Pith. sign in

REVIEW 1 cited by

Identification of planetary and proto-planetary nebulae candidates through akari infrared photometry

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 2407.16060 v1 pith:QSCWHUSJ submitted 2024-07-22 astro-ph.SR astro-ph.GA

R. A. Marquez-Lugo , S.N. Kemp , G. Ramos-Larios , A. Nigoche-Netro , S.G. Navarro , L.J. Corral This is my paper · ORCID
classification astro-ph.SRastro-ph.GA
keywords candidatesnebulaeppneakariobjectsplanetarypotentialproto-planetary
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

We utilized photometric data from the space telescope AKARI to identify potential planetary nebulae (PNe) and proto-planetary nebulae (PPNe) candidates. Using the colour-colour diagram, we found a region with a high concentration of established PNe and PPNe, comprising about 95% of the objects. Based on this, we identified 67 objects within this region that lack definitive classification in existing literature, suggesting they are promising candidates. We conducted Spectral Energy Distribution (SED) analysis and morphological investigations using imagery from various observatories and satellites. Finally, we present a list of 65 potential PNe and PPNe candidates.

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. DECaPS and SMA discovery of a highly-inclined class I YSO with an outflow: IRAS 08235-4316

    astro-ph.SR 2024-11 conditional novelty 6.0 of 10

    IRAS 08235-4316 is a newly identified, highly inclined class I young stellar object with an embedded disk, an outflow, and a millimeter radius of about 440 au.

Pith tools