4.6 Article

The strong gravitational lens finding challenge

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ASTRONOMY & ASTROPHYSICS
卷 625, 期 -, 页码 -

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EDP SCIENCES S A
DOI: 10.1051/0004-6361/201832797

关键词

gravitational lensing: strong; methods: data analysis

资金

  1. World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan
  2. project GLENCO
  3. European Seventh Framework Programme, Ideas [259349]
  4. ERC advanced grant LIDA
  5. ESA-NPI [491-2016]
  6. Enrico Fermi Institute at the University of Chicago
  7. University of Chicago Provost's Office
  8. NSFC [11503064]
  9. Shanghai Natural Science Foundation [15ZR1446700]
  10. Kavli Institute for Cosmological Physics at the University of Chicago [NSF PHY-1125897]
  11. Kavli Foundation
  12. NWO-VICI grant [639.043.308]
  13. Netherlands Research School for Astronomy (NOVA)
  14. Samenwerkingsverband Noord Nederland
  15. European fund for regional development, Dutch Ministry of economic affairs
  16. Provinces of Groningen and Drenthe
  17. STFC [ST/P000584/1] Funding Source: UKRI

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Large-scale imaging surveys will increase the number of galaxy-scale strong lensing candidates by maybe three orders of magnitudes beyond the number known today. Finding these rare objects will require picking them out of at least tens of millions of images, and deriving scientific results from them will require quantifying the efficiency and bias of any search method. To achieve these objectives automated methods must be developed. Because gravitational lenses are rare objects, reducing false positives will be particularly important. We present a description and results of an open gravitational lens finding challenge. Participants were asked to classify 100 000 candidate objects as to whether they were gravitational lenses or not with the goal of developing better automated methods for finding lenses in large data sets. A variety of methods were used including visual inspection, arc and ring finders, support vector machines (SVM) and convolutional neural networks (CNN). We find that many of the methods will be easily fast enough to analyse the anticipated data flow. In test data, several methods are able to identify upwards of half the lenses after applying some thresholds on the lens characteristics such as lensed image brightness, size or contrast with the lens galaxy without making a single false-positive identification. This is significantly better than direct inspection by humans was able to do. Having multi-band, ground based data is found to be better for this purpose than single-band space based data with lower noise and higher resolution, suggesting that multi-colour data is crucial. Multi-band space based data will be superior to ground based data. The most difficult challenge for a lens finder is differentiating between rare, irregular and ring-like face-on galaxies and true gravitational lenses. The degree to which the efficiency and biases of lens finders can be quantified largely depends on the realism of the simulated data on which the finders are trained.

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Article Astronomy & Astrophysics

Joint analysis of Dark Energy Survey Year 3 data and CMB lensing and cosmological constraints

C. Chang, Y. Omori, E. J. Baxter, C. Doux, A. Choi, S. Pandey, A. Alarcon, O. Alves, A. Amon, F. Andrade-Oliveira, K. Bechtol, M. R. Becker, G. M. Bernstein, F. Bianchini, J. Blazek, L. E. Bleem, H. Camacho, A. Campos, A. Carnero Rosell, M. Carrasco Kind, R. Cawthon, R. Chen, J. Cordero, T. M. Crawford, M. Crocce, C. Davis, J. DeRose, S. Dodelson, A. Drlica-Wagner, K. Eckert, T. F. Eifler, F. Elsner, J. Elvin-Poole, S. Everett, X. Fang, A. Ferte, P. Fosalba, O. Friedrich, M. Gatti, G. Giannini, D. Gruen, R. A. Gruendl, I. Harrison, K. Herner, H. Huang, E. M. Huff, D. Huterer, M. Jarvis, A. Kovacs, E. Krause, N. Kuropatkin, P. -F. Leget, P. Lemos, A. R. Liddle, N. MacCrann, J. McCullough, J. Muir, J. Myles, A. Navarro-Alsina, Y. Park, A. Porredon, J. Prat, M. Raveri, R. P. Rollins, A. Roodman, R. Rosenfeld, A. J. Ross, E. S. Rykoff, C. Sanchez, J. Sanchez, L. F. Secco, I Sevilla-Noarbe, E. Sheldon, T. Shin, M. A. Troxel, I. Tutusaus, T. N. Varga, N. Weaverdyck, R. H. Wechsler, W. L. K. Wu, B. Yanny, B. Yin, Y. Zhang, J. Zuntz, T. M. C. Abbott, M. Aguena, S. Allam, J. Annis, D. Bacon, B. A. Benson, E. Bertin, S. Bocquet, D. Brooks, D. L. Burke, J. E. Carlstrom, J. Carretero, C. L. Chang, R. Chown, M. Costanzi, L. N. da Costa, A. T. Crites, M. E. S. Pereira, T. de Haan, J. De Vicente, S. Desai, H. T. Diehl, M. A. Dobbs, P. Doel, W. Everett, I. Ferrero, B. Flaugher, D. Friedel, J. Frieman, J. Garcia-Bellido, E. Gaztanaga, E. M. George, T. Giannantonio, N. W. Halverson, S. R. Hinton, G. P. Holder, D. L. Hollowood, W. L. Holzapfel, K. Honscheid, J. D. Hrubes, D. J. James, L. Knox, K. Kuehn, O. Lahav, A. T. Lee, M. Lima, D. Luong-Van, M. March, J. J. McMahon, P. Melchior, F. Menanteau, S. S. Meyer, R. Miquel, L. Mocanu, J. J. Mobr, R. Morgan, T. Natoli, S. Padin, A. Palmese, F. Paz-Chinchon, A. Pieres, A. A. Plazas Malagon, C. Pryke, C. L. Reichardt, M. Rodriguez-Monroy, A. K. Romer, J. E. Ruhl, E. Sanchez, K. K. Schaffer, M. Schubnell, S. Serrano, E. Shirokoff, M. Smith, Z. Staniszewski, A. A. Stark, E. Suchyta, G. Tarle, D. Thomas, C. To, J. D. Vieira, J. Weller, R. Williamson

