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Jessica Herrington

Researcher at University of Michigan

Publications -  8
Citations -  4397

Jessica Herrington is an academic researcher from University of Michigan. The author has contributed to research in topics: Bulge & Star formation. The author has an hindex of 6, co-authored 8 publications receiving 3939 citations. Previous affiliations of Jessica Herrington include Clemson University.

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Candels: The cosmic assembly near-infrared deep extragalactic legacy survey - The hubble space telescope observations, imaging data products, and mosaics

Anton M. Koekemoer, +124 more
TL;DR: In this paper, the authors describe the Hubble Space Telescope imaging data products and data reduction procedures for the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS).
Journal ArticleDOI

CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics

Anton M. Koekemoer, +122 more
TL;DR: The Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (CANDELS) as mentioned in this paper was designed to document the evolution of galaxies and black holes at $z\sim 1.5-8$, and to study Type Ia SNe beyond $z>1.5.
Journal ArticleDOI

The host galaxies of X-ray selected Active Galactic Nuclei to z= 2.5: Structure, star-formation and their relationships from CANDELS and Herschel/PACS ⋆

David J. Rosario, +65 more
TL;DR: In this paper, the authors studied the relationship between the structure and star formation rate (SFR) of X-ray selected low and moderate luminosity active galactic nuclei (AGNs) in the two Chandra Deep Fields, using Hubble Space Telescope imaging from the Cosmic Assembly Near Infrared Extragalactic Legacy Survey (CANDELS) and deep far-infrared maps from the PEP+GOODS-Herschel survey.

The host galaxies of X-ray selected active galactic nuclei to z =2 .5: Structure, star formation, and their relationships from CANDELS

TL;DR: In this article, the authors studied the relationship between the structure and star formation rate (SFR) of X-ray selected low and moderate luminosity active galactic nuclei (AGNs) in the two Chandra Deep Fields, using Hubble Space Telescope imaging from the Cosmic Assembly Near Infrared Extragalactic Legacy Survey (CANDELS) and deep far-infrared maps from the PEP+GOODS-Herschel survey.