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20182026
most citedThe EXPRES Stellar Signals Project II. State of the Field in Disentangling Photospheric Velocities

61 citations · 315 across the 27 of their papers we have counts for

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Showing astro-ph.IMShow all

9 papers · 1 filter

astro-ph.IM2023★ 8 cited

Practical Guidance for Bayesian Inference in Astronomy

Gwendolyn M. Eadie, Joshua S. Speagle, Jessi Cisewski-Kehe +5

In the last two decades, Bayesian inference has become commonplace in astronomy. At the same time, the choice of algorithms, terminology, notation, and interpretation of Bayesian i…

astro-ph.IM2022★ 7 cited

Differentiating small-scale subhalo distributions in CDM and WDM models using persistent homology

Jessi Cisewski-Kehe, Brittany Terese Fasy, Wojciech Hellwing +3

The spatial distribution of galaxies at sufficiently small scales will encode information about the identity of the dark matter. We develop a novel description of the halo distribu…

astro-ph.IM2020★ 6 cited

Trend Filtering -- II. Denoising Astronomical Signals with Varying Degrees of Smoothness

Collin A. Politsch, Jessi Cisewski-Kehe, Rupert A. C. Croft +1

Trend filtering---first introduced into the astronomical literature in Paper I of this series---is a state-of-the-art statistical tool for denoising one-dimensional signals that po…

astro-ph.IM2019★ 2 cited

Realizing the potential of astrostatistics and astroinformatics

Gwendolyn Eadie, Thomas J. Loredo, Ashish A. Mahabal +12

This Astro2020 State of the Profession Consideration White Paper highlights the growth of astrostatistics and astroinformatics in astronomy, identifies key issues hampering the mat…

astro-ph.IM2019★ 21 cited

Trend Filtering -- I. A Modern Statistical Tool for Time-Domain Astronomy and Astronomical Spectroscopy

Collin A. Politsch, Jessi Cisewski-Kehe, Rupert A. C. Croft +1

The problem of denoising a one-dimensional signal possessing varying degrees of smoothness is ubiquitous in time-domain astronomy and astronomical spectroscopy. For example, in the…

astro-ph.IM2019★ 11 cited

A Preferential Attachment Model for the Stellar Initial Mass Function

Jessi Cisewski-Kehe, Grant Weller, Chad Schafer

Accurate specification of a likelihood function is becoming increasingly difficult in many inference problems in astronomy. As sample sizes resulting from astronomical surveys cont…

astro-ph.IM2019★ 33 cited

Modeling the Echelle Spectra Continuum with Alpha Shapes and Local Regression Fitting

Xin Xu, Jessi Cisewski-Kehe, Allen B. Davis +2

Continuum normalization of echelle spectra is an important data analysis step that is difficult to automate. Polynomial fitting requires a reasonably high order model to follow the…

astro-ph.IM2019★ 1 cited

Astro2020 Science White Paper: The Next Decade of Astroinformatics and Astrostatistics

A. Siemiginowska, G. Eadie, I. Czekala +49

Over the past century, major advances in astronomy and astrophysics have been largely driven by improvements in instrumentation and data collection. With the amassing of high quali…

astro-ph.IM2019★ 36 cited

The Role of Machine Learning in the Next Decade of Cosmology

Michelle Ntampaka, Camille Avestruz, Steven Boada +27

In recent years, machine learning (ML) methods have remarkably improved how cosmologists can interpret data. The next decade will bring new opportunities for data-driven cosmologic…