Summary: Cross-correlations between galaxy positions and galaxy shears with CMB lensing maps are measured and modeled to study the large-scale structure in the Universe. These cross-correlations provide less systematic biases compared to internal galaxy surveys. Constraints on cosmological parameters are obtained using the cross-correlation measurements, and the results are consistent with cosmic shear measurements but lower than Planck's primary CMB measurements in terms of S8 value.

PHYSICAL REVIEW D (2023)

Article Astronomy & Astrophysics

Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. I. Construction of CMB lensing maps and modeling choices

Y. Omori, E. J. Baxter, C. Chang, O. Friedrich, A. Alarcon, O. Alves, A. Amon, F. Andrade-Oliveira, K. Bechtol, M. R. Becker, G. M. Bernstein, J. Blazek, L. E. Bleem, H. Camacho, A. Campos, A. Carnero Rosell, M. Carrasco Kind, R. Cawthon, R. Chen, A. Choi, J. Cordero, T. M. Crawford, M. Crocce, C. Davis, J. DeRose, S. Dodelson, C. Doux, A. Drlica-Wagner, K. Eckert, T. F. Eifler, F. Elsner, J. Elvin-Poole, S. Everett, X. Fang, A. Ferte, P. Fosalba, M. Gatti, G. Giannini, D. Gruen, R. A. Gruendl, I. Harrison, K. Herner, H. Huang, E. M. Huff, D. Huterer, M. Jarvis, E. Krause, N. Kuropatkin, P. -F. Leget, P. Lemos, A. R. Liddle, N. MacCrann, J. McCullough, J. Muir, J. Myles, A. Navarro-Alsina, S. Pandey, Y. Park, A. Porredon, J. Prat, M. Raveri, R. P. Rollins, A. Roodman, R. Rosenfeld, A. J. Ross, E. S. Rykoff, C. Sanchez, J. Sanchez, L. F. Secco, I. Sevilla-Noarbe, E. Sheldon, T. Shin, M. A. Troxel, I. Tutusaus, T. N. Varga, N. Weaverdyck, R. H. Wechsler, W. L. K. Wu, B. Yanny, B. Yin, Y. Zhang, J. Zuntz, T. M. C. Abbott, M. Aguena, S. Allam, J. Annis, D. Bacon, B. A. Benson, E. Bertin, S. Bocquet, D. Brooks, D. L. Burke, J. E. Carlstrom, J. Carretero, C. L. Chang, R. Chown, M. Costanzi, L. N. da Costa, A. T. Crites, M. E. S. Pereira, T. de Haan, J. De Vicente, S. Desai, H. T. Diehl, M. A. Dobbs, P. Doel, W. Everett, I. Ferrero, B. Flaugher, D. Friedel, J. Frieman, J. Garcia-Bellido, E. Gaztanaga, E. M. George, T. Giannantonio, N. W. Halverson, S. R. Hinton, G. P. Holder, D. L. Hollowood, W. L. Holzapfel, K. Honscheid, J. D. Hrubes, D. J. James, L. Knox, K. Kuehn, O. Lahav, A. T. Lee, M. Lima, D. Luong-Van, M. March, J. J. McMahon, P. Melchior, F. Menanteau, S. S. Meyer, R. Miquel, L. Mocanu, J. J. Mohr, R. Morgan, T. Natoli, S. Padin, A. Palmese, F. Paz-Chinchon, A. Pieres, A. A. Plazas Malagon, C. Pryke, C. L. Reichardt, A. K. Romer, J. E. Ruhl, E. Sanchez, K. K. Schaffer, M. Schubnell, S. Serrano, E. Shirokoff, M. Smith, Z. Staniszewski, A. A. Stark, E. Suchyta, G. Tarle, D. Thomas, C. To, J. D. Vieira, J. Weller, R. Williamson

