Pith. sign in

REVIEW 1 cited by

Nancy Grace Roman Space Telescope Coronagraph Instrument Overview and Status

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 2309.08672 v1 pith:B275TUW7 submitted 2023-09-15 astro-ph.IM astro-ph.EP

Nancy Grace Roman Space Telescope Coronagraph Instrument Overview and Status

Vanessa P. Bailey , Eduardo Bendek , Brian Monacelli , Caleb Baker , Gasia Bedrosian , Eric Cady , Ewan S. Douglas , Tyler Groff
show 14 more authors
Sergi R. Hildebrandt N. Jeremy Kasdin John Krist Bruce Macintosh Bertrand Mennesson Patrick Morrissey Ilya Poberezhskiy Hari B. Subedi Jason Rhodes Aki Roberge Marie Ygouf Robert T. Zellem Feng Zhao Neil T. Zimmerman
This is my paper
classification astro-ph.IM astro-ph.EP
keywords instrumentintegrationspacecoronagraphgracenancyobservingroman
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
Share X Bluesky LinkedIn Reddit HN
read the original abstract

The Nancy Grace Roman Space Telescope Coronagraph Instrument is a critical technology demonstrator for NASA's Habitable Worlds Observatory. With a predicted visible-light flux ratio detection limit of 1E-8 or better, it will be capable of reaching new areas of parameter space for both gas giant exoplanets and circumstellar disks. It is in the final stages of integration and test at the Jet Propulsion Laboratory, with an anticipated delivery to payload integration in the coming year. This paper will review the instrument systems, observing modes, potential observing applications, and overall progress toward instrument integration and test.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

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

  1. Estimating Orbital Parameters of Direct Imaging Exoplanet Using Neural Network

    astro-ph.EP 2025-10 conditional novelty 4.0

    Warm-starting parallel-tempered MCMC with flow-matching posterior proposals infers β Pictoris b's orbit about 78-365× faster than conventional samplers with comparable posteriors, though the comparison is not fully ap...