Search NASA⌕ Search

DOE OSTI · 2432453

Enhancing weak lensing redshift distribution characterization by optimizing the Dark Energy Survey Self-Organizing Map Photo-z method

Campos, A. [Carnegie Mellon U.] (ORCID:0000000251240771)·Yin, B. [Duke U.] (ORCID:0009000656049980)·Dodelson, S. [Carnegie Mellon U.] (ORCID:0000000284463859)·Amon, A. [Cambridge U., Inst. of Astron.]·Alarcon, A. [Argonne; Barcelona, IEEC]·Sánchez, C. [UPenn, Philadelphia]·Bernstein, G. M. [UPenn, Philadelphia]·Giannini, G. [Chicago U., KICP; Barcelona, IFAE] (ORCID:0000000237301750)·Myles, J. [Princeton U., Astrophys. Sci. Dept.]·Samuroff, S. [Northeastern U.]·Alves, O. [U. Michigan, Ann Arbor]·Andrade-Oliveira, F. [U. Michigan, Ann Arbor]·Bechtol, K. [Wisconsin U., Madison]·Becker, M. R. [Argonne]·Blazek, J. [Northeastern U.]·Camacho, H. [LIneA, Rio de Janeiro; Sao Paulo, IFT; Brookhaven]·Carnero Rosell, A. [LIneA, Rio de Janeiro; IAC, La Laguna; Laguna U., Tenerife]·Carrasco Kind, M. [Illinois U., Urbana, Astron. Dept.; Illinois U., Urbana (main)]·Cawthon, R. [William-Mary Coll.]·Chang, C. [Chicago U., Astron. Astrophys. Ctr.; Chicago U., KICP] (ORCID:0000000278870896)·Chen, R. [Duke U.]·Choi, A. [NASA, Goddard]·Cordero, J. [Jodrell Bank]·Davis, C. [KIPAC, Menlo Park]·DeRose, J. [LBL, Berkeley]·Diehl, H. T. [Fermilab] (ORCID:0000000283577467)·Doux, C. [UPenn, Philadelphia; LPSC, Grenoble]·Drlica-Wagner, A. [Chicago U., KICP; Chicago U., Astron. Astrophys. Ctr.; Fermilab] (ORCID:000000018251933X)·Eckert, K. [UPenn, Philadelphia]·Eifler, T. F. [Caltech, JPL; Arizona U., Astron. Dept. - Steward Observ.]·Elvin-Poole, J. [Waterloo U.]·Everett, S. [Caltech, JPL]·Fang, X. [Arizona U., Astron. Dept. - Steward Observ.; UC, Berkeley, Astron. Dept.] (ORCID:0000000250549566)·Ferté, A. [SLAC]·Friedrich, O. [Cambridge U., Inst. of Astron.]·Gatti, M. [UPenn, Philadelphia]·Gruen, D. [Munich U.]·Gruendl, R. A. [Illinois U., Urbana, Astron. Dept.; Illinois U., Urbana (main)]·Harrison, I. [Cardiff U.]·Hartley, W. G. [U. Geneva (main)]·Herner, K. [Fermilab]·Huang, H. [Arizona U., Astron. Dept. - Steward Observ.; Arizona U.]·Huff, E. M. [Caltech, JPL]·Jarvis, M. [UPenn, Philadelphia]·Krause, E. [Arizona U., Astron. Dept. - Steward Observ.]·Kuropatkin, N. [Fermilab]·Leget, P.-F. [KIPAC, Menlo Park]·MacCrann, N. [Cambridge U., DAMTP]·McCullough, J. [KIPAC, Menlo Park] (ORCID:0000000244753456)·Navarro-Alsina, A. [Campinas State U.]·Pandey, S. [UPenn, Philadelphia]·Prat, J. [Nordita; Chicago U., Astron. Astrophys. Ctr.]·Raveri, M. [MIT, Cambridge, Dept. Phys.; INFN, Genoa]·Rollins, R. P. [Jodrell Bank]·Roodman, A. [KIPAC, Menlo Park; SLAC]·Rosenfeld, R. [Sao Paulo, IFT; LIneA, Rio de Janeiro]·Ross, A. J. [Ohio State U., CCAPP]·Rykoff, E. S. [SLAC; KIPAC, Menlo Park]·Sanchez, J. [Baltimore, Space Telescope Sci.]·Secco, L. F. [Chicago U., KICP]·Sevilla-Noarbe, I. [Madrid, CIEMAT]·Sheldon, E. [Brookhaven]·Shin, T. [SUNY, Stony Brook]·Troxel, M. A. [Duke U.]·Tutusaus, I. [IRAP, Toulouse]·Varga, T. N. [ORIGINS, Garching; Garching, Max Planck Inst., MPE; Munich U.]·Wechsler, R. H. [KIPAC, Menlo Park; Stanford U.; SLAC]·Yanny, B. [Fermilab] (ORCID:0000000295412678)·Zhang, Y. [Cerro-Tololo InterAmerican Obs.]·Zuntz, J. [Edinburgh U., Inst. Astron.]·Aguena, M. [LIneA, Rio de Janeiro]·Annis, J. [Fermilab]·Bacon, D. [Portsmouth U., ICG]·Bocquet, S. [Munich U.]·Brooks, D. [University Coll. London]·Burke, D. L. [KIPAC, Menlo Park; SLAC]·Carretero, J. [Barcelona, IFAE]·Castander, F. J. [Barcelona, IEEC]·Costanzi, M. [IFPU, Trieste; Trieste Observ.]·da Costa, L. N. [LIneA, Rio de Janeiro]·De Vicente, J. [Madrid, CIEMAT]·Doel, P. [University Coll. London]·Ferrero, I. [Inst. Theor. Astrophys., Oslo]·Flaugher, B. [Fermilab] (ORCID:0000000223675049)·Frieman, J. [Chicago U., KICP; Fermilab] (ORCID:0000000340793263)·García-Bellido, J. [Madrid, IFT]·Gaztanaga, E. [Barcelona, IEEC; Portsmouth U., ICG]·Gutierrez, G. [Fermilab] (ORCID:0000000308250517)·Hinton, S. R. [Queensland U.]·Hollowood, D. L. [UC, Santa Cruz]·Honscheid, K. [Ohio State U., CCAPP; Ohio State U.]·James, D. J. [Harvard-Smithsonian Ctr. Astrophys.]·Kuehn, K. [Australia, CSIRO, North Ryde; Lowell Observ.]·Lima, M. [LIneA, Rio de Janeiro; Sao Paulo U., Sao Carlos]·Lin, H. [Fermilab]·Marshall, J. L. [Texas A-M]·Mena-Fernández, J. [LPSC, Grenoble]·Menanteau, F. [Illinois U., Urbana, Astron. Dept.; Illinois U., Urbana (main)]·Miquel, R. [Barcelona, IFAE; ICREA, Barcelona; Barcelona, Autonoma U.]·Ogando, R. L.C. [Rio de Janeiro Observ.]

