Pith. sign in

REVIEW 1 cited by

Dust emission from the first massive galaxies

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2001.04303 v1 pith:GYAZSH7H submitted 2020-01-13 astro-ph.GA astro-ph.CO

Maria Emilia De Rossi , George H. Rieke , Irene Shivaei , Volker Bromm , Jianwei Lyu This is my paper · ORCID
classification astro-ph.GAastro-ph.CO
keywords galaxiesdustmassiveobservedsedsemissionenergyfirst
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

We compare observed far-infrared (FIR) galaxy spectral energy distributions (SEDs) at $z\sim6$ and theoretical predictions for first massive population II (Pop II) galaxies. Observed FIR SEDs at $z\gtrsim5$ are broad and shifted to bluer wavelengths when compared to galaxies at $z\sim3$. By implementing an analytical model for dust emission from Pop II massive galaxies,we were able to reproduce the observed behaviour as a consequence of the high energy densities and silicate-rich dust composition of high-$z$ model galaxies. As noted in a previous work, the non-blackbody nature of galaxy SEDs at $z \sim 6$ should be taken into account when interpreting measurements of FIR luminosities to avoid underestimating star formation rates.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Determining Total Infrared Luminosities from Submm Measurements of High Redshift Galaxies

    astro-ph.GA 2026-07 conditional novelty 5.0 of 10

    IR SED broadening in high-z galaxies is driven primarily by luminosity density, requiring ~1.6–1.7 (up to ~2) corrections to modified-blackbody total infrared luminosities.

Pith tools