Pith. sign in

REVIEW 1 cited by

Photometric evolution and peculiar dust formation in the gamma-ray Nova Sco 2012 (V1324 Sco)

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 1506.06031 v1 pith:VTMXYBIC submitted 2015-04-20 astro-ph.SR

U. Munari , F. M. Walter , A. Henden , S. Dallaporta , T. Finzell , L. Chomiuk This is my paper · ORCID
classification astro-ph.SR
keywords novadustearlyformationgamma-raymagnitudemaximumoptical
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Optical (BVRI) and infrared (JHK) photometry of the gamma-ray nova Nova Sco 2012 (V1324 Sco) is presented and the lightcurve reconstructed and discussed. An interstellar reddening E(B-V)=1.23 is derived. Dust begun to form at an early date in the nova, only one magnitude down and 20 days past maximum optical brightness and caused an extinction of at least 6 magnitudes in V band, that cleared some months later. This unusual early dust formation compromises the application of the magnitude at maximum versus rate of decline (MMRD) relations in estimating the distance to the nova.

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. An Optically Motivated Gamma-ray Study of Fermi-LAT Novae

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    For 26 Fermi-LAT novae, the optical three-magnitude decay time is the most common time window that maximizes gamma-ray detection significance.

Pith tools