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DES science portal: Computing photometric redshifts

文献类型:期刊论文

作者Gschwend, J.1,2; Rossel, A. C.1,2; Ogando, R. L. C.1,2; Neto, A. F.2,3; Maia, M. A. G.1,2; da Costa, L. N.1,2; Lima, M.2,4; Pellegrini, P.1,2; Campisano, R.2,5; Singulani, C.1,2
刊名ASTRONOMY AND COMPUTING
出版日期2018-10-01
卷号25页码:58-80
关键词Astronomical databases: catalogs, surveys Methods: data analysis Galaxies: distances and redshifts, statistics
ISSN号2213-1337
DOI10.1016/j.ascom.2018.08.008
通讯作者Gschwend, J.(julia@linea.gov.br)
英文摘要A significant challenge facing photometric surveys for cosmological purposes is the need to produce reliable redshift estimates. The estimation of photometric redshifts (photo-zs) has been consolidated as the standard strategy to bypass the high production costs and incompleteness of spectroscopic redshift samples. Training-based photo-z methods require the preparation of a high-quality list of spectroscopic redshifts, which needs to be constantly updated. The photo-z training, validation, and estimation must be performed in a consistent and reproducible way in order to accomplish the scientific requirements. To meet this purpose, we developed an integrated web-based data interface that not only provides the framework to carry out the above steps in a systematic way, enabling the ease testing and comparison of different algorithms, but also addresses the processing requirements by parallelizing the calculation in a transparent way for the user. This framework called the Science Portal (hereafter Portal) was developed in the context the Dark Energy Survey (DES) to facilitate scientific analysis. In this paper, we show how the Portal can provide a reliable environment to access vast datasets, provide validation algorithms and metrics, even in the case of multiple photo-zs methods. It is possible to maintain the provenance between the steps of a chain of workflows while ensuring reproducibility of the results. We illustrate how the Portal can be used to provide photo-z estimates using the DES first year (Y1A1) data. While the DES collaboration is still developing techniques to obtain more precise photo-zs, having a structured framework like the one presented here is critical for the systematic vetting of DES algorithmic improvements and the consistent production of photo-zs in future DES releases. (C) 2018 Elsevier B.V. All rights reserved.
WOS关键词VLT DEEP SURVEY ; SPECTROSCOPIC SURVEY ; CALIBRATION ; GALAXIES ; SPECTRA ; SAMPLES
WOS研究方向Astronomy & Astrophysics ; Computer Science
语种英语
WOS记录号WOS:000451390700007
出版者ELSEVIER SCIENCE BV
源URL[http://libir.pmo.ac.cn/handle/332002/20816]  
专题中国科学院紫金山天文台
通讯作者Gschwend, J.
作者单位1.Observ Nacl, Rua Gen Jose Cristino 77, BR-20921400 Rio de Janeiro, RJ, Brazil
2.Lab Interinst E Astron LIneA, Rua Gen Jose Cristino 77, BR-20921400 Rio de Janeiro, RJ, Brazil
3.LSST Project Management Off, Tucson, AZ USA
4.Univ Sao Paulo, Inst Fis, Dept Fis Matemat, CP 66318, BR-05314970 Sao Paulo, Brazil
5.Ctr Fed Educ Tecnol Celso Suckow Fonseca CEFET RJ, Av Maracana 229, BR-20271110 Rio De Janeiro, RJ, Brazil
6.Univ Cote dAzur, Observ Cote dAzur, Lab Lagrange, CNRS, Blvd Observ,CS 34229, F-06304 Nice 4, France
7.Univ Illinois, Dept Astron, 1002 W Green St, Urbana, IL 61801 USA
8.Natl Ctr Supercomp Applicat, 1205 West Clark St, Urbana, IL 61801 USA
9.Univ Queensland, Dept Math & Phys, Brisbane, Qld 4072, Australia
10.ARC Ctr Excellence All Sky Astrophys CAASTRO, Melbourne, Vic, Australia
推荐引用方式
GB/T 7714
Gschwend, J.,Rossel, A. C.,Ogando, R. L. C.,et al. DES science portal: Computing photometric redshifts[J]. ASTRONOMY AND COMPUTING,2018,25:58-80.
APA Gschwend, J..,Rossel, A. C..,Ogando, R. L. C..,Neto, A. F..,Maia, M. A. G..,...&Walker, A. R..(2018).DES science portal: Computing photometric redshifts.ASTRONOMY AND COMPUTING,25,58-80.
MLA Gschwend, J.,et al."DES science portal: Computing photometric redshifts".ASTRONOMY AND COMPUTING 25(2018):58-80.

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来源:紫金山天文台

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