activity
20202024
most citedA new approach to observational cosmology using the scattering transform

142 citations · 551 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.EP2024★ 3 cited

A candidate giant planet companion to the massive, young white dwarf GALEX J071816.4+373139 informs the occurrence of giant planets orbiting B stars

Sihao Cheng, Kevin C. Schlaufman, Ilaria Caiazzo

It has been suggested that giant planet occurrence peaks for stars with at a value a factor of 4 higher than observed for solar-mass stars. This popu…

astro-ph.CO2023★ 32 cited

Cosmology from weak lensing peaks and minima with Subaru Hyper Suprime-Cam survey first-year data

Gabriela A. Marques, Jia Liu, Masato Shirasaki +7

We present cosmological constraints derived from peak counts, minimum counts, and the angular power spectrum of the Subaru Hyper Suprime-Cam first-year (HSC Y1) weak lensing shear…

astro-ph.SR2023★ 7 cited

Dynamical masses across the Hertzsprung-Russell diagram

Hsiang-Chih Hwang, Yuan-Sen Ting, Sihao Cheng +1

We infer the dynamical masses of stars across the Hertzsprung-Russell (H-R) diagram using wide binaries from the Gaia survey. Gaia's high-precision astrometry measures the wide bin…

physics.data-an2023★ 15 cited

Scattering Spectra Models for Physics

Sihao Cheng, Rudy Morel, Erwan Allys +2

Physicists routinely need probabilistic models for a number of tasks such as parameter inference or the generation of new realizations of a field. Establishing such models for high…

astro-ph.IM2021★ 24 cited

How to quantify fields or textures? A guide to the scattering transform

Sihao Cheng, Brice Ménard

Extracting information from stochastic fields or textures is a ubiquitous task in science, from exploratory data analysis to classification and parameter estimation. From physics t…

astro-ph.CO2021★ 61 cited

Weak lensing scattering transform: dark energy and neutrino mass sensitivity

Sihao Cheng, Brice Ménard

As weak lensing surveys become deeper, they reveal more non-Gaussian aspects of the convergence field which can only be extracted using statistics beyond the power spectrum. In Che…

astro-ph.EP2020★ 31 cited

An Increase in Small-planet Occurrence with Metallicity for Late-type Dwarf Stars in the Kepler Field and Its Implications for Planet Formation

Cicero X. Lu, Kevin C. Schlaufman, Sihao Cheng

While it is well established that giant-planet occurrence rises rapidly with host star metallicity, it is not yet clear if small-planet occurrence around late-type dwarf stars depe…

astro-ph.SR2020★ 65 cited

Multi-Gigayear White Dwarf Cooling Delays from Clustering-Enhanced Gravitational Sedimentation

Evan B. Bauer, Josiah Schwab, Lars Bildsten +1

Cooling white dwarfs (WDs) can yield accurate ages when theoretical cooling models fully account for the physics of the dense plasma of WD interiors. We use MESA to investigate coo…

astro-ph.SR2020★ 34 cited

A Gravitational Redshift Measurement of the White Dwarf Mass-Radius Relation

Vedant Chandra, Hsiang-Chih Hwang, Nadia L. Zakamska +1

The mass-radius relation of white dwarfs is largely determined by the equation of state of degenerate electrons, which causes the stellar radius to decrease as mass increases. Here…

astro-ph.SR2020★ 45 cited

Forever young white dwarfs: when stellar ageing stops

María E. Camisassa, Leandro G. Althaus, Santiago Torres +5

White dwarf stars are the most common end point of stellar evolution. Of special interest are the ultramassive white dwarfs, as they are related to type Ia Supernovae explosions, m…

astro-ph.SR2020★ 91 cited

Carbon star formation as seen through the non-monotonic initial-final mass relation

Paola Marigo, Jeffrey D. Cummings, Jason Lee Curtis +13

The initial-final mass relation (IFMR) links the birth mass of a star to the mass of the compact remnant left at its death. While the relevance of the IFMR across astrophysics is u…

astro-ph.CO2020★ 142 cited

A new approach to observational cosmology using the scattering transform

Sihao Cheng, Yuan-Sen Ting, Brice Ménard +1

Parameter estimation with non-Gaussian stochastic fields is a common challenge in astrophysics and cosmology. In this paper, we advocate performing this task using the scattering t…

astro-ph.SR2020★ 1 cited

Two delays in white dwarf evolution revealed by Gaia

Sihao Cheng

By comparing two age indicators of high-mass white dwarfs derived from Gaia data, two discoveries have been made recently: one is the existence of a cooling anomaly that produces t…