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19972022
most citedCANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey

2.2k citations · 10.2k across the 79 of their papers we have counts for

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12 papers · 1 filter

astro-ph.CO2013★ 132 cited

The Progenitors of the Compact Early-Type Galaxies at High-Redshift

Christina C. Williams, Mauro Giavalisco, Paolo Cassata +19

We use GOODS and CANDELS images to identify progenitors of massive (log M > 10 Msun) compact "early-type" galaxies (ETGs) at z~1.6. Since merging and accretion increase the size of…

astro-ph.CO2013★ 362 cited

A Critical Assessment of Photometric Redshift Methods: A CANDELS Investigation

Tomas Dahlen, Bahram Mobasher, Sandra M. Faber +35

We present results from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) photometric redshift methods investigation. In this investigation, the results…

astro-ph.CO2013★ 38 cited

ALMA follows streaming of dense gas down to 40 pc from the supermassive black hole in NGC1097

Kambiz Fathi, Andreas A. Lundgren, Kotaro Kohno +14

We present a kinematic analysis of the dense molecular gas in the central 200 parsecs of the nearby galaxy NGC1097, based on Cycle 0 observations with the Atacama Large Millimeter/…

astro-ph.CO2013★ 86 cited

The Discovery of the Most Distant Known Type Ia Supernova at Redshift 1.914

David O. Jones, Steven A. Rodney, Adam G. Riess +22

We present the discovery of a Type Ia supernova (SN) at redshift from the CANDELS multi-cycle treasury program on the \textit{Hubble Space Telescope (HST)}. This SN was…

astro-ph.CO2012★ 103 cited

[CII] line emission in massive star-forming galaxies at z=4.7

J. Wagg, T. Wiklind, C. L. Carilli +20

We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of the [CII] 157.7micron fine structure line and thermal dust continuum emission from a pair of gas-rich…

astro-ph.CO2011★ 149 cited

How Do Star-Forming Galaxies at Z>3 Assemble Their Masses?

Kyoung-Soo Lee, Henry C. Ferguson, Tommy Wiklind +8

We investigate how star-forming galaxies typically assemble their masses at high redshift. Using the deep multi-wavelength coverage of the GOODS dataset, we measure stellar mass of…