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Cosmic Origins at the Roman Workshop

The Nancy Grace Roman Space Telescope is a NASA observatory designed to settle essential questions in the areas of dark energy, exoplanets, and infrared astrophysics.

Location

Pasadena, California

Dates

13-16 July 2026

Community

Cosmic Origins

Type

Workshop

Shifting Landscapes in Astrophysics

New Frontiers to Explore with Roman

This Caltech/IPAC workshop will take place July 13 through 16, 2026, and is being organized and hosted by the Roman Science Support Center. The goal of this conference is to bring members of the community together to focus on the new exciting landscapes poised for potential breakthroughs using the Roman surveys with the Wide Field Instrument, as well as on the Coronagraph Instrument.

We will cover topics across all types of Roman science, from exoplanets to high-redshift galaxy evolution to cosmology, and beyond. The conference will focus on new results and questions that have emerged since Roman was first envisioned, that Roman is uniquely suited to address, given its high spatial resolution, sensitivity, and wide field spectroscopy and imaging capabilities. We look forward to fascinating and stimulating presentations and discussions from the broader astronomical community, as we approach the era of Roman.

Participation in this conference is limited to professional astronomers, research scientists, and other professionals actively engaged in the relevant field. 

Roman event poster 2026
Workshop Poster

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.