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researcher

Matthew Ho

7 papers hereh-index 218 citations7 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author4
  • last author3

Across the 7 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
  • astro-ph.CO2
  • astro-ph.HE1
same name
  • Matthew Ho — 4 papers, h 3
  • Matthew Ho — 2 papers, h 2
  • Matthew Ho — 1 paper, h 1
  • Matthew Ho — 1 paper, h 2
  • Matthew Ho — 1 paper, h 8
  • Matthew Ho — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators
Showing astro-ph.GAShow all

4 papers · 1 filter

astro-ph.GA2026

Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations

Laura Sommovigo, Deaglan J. Bartlett, Rachel K. Cochrane +3

Dust attenuation is a major source of systematic uncertainty in both SED fitting and forward modeling of galaxy populations, yet the functional form used to parameterize attenuatio…

astro-ph.GA2025

Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer

Thomas Harvey, Christopher C. Lovell, Sophie Newman +13

We introduce Synference, a new, flexible Python framework for galaxy SED fitting using simulation-based inference (SBI). Synference leverages the Synthesizer package for flexible f…

astro-ph.GA2025

Learning the Universe: Cosmological and Astrophysical Parameter Inference with Galaxy Luminosity Functions and Colours

Christopher C. Lovell, Tjitske Starkenburg, Matthew Ho +9

We perform the first direct cosmological and astrophysical parameter inference from the combination of galaxy luminosity functions and colours using a simulation based inference ap…

astro-ph.GA2025

Learning the Universe: physically-motivated priors for dust attenuation curves

Laura Sommovigo, Rachel K. Cochrane, Rachel S. Somerville +9

Understanding the impact of dust on the spectral energy distributions (SEDs) of galaxies is crucial for inferring their physical properties and for studying the nature of interstel…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.