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dc.contributor.author
Zuntz, Joe
dc.contributor.author
Lanusse, Francois
dc.contributor.author
Malz, Alex I.
dc.contributor.author
Wright, Angus H.
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Slosar, Anze
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Abolfathi, Bela
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Alonso, David
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Bault, Abby
dc.contributor.author
Bom, Clecio R.
dc.contributor.author
Brescia, Massimo
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Broussard, Adam
dc.contributor.author
Campagne, Jean Eric
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Cavuoti, Stefano
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Cypriano, Eduardo S.
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Fraga, Bernardo M. O.
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Gawiser, Eric
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Gonzalez, Elizabeth Johana
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Green, Dylan
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Hatfield, Peter
dc.contributor.author
Iyer, Kartheik
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Kirkby, David
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Nicola, Andrina
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Nourbakhsh, Erfan
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Park, Andy
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Teixeira, Gabriel
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Heitmann, Katrin
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Kovacs, Eve
dc.contributor.author
Mao, Yao Yuan
dc.date.available
2022-09-29T12:59:01Z
dc.date.issued
2021-10
dc.identifier.citation
Zuntz, Joe; Lanusse, Francois; Malz, Alex I.; Wright, Angus H.; Slosar, Anze; et al.; The LSST-DESC 3x2pt Tomography Optimization Challenge; Maynooth Academic Publishing; The Open Journal of Astrophysics; 4; 13; 10-2021; 1-26
dc.identifier.uri
http://hdl.handle.net/11336/170946
dc.description.abstract
This paper presents the results of the Rubin Observatory Dark Energy Science Collaboration (DESC) 3x2pt tomography challenge, which served as a first step toward optimizing the tomographic binning strategy for the main DESC analysis. The task of choosing an optimal tomographic binning scheme for a photometric survey is made particularly delicate in the context of a metacalibrated lensing catalogue, as only the photometry from the bands included in the metacalibration process (usually riz and potentially g) can be used in sample definition. The goal of the challenge was to collect and compare bin assignment strategies under various metrics of a standard 3x2pt cosmology analysis in a highly idealized setting to establish a baseline for realistically complex follow-up studies; in this preliminary study, we used two sets of cosmological simulations of galaxy redshifts and photometry under a simple noise model neglecting photometric outliers and variation in observing conditions, and contributed algorithms were provided with a representative and complete training set. We review and evaluate the entries to the challenge, finding that even from this limited photometry information, multiple algorithms can separate tomographic bins reasonably well, reaching figures-of-merit scores close to the attainable maximum. We further find that adding the g band to riz photometry improves metric performance by ~15% and that the optimal bin assignment strategy depends strongly on the science case: which figure-of-merit is to be optimized, and which observables (clustering, lensing, or both) are included.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
Maynooth Academic Publishing
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
TOMOGRAPHY
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CHALLENGE
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LENSING
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Astronomía
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
dc.title
The LSST-DESC 3x2pt Tomography Optimization Challenge
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2022-09-21T13:52:15Z
dc.identifier.eissn
2565-6120
dc.journal.volume
4
dc.journal.number
13
dc.journal.pagination
1-26
dc.journal.pais
Irlanda
dc.description.fil
Fil: Zuntz, Joe. University of Hawaii at Manoa; Estados Unidos
dc.description.fil
Fil: Lanusse, Francois. Université Paris Sud; Francia
dc.description.fil
Fil: Malz, Alex I.. Ruhr Universität Bochum; Alemania
dc.description.fil
Fil: Wright, Angus H.. Ruhr Universität Bochum; Alemania
dc.description.fil
Fil: Slosar, Anze. Brookhaven National Laboratory; Estados Unidos
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Fil: Abolfathi, Bela. University Of California At Los Angeles. Department Of Physics And Astronomy.; Estados Unidos
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Fil: Alonso, David. University of Oxford; Reino Unido
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Fil: Bault, Abby. University Of California At Los Angeles. Department Of Physics And Astronomy.; Estados Unidos
dc.description.fil
Fil: Bom, Clecio R.. Centro Brasileiro de Pesquisas Físicas; Brasil
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Fil: Brescia, Massimo. Istituto Nazionale di Astrofisica; Italia
dc.description.fil
Fil: Broussard, Adam. Texas A&M University; Estados Unidos
dc.description.fil
Fil: Campagne, Jean Eric. Université Paris Sud; Francia
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Fil: Cavuoti, Stefano. Istituto Nazionale di Astrofisica; Italia
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Fil: Cypriano, Eduardo S.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; Brasil
dc.description.fil
Fil: Fraga, Bernardo M. O.. Centro Brasileiro de Pesquisas Físicas; Brasil
dc.description.fil
Fil: Gawiser, Eric. Rutgers University; Estados Unidos
dc.description.fil
Fil: Gonzalez, Elizabeth Johana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
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Fil: Green, Dylan. University Of California At Los Angeles. Department Of Physics And Astronomy.; Estados Unidos
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Fil: Hatfield, Peter. University of Oxford; Reino Unido
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Fil: Iyer, Kartheik. Dunlap Institute for Astronomy & Astrophysics; Canadá
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Fil: Kirkby, David. University Of California At Los Angeles. Department Of Physics And Astronomy.; Estados Unidos
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Fil: Nicola, Andrina. University of Princeton; Estados Unidos
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Fil: Nourbakhsh, Erfan. University Of California At Los Angeles. Department Of Physics And Astronomy.; Estados Unidos
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Fil: Park, Andy. University Of California At Los Angeles. Department Of Physics And Astronomy.; Estados Unidos
dc.description.fil
Fil: Teixeira, Gabriel. Centro Brasileiro de Pesquisas Físicas; Brasil
dc.description.fil
Fil: Heitmann, Katrin. Argonne National Laboratory; Estados Unidos
dc.description.fil
Fil: Kovacs, Eve. Argonne National Laboratory; Estados Unidos
dc.description.fil
Fil: Mao, Yao Yuan. University of Utah; Estados Unidos
dc.journal.title
The Open Journal of Astrophysics
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.21105/astro.2108.13418
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/2108.13418v2
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://astro.theoj.org/article/29530-the-lsst-desc-3x2pt-tomography-optimization-challenge
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