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Carol J. Lonsdale

Researcher at National Radio Astronomy Observatory

Publications -  185
Citations -  20937

Carol J. Lonsdale is an academic researcher from National Radio Astronomy Observatory. The author has contributed to research in topics: Galaxy & Luminous infrared galaxy. The author has an hindex of 63, co-authored 182 publications receiving 18841 citations. Previous affiliations of Carol J. Lonsdale include California Institute of Technology & Jet Propulsion Laboratory.

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Book ChapterDOI

The ISO-IRAS Faint Galaxy Survey: ISOCAM Imaging and Optical Spectroscopy

TL;DR: The ISO-IRAS Faint Galaxy Survey (ISO-FSS) as discussed by the authors was designed to obtain a sample of the most distant, highest luminosity infrared galaxies from the 0.75 million sources in the IRAS Faintsource survey.
Posted Content

Angular Clustering of Galaxies at 3.6 μm from the SWIRE survey

TL;DR: In this paper, the angular correlation function of galaxies selected to have 3.6 μm fluxes brighter than 32 μJy in three fields totaling two square degrees in area is computed.
Journal ArticleDOI

Dust-Obscured Radio AGNS from the Wise Survey

TL;DR: In this paper, the authors select a unique sample containing ~ 200 of the most luminous obscured quasars by cross-matching the WISE catalog with the FIRST and NVSS radio surveys and present overall statistics for the observed range of colors and radio/mid-IR flux density ratio.
Journal ArticleDOI

The SWIRE/Chandra Survey: The X-ray Sources

TL;DR: In this paper, a moderate-depth (70 ksec), contiguous 0.7 sq.deg, Chandra survey was conducted in the Lockman Hole Field of the Spitzer/SWIRE Legacy Survey coincident with a completed, ultra-deep VLA survey with deep optical and near-infrared imaging in-hand.
Posted Content

The ISO/NASA Key Project on AGN Spectral Energy Distributions (Characteristics of the ISO Data)

TL;DR: The US ISO Key Project on quasar spectral energy distributions seeks to better understand the very broad-band emission features of quasars from radio to X-rays as mentioned in this paper, using the ISOPHOT instrument at 8 bands from 5 to 200 microns.