Abstract

Characterization of the redshift distribution of ensembles of galaxies is pivotal for large scale structure cosmological studies. In this work, we focus on improving the Self-Organizing Map (SOM) methodology for photometric redshift estimation (SOMPZ), specifically in anticipation of the Dark Energy Survey Year 6 (DES Y6) data. This data set, featuring deeper and fainter galaxies than DES Year 3 (DES Y3), demands adapted techniques to ensure accurate recovery of the underlying redshift distribution. We investigate three strategies for enhancing the existing SOM-based approach used in DES Y3: 1) Replacing the Y3 SOM algorithm with one tailored for redshift estimation challenges; 2) Incorporating $\textit{g}$-band flux information to refine redshift estimates (i.e. using $\textit{griz}$ fluxes as opposed to only $\textit{riz}$); 3) Augmenting redshift data for galaxies where available. These methods are applied to DES Y3 data, and results are compared to the Y3 fiducial ones. Our analysis indicates significant improvements with the first two strategies, notably reducing the overlap between redshift bins. By combining strategies 1 and 2, we have successfully managed to reduce redshift bin overlap in DES Y3 by up to 66$\%$. Conversely, the third strategy, involving the addition of redshift data for selected galaxies as an additional feature in the method, yields inferior results and is abandoned. Our findings contribute to the advancement of weak lensing redshift characterization and lay the groundwork for better redshift characterization in DES Year 6 and future stage IV surveys, like the Rubin Observatory.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Campos, A. [Carnegie Mellon U.] (ORCID:0000000251240771), Yin, B. [Duke U.] (ORCID:0009000656049980), Dodelson, S. [Carnegie Mellon U.] (ORCID:0000000284463859), Amon, A. [Cambridge U., Inst. of Astron.], Alarcon, A. [Argonne; Barcelona, IEEC], Sánchez, C. [UPenn, Philadelphia], Bernstein, G. M. [UPenn, Philadelphia], Giannini, G. [Chicago U., KICP; Barcelona, IFAE] (ORCID:0000000237301750), Myles, J. [Princeton U., Astrophys. Sci. Dept.], Samuroff, S. [Northeastern U.], Alves, O. [U. Michigan, Ann Arbor], Andrade-Oliveira, F. [U. Michigan, Ann Arbor], Bechtol, K. [Wisconsin U., Madison], Becker, M. R. [Argonne], Blazek, J. [Northeastern U.], Camacho, H. [LIneA, Rio de Janeiro; Sao Paulo, IFT; Brookhaven], Carnero Rosell, A. [LIneA, Rio de Janeiro; IAC, La Laguna; Laguna U., Tenerife], Carrasco Kind, M. [Illinois U., Urbana, Astron. Dept.; Illinois U., Urbana (main)], Cawthon, R. [William-Mary Coll.], Chang, C. [Chicago U., Astron. Astrophys. Ctr.; Chicago U., KICP] (ORCID:0000000278870896), Chen, R. [Duke U.], Choi, A. [NASA, Goddard], Cordero, J. [Jodrell Bank], Davis, C. [KIPAC, Menlo Park], DeRose, J. [LBL, Berkeley], Diehl, H. T. [Fermilab] (ORCID:0000000283577467), Doux, C. [UPenn, Philadelphia; LPSC, Grenoble], Drlica-Wagner, A. [Chicago U., KICP; Chicago U., Astron. Astrophys. Ctr.; Fermilab] (ORCID:000000018251933X), Eckert, K. [UPenn, Philadelphia], Eifler, T. F. [Caltech, JPL; Arizona U., Astron. Dept. - Steward Observ.], Elvin-Poole, J. [Waterloo U.], Everett, S. [Caltech, JPL], Fang, X. [Arizona U., Astron. Dept. - Steward Observ.; UC, Berkeley, Astron. Dept.] (ORCID:0000000250549566), Ferté, A. [SLAC], Friedrich, O. [Cambridge U., Inst. of Astron.], Gatti, M. [UPenn, Philadelphia], Gruen, D. [Munich U.], Gruendl, R. A. [Illinois U., Urbana, Astron. Dept.; Illinois U., Urbana (main)], Harrison, I. [Cardiff U.], Hartley, W. G. [U. Geneva (main)], Herner, K. [Fermilab], Huang, H. [Arizona U., Astron. Dept. - Steward Observ.; Arizona U.], Huff, E. M. [Caltech, JPL], Jarvis, M. [UPenn, Philadelphia], Krause, E. [Arizona U., Astron. Dept. - Steward Observ.], Kuropatkin, N. [Fermilab], Leget, P.-F. [KIPAC, Menlo Park], MacCrann, N. [Cambridge U., DAMTP], McCullough, J. [KIPAC, Menlo Park] (ORCID:0000000244753456), Navarro-Alsina, A. [Campinas State U.], Pandey, S. [UPenn, Philadelphia], Prat, J. [Nordita; Chicago U., Astron. Astrophys. Ctr.], Raveri, M. [MIT, Cambridge, Dept. Phys.; INFN, Genoa], Rollins, R. P. [Jodrell Bank], Roodman, A. [KIPAC, Menlo Park; SLAC], Rosenfeld, R. [Sao Paulo, IFT; LIneA, Rio de Janeiro], Ross, A. J. [Ohio State U., CCAPP], Rykoff, E. S. [SLAC; KIPAC, Menlo Park], Sanchez, J. [Baltimore, Space Telescope Sci.], Secco, L. F. [Chicago U., KICP], Sevilla-Noarbe, I. [Madrid, CIEMAT], Sheldon, E. [Brookhaven], Shin, T. [SUNY, Stony Brook], Troxel, M. A. [Duke U.], Tutusaus, I. [IRAP, Toulouse], Varga, T. N. [ORIGINS, Garching; Garching, Max Planck Inst., MPE; Munich U.], Wechsler, R. H. [KIPAC, Menlo Park; Stanford U.; SLAC], Yanny, B. [Fermilab] (ORCID:0000000295412678), Zhang, Y. [Cerro-Tololo InterAmerican Obs.], Zuntz, J. [Edinburgh U., Inst. Astron.], Aguena, M. [LIneA, Rio de Janeiro], Annis, J. [Fermilab], Bacon, D. [Portsmouth U., ICG], Bocquet, S. [Munich U.], Brooks, D. [University Coll. London], Burke, D. L. [KIPAC, Menlo Park; SLAC], Carretero, J. [Barcelona, IFAE], Castander, F. J. [Barcelona, IEEC], Costanzi, M. [IFPU, Trieste; Trieste Observ.], da Costa, L. N. [LIneA, Rio de Janeiro], De Vicente, J. [Madrid, CIEMAT], Doel, P. [University Coll. London], Ferrero, I. [Inst. Theor. Astrophys., Oslo], Flaugher, B. [Fermilab] (ORCID:0000000223675049), Frieman, J. [Chicago U., KICP; Fermilab] (ORCID:0000000340793263), García-Bellido, J. [Madrid, IFT], Gaztanaga, E. [Barcelona, IEEC; Portsmouth U., ICG], Gutierrez, G. [Fermilab] (ORCID:0000000308250517), Hinton, S. R. [Queensland U.], Hollowood, D. L. [UC, Santa Cruz], Honscheid, K. [Ohio State U., CCAPP; Ohio State U.], James, D. J. [Harvard-Smithsonian Ctr. Astrophys.], Kuehn, K. [Australia, CSIRO, North Ryde; Lowell Observ.], Lima, M. [LIneA, Rio de Janeiro; Sao Paulo U., Sao Carlos], Lin, H. [Fermilab], Marshall, J. L. [Texas A-M], Mena-Fernández, J. [LPSC, Grenoble], Menanteau, F. [Illinois U., Urbana, Astron. Dept.; Illinois U., Urbana (main)], Miquel, R. [Barcelona, IFAE; ICREA, Barcelona; Barcelona, Autonoma U.], Ogando, R. L.C. [Rio de Janeiro Observ.]. 2026-07-27. Enhancing weak lensing redshift distribution characterization by optimizing the Dark Energy Survey Self-Organizing Map Photo-z method. https://doi.org/10.33232/001c.165871

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related reports

Performance evaluation of neutron noise analysis in detecting special nuclear materials

Reliable and rapid inspection techniques play a vital role in preventing illicit trafficking of special nuclear materials. Active interrogation systems using neutrons produced by portable, high-flux deuterium-deuterium or deuterium-tritium neutron generators are being actively developed as a secondary scanning tool for this purpose. In this study, a neutron noise analysis-based approach for detecting unshielded and shielded special nuclear materials by using a pulsed deuterium-tritium neutron generator was evaluated. Here, this approach analyzes the fluctuation of neutron counts. Its performance was quantified with regard to time-to-detection to achieve a minimum probability of detection of 99% and a probability of false alarm of less than 1% considering various amounts of special nuclear materials and different shielding configurations. It was demonstrated that this approach could detect 17 uranium slugs in 5 s given a neutron generator yield of 8.1 × 10 7 n/s. These slugs could be detected within a reasonable time frame (200 s) when they were shielded by 10.16 cm of high-density polyethylene. The results obtained using the neutron noise analysis approach were compared with those obtained using the commonly used differential die-away analysis technique, a sensitive technique for detecting the presence of fissile materials by utilizing the prompt fission neutrons produced when the source neutrons from a neutron generator are completely diminished. For example, the time to detect 2 unshielded uranium slugs was 2.1 s when using the differential die-away analysis technique; it increased to 93 s for the neutron noise analysis approach. Although the noise analysis-based approach exhibits an overall performance which is not as good as that of differential die-away, neutron noise provides an alternative method for effective detection of special nuclear materials.

46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND ↗

A proximity-focusing RICH detector for the ePIC Experiment at the EIC

The Electron-Proton/Ion Collider Experiment (ePIC) will be a large, multi-purpose detector to be installed at the Electron-Ion Collider (EIC) being built at Brookhaven National Laboratory. As robust particle identification (PID) capabilities are essential for fully realizing the EIC science program, ePIC contains several PID subsystems spanning different angular ranges. PID capability in the electron-going endcap is provided by a proximity-focusing Ring Imaging Cherenkov detector (pfRICH) designed to deliver at least 3σ separation between pions and kaons for momenta up to 7 GeV/ c . It will also aid with electron-hadron discrimination at low momentum and assist in the determination of the collision time (t 0 ). This contribution will summarize the design of the pfRICH as well as ongoing fabrication and component testing efforts. geant-based performance simulations will also be discussed.

46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND ↗

Design of a high voltage delivery system for noble liquid time projection chambers

Noble liquid time projection chambers (TPCs) are a leading technology in the detection of ionizing radiation, particularly in applications such as accelerator neutrino physics, dark matter detection, and neutrinoless double beta decay. This work addresses the design considerations for implementing stable high voltage (HV) systems within large noble liquid TPCs, with a focus on the nEXO experiment. Utilizing insights from prior HV research and experimental investigations, we outline factors influencing HV stability and discuss design choices to improve stability and prevent electrical discharges. A novel HV delivery system concept is presented, tailored for the nEXO TPC, which incorporates these design considerations while also meeting the stringent radiopurity requirements of the nEXO neutrinoless double beta decay search. These design considerations and their specific implementation towards a HV delivery system offer guidance to future experiments applying high voltage in noble liquid environments.

46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND ↗