Summary: Joint analyses of cross-correlations between galaxy measurements and lensing of the cosmic microwave background (CMB) provide powerful constraints on the large-scale structure of the Universe. In this article, we present an improved CMB lensing map in the SPT-SZ survey footprint and the analysis methodology to extract cosmological information. We find that the joint analysis of CMB lensing cross-correlations can provide constraints on the shear calibration amplitude at the 5% to 10% level.

PHYSICAL REVIEW D (2023)

Article Astronomy & Astrophysics

Measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES

E. Schiappucci, F. Bianchini, M. Aguena, M. Archipley, L. Balkenhol, L. E. Bleem, P. Chaubal, T. M. Crawford, S. Grandis, Y. Omori, C. L. Reichardt, E. Rozo, E. S. Rykoff, C. To, T. M. C. Abbott, P. A. R. Ade, O. Alves, A. J. Anderson, F. Andrade-Oliveira, J. Annis, J. S. Avva, D. Bacon, K. Benabed, A. N. Bender, B. A. Benson, G. M. Bernstein, E. Bertin, S. Bocquet, F. R. Bouchet, D. Brooks, D. L. Burke, J. E. Carlstrom, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, T. W. Cecil, C. L. Chang, P. M. Chichura, T. -L. Chou, M. Costanzi, A. Cukierman, L. N. da Costa, C. Daley, T. de Haan, S. Desai, K. R. Dibert, H. T. Diehl, M. A. Dobbs, P. Doel, C. Doux, D. Dutcher, S. Everett, W. Everett, C. Feng, K. R. Ferguson, I. Ferrero, A. Ferte, B. Flaugher, A. Foster, J. Frieman, S. Galli, A. E. Gambrel, J. Garcia-Bellido, R. W. Gardner, M. Gatti, T. Giannantonio, N. Goeckner-Wald, D. Gruen, R. Gualtieri, S. Guns, G. Gutierrez, N. W. Halverson, S. R. Hinton, E. Hivon, G. P. Holder, D. L. Hollowood, W. L. Holzapfel, K. Honscheid, J. C. Hood, N. Huang, D. J. James, L. Knox, M. Korman, K. Kuehn, C. -L. Kuo, O. Lahav, A. T. Lee, C. Lidman, M. Lima, A. E. Lowitz, C. Lu, M. March, J. Mena-Fernandez, F. Menanteau, M. Millea, R. Miquel, J. J. Mohr, J. Montgomery, J. Muir, T. Natoli, G. I. Noble, V. Novosad, R. L. C. Ogando, S. Padin, Z. Pan, F. Paz-Chinchon, M. E. S. Pereira, A. Pieres, A. A. Plazas Malagon, K. Prabhu, J. Prat, W. Quan, A. Rahlin, M. Raveri, M. Rodriguez-Monroy, A. K. Romer, M. Rouble, J. E. Ruhl, E. Sanchez, V. Scarpine, M. Schubnell, G. Smecher, M. Smith, M. Soares-Santos, J. A. Sobrin, E. Suchyta, A. Suzuki, G. Tarle, D. Thomas, K. L. Thompson, B. Thorne, C. Tucker, C. Umilta, J. D. Vieira, M. Vincenzi, G. Wang, N. Weaverdyck, J. Weller, N. Whitehorn, W. L. K. Wu, V. Yefremenko, M. R. Young

Summary: We use the pairwise kinematic Sunyaev-Zel'dovich (KSZ) effect to infer the average optical depth of a sample of optically selected galaxy clusters from the Dark Energy Survey. The pairwise KSZ signal is detected at 4.1 sigma in cosmic microwave background temperature maps from two years of observations with the SPT-3G camera. After data cuts, there are 24,580 clusters in the observed area. We calculate the mean optical depth using two techniques: the pairwise KSZ signal gives tau over bar e = (2.97 +/- 0.73) x 10-3, while the thermal SZ signal gives tau over bar e = (2.51 +/- 0.55stat +/- 0.15syst) x 10-3. The two measures agree within 0.6 sigma. We perform systematic checks to ensure the validity of our analysis.

PHYSICAL REVIEW D (2023)

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