyriod: Interactive Pre-Whitening Frequency Analysis in Python." Here is a quick guide to reproducing the analysis of TESS data on a pulsating white dwarf from Bell et al. (2019, ui.adsabs.harvard.edu/abs/2019A%26A...632A..42B).