Pith. sign in

REVIEW 2 cited by

The JWST Early Release Observations

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 2207.13067 v2 pith:WOYWSODW submitted 2022-07-26 astro-ph.IM

The JWST Early Release Observations

Klaus Pontoppidan , Jaclyn Barrientes , Claire Blome , Hannah Braun , Matthew Brown , Margaret Carruthers , Dan Coe , Joseph DePasquale
show 28 more authors
Nestor Espinoza Macarena Garcia Marin Karl D. Gordon Alaina Henry Leah Hustak Andi James Anton M. Koekemoer Stephanie LaMassa David Law Alexandra Lockwood Amaya Moro-Martin Susan E. Mullally Alyssa Pagan Dani Player Charles Proffitt Christine Pulliam Leah Ramsay Swara Ravindranath Neill Reid Massimo Robberto Elena Sabbi Leonardo Ubeda Michael Balogh Kathryn Flanagan Jonathan Gardner Hashima Hasan Bonnie Meinke Antonella Nota
This is my paper
classification astro-ph.IM
keywords jwstobservationsproductsearlygalaxyimagesoutreachpublic
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

The James Webb Space Telescope (JWST) Early Release Observations (EROs) is a set of public outreach products created to mark the end of commissioning and the beginning of science operations for JWST. Colloquially known as the "Webb First Images and Spectra", these products were intended to demonstrate to the worldwide public that JWST is ready for science, and is capable of producing spectacular results. The package was released on July 12, 2022, and included images and spectra of the galaxy cluster SMACS~J0723.3-7327 and distant lensed galaxies, the interacting galaxy group Stephan's Quintet, NGC 3324 in the Carina star-forming complex, the Southern Ring planetary nebula NGC 3132, and the transiting hot Jupiter WASP 96b. This paper describes the ERO technical design, observations, and scientific processing of data underlying the colorful outreach products.

discussion (0)

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

Forward citations

Cited by 2 Pith papers

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

  1. A JWST, ALMA and VLA survey of the Ophiuchus-A star-forming region: Unveiling hidden dust mass and connecting infrared outflows to their radio origins

    astro-ph.GA 2026-07 conditional novelty 4.0

    A multi-wavelength survey of 20 Ophiuchus protostars finds dust masses tens to hundreds of times larger than millimetre-only estimates, if the adopted dust-opacity model is correct.

  2. The energy conditions and model selection in the local Universe

    astro-ph.CO 2026-05 unverdicted novelty 4.0

    Local HII galaxy and cosmic chronometer data favor the Rh=ct universe over ΛCDM at 92% vs 8% likelihood, with Rh=ct satisfying all energy conditions while ΛCDM violates the strong energy condition at z≲2.