CaltechAUTHORS
  A Caltech Library Service

G10/COSMOS: 38 band (far-UV to far-IR) panchromatic photometry using LAMBDAR

Andrews, S. K. and Driver, S. P. and Davies, L. J. M. and Kafle, Prajwal R. and Robotham, Aaron S. G. and Wright, Angus H. (2017) G10/COSMOS: 38 band (far-UV to far-IR) panchromatic photometry using LAMBDAR. Monthly Notices of the Royal Astronomical Society, 464 (2). pp. 1569-1590. ISSN 0035-8711. http://resolver.caltech.edu/CaltechAUTHORS:20170628-135713279

Full text is not posted in this repository. Consult Related URLs below.

Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20170628-135713279

Abstract

We present a consistent total flux catalogue for a ∼1 deg2 subset of the Cosmic Evolution Survey (COSMOS) region (RA ∈ [149 ∘. .∘ 55, 150 ∘. .∘ 65], Dec. ∈ [1 ∘. .∘ 80, 2 ∘. .∘ 73]) with near-complete coverage in 38 bands from the far-ultraviolet to the far-infrared. We produce aperture matched photometry for 128 304 objects with i < 24.5 in a manner that is equivalent to the Wright et al. catalogue from the low-redshift (z < 0.4) Galaxy and Mass Assembly (GAMA) survey. This catalogue is based on publicly available imaging from GALEX, Canada–France–Hawaii Telescope, Subaru, Visible and Infrared Survey Telescope for Astronomy, Spitzer and Herschel, contains a robust total flux measurement or upper limit for every object in every waveband and complements our re-reduction of publicly available spectra in the same region. We perform a number of consistency checks, demonstrating that our catalogue is comparable to existing data sets, including the recent COSMOS2015 catalogue. We also release an updated Davies et al. spectroscopic catalogue that folds in new spectroscopic and photometric redshift data sets. The catalogues are available for download at http://cutout.icrar.org/G10/dataRelease.php. Our analysis is optimised for both panchromatic analysis over the full wavelength range and for direct comparison to GAMA, thus permitting measurements of galaxy evolution for 0 < z < 1 while minimizing the systematic error resulting from disparate data reduction methods.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/stw2395DOIArticle
Additional Information:© 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2016 September 21. Received 2016 September 16; in original form 2016 April 21.
Group:SPLASH, COSMOS
Record Number:CaltechAUTHORS:20170628-135713279
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170628-135713279
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:78660
Collection:CaltechAUTHORS
Deposited By: Joy Painter
Deposited On:28 Jun 2017 21:06
Last Modified:29 Jun 2017 21:48

Repository Staff Only: item control page