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  Dark Energy Survey year 3 results: point spread function modelling

Jarvis, M., Bernstein, G. M., Amon, A., Davis, C., Leget, P. F., Bechtol, K., et al. (2020). Dark Energy Survey year 3 results: point spread function modelling. Monthly Notices of the Royal Astronomical Society, 501(1), 1282-1299. doi:10.1093/mnras/staa3679.

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Jarvis, M., Author
Bernstein, G. M., Author
Amon, A., Author
Davis, C., Author
Leget, P. F., Author
Bechtol, K., Author
Harrison, I., Author
Gatti, M., Author
Roodman, A., Author
Chang, C., Author
Chen, R., Author
Choi, A., Author
Desai, S., Author
Drlica-Wagner, A., Author
Gruen, D., Author
Gruendl, R. A., Author
Hernandez, A., Author
MacCrann, N., Author
Meyers, J., Author
Navarro-Alsina, A., Author
Pandey, S., AuthorPlazas, A. A., AuthorSecco, L. F., AuthorSheldon, E., AuthorTroxel, M. A., AuthorVorperian, S., AuthorWei, K., AuthorZuntz, J., AuthorAbbott, T. M. C., AuthorAguena, M., AuthorAllam, S., AuthorAvila, S., AuthorBhargava, S., AuthorBridle, S. L., AuthorBrooks, D., AuthorRosell, A. Carnero, AuthorKind, M. Carrasco, AuthorCarretero, J., AuthorCostanzi, M., Authorda Costa, L. N., AuthorVicente, J. De, AuthorDiehl, H. T., AuthorDoel, P., AuthorEverett, S., AuthorFlaugher, B., AuthorFosalba, P., AuthorFrieman, J., AuthorGarcia-Bellido, J., AuthorGaztanaga, E., AuthorGerdes, D. W., AuthorGutierrez, G., AuthorHinton, S. R., AuthorHollowood, D. L., AuthorHonscheid, K., AuthorJames, D. J., AuthorKent, S., AuthorKuehn, K., AuthorKuropatkin, N., AuthorLahav, O., AuthorMaia, M. A. G., AuthorMarch, M., AuthorMarshall, J. L., AuthorMelchior, P., AuthorMenanteau, F., AuthorMiquel, R., AuthorOgando, R. L. C., AuthorPaz-Chinchon, F., AuthorRykoff, E. S., AuthorSanchez, E., AuthorScarpine, V., AuthorSchubnell, M., AuthorSerrano, S., AuthorSevilla-Noarbe, I., AuthorSmith, M., AuthorSuchyta, E., AuthorSwanson, M. E. C., AuthorTarle, G., AuthorVarga, T. N.1, Author           Walker, A. R., AuthorWester, W., AuthorWilkinson, R.D., Author more..
Affiliations:
1Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159895              

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 Abstract: We introduce a new software package for modelling the point spread function (PSF) of astronomical images, called piff (PSFs In the Full FOV), which we apply to the first three years (known as Y3) of the Dark Energy Survey (DES) data. We describe the relevant details about the algorithms used by piff to model the PSF, including how the PSF model varies across the field of view (FOV). Diagnostic