Show simple item record

Files in this item


Item metadata

dc.contributor.authorAndrews, S. K.
dc.contributor.authorDriver, S. P.
dc.contributor.authorDavies, L. J. M.
dc.contributor.authorKafle, Prajwal R.
dc.contributor.authorRobotham, Aaron S. G.
dc.contributor.authorWright, Angus H.
dc.identifier.citationAndrews , S K , Driver , S P , Davies , L J M , Kafle , P R , Robotham , A S G & Wright , A H 2017 , ' G10/COSMOS : 38 band (far-UV to far-IR) panchromatic photometry using LAMBDAR ' , Monthly Notices of the Royal Astronomical Society , vol. 464 , no. 2 , pp. 1569-1590 .
dc.identifier.otherPURE: 252098434
dc.identifier.otherPURE UUID: 4167e512-b7bb-406d-b200-1dd33efb775c
dc.identifier.otherScopus: 85014647868
dc.identifier.otherWOS: 000393647100024
dc.description.abstractWe 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 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.
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2017, the Author(s). This work has been made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at
dc.subjectGalaxies: generalen
dc.subjectGalaxies: photometryen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.titleG10/COSMOS : 38 band (far-UV to far-IR) panchromatic photometry using LAMBDARen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.description.statusPeer revieweden

This item appears in the following Collection(s)

Show simple item record