English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/213458
Share/Impact:
Statistics
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE
Exportar a otros formatos:

Title

Multifrequency filter search for high redshift sources and lensing systems in Herschel -ATLAS

AuthorsManjón-García, Alberto; Herranz, D. ; Diego, José María ; Bonavera, Laura ; González-Nuevo, J.
KeywordsMethods: data analysis
Techniques: image processing
Surveys
Submillimeter: galaxies
Galaxies: high-redshift
Gravitational lensing: strong
Issue Date2019
PublisherEDP Sciences
CitationAstronomy and Astrophysics 622: A 106 (2019)
AbstractWe present a new catalog of high-redshift candidate Herschel sources. Our sample is obtained after applying a multifrequency filtering method (>matched multifilter>), which is designed to improve the signal-to-noise ratio of faint extragalactic point sources. The method is tested against already-detected sources from the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) and used to search for new high-redshift candidates. The multifilter technique also produces an estimation of the photometric redshift of the sources. When compared with a sample of sources with known spectroscopic redshift, the photometric redshift returned from the multifilter is unbiased in the redshift range 0.8 < z < 4.3. Using simulated data we reproduced the same unbiased result in roughly the same redshift range and determined the error (and bias above z 4) in the photometric redshifts. Based on the multifilter technique, and a selection based on color, flux, and agreement of fit between the observed photometry and assumed SED, we find 370 robust candidates to be relatively bright high-redshift sources. A second sample with 237 objects focuses on the faint end at high-redshift. These 237 sources were previously near the H-ATLAS detection limit but are now confirmed with our technique as high significance detections. Finally, we look for possible lensed Herschel sources by cross-correlating the first sample of 370 objects with two different catalogs of known low-redshift objects, the redMaPPer Galaxy Cluster Catalog and a catalog of galaxies with spectroscopic redshift from the Sloan Digital Sky Survey Data Release 14. Our search renders a number of candidates to be lensed systems from the SDSS cross-correlation but none from the redMaPPeR confirming the more likely galactic nature of the lenses.
Publisher version (URL)https://doi.org/10.1051/0004-6361/201834549
URIhttp://hdl.handle.net/10261/213458
DOI10.1051/0004-6361/201834549
Identifiersdoi: 10.1051/0004-6361/201834549
e-issn: 1432-0746
issn: 0004-6361
Appears in Collections:(IFCA) Artículos
Files in This Item:
File Description SizeFormat 
multifrequ.pdf1,89 MBAdobe PDFThumbnail
View/Open
Show full item record
Review this work
 


WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.