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D. Sponseller

4 papers here

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

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO4
same name
  • D. Sponseller — 3 papers
  • D. Sponseller — 1 paper

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

4 papers

astro-ph.CO2026

Cosmoglobe DR2. VI. Disentangling hot and cold thermal dust emission with Planck HFI

R. M. Sullivan, E. Gjerløw, M. Galloway +20

We present a four-component high-resolution model of thermal dust emission for microwave and sub-mm frequencies derived from Planck HFI, WHAM and Gaia. The resulting high-resolutio…

astro-ph.CO2026

Cosmoglobe DR2. IV. Modelling starlight in DIRBE with Gaia and WISE

M. Galloway, E. Gjerløw, M. San +20

We present a model of starlight emission in the Diffuse Infrared Background Explorer (DIRBE) data between 1.25 and 25μm based on \textit{Gaia} and WISE measurements. We include…

astro-ph.CO2026

Cosmoglobe DR2. VII. Towards a concordance model of large-scale thermal dust emission for microwave and infrared frequencies

E. Gjerløw, R. M. Sullivan, R. Aurvik +20

We fit a four-component thermal dust model to COBE-DIRBE data between 3.5 and 240 micron within the global Bayesian end-to-end Cosmoglobe DR2 reanalysis. Following a companion anal…

astro-ph.CO2026

Cosmoglobe DR2. V. Spatial correlations between thermal dust and ionized carbon emission in Planck HFI and COBE-DIRBE

E. Gjerløw, R. M. Sullivan, R. Aurvik +20

We fit five tracers of thermal dust emission to ten Planck HFI and COBE-DIRBE frequency maps between 353 GHz and 25 THz, aiming to map the relative importance of each physical host…

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