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Swara Ravindranath

Researcher at Space Telescope Science Institute

Publications -  165
Citations -  17434

Swara Ravindranath is an academic researcher from Space Telescope Science Institute. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 52, co-authored 118 publications receiving 15426 citations. Previous affiliations of Swara Ravindranath include Carnegie Learning & Inter-University Centre for Astronomy and Astrophysics.

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CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey

Norman A. Grogin, +108 more
TL;DR: The Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (CANDELS) as discussed by the authors was designed to document the first third of galactic evolution, from z approx. 8 - 1.5 to test their accuracy as standard candles for cosmology.
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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).
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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, +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.
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The Great Observatories Origins Deep Survey: Initial results from optical and near-infrared imaging

Mauro Giavalisco, +62 more
TL;DR: The GOODS survey as mentioned in this paper is based on multiband imaging data obtained with the Hubble Space Telescope and the Advanced Camera for Surveys (ACS) and covers roughly 320 arcmin2 in the ACS F435W, F606w, F814W, and F850LP bands, divided into two well-studied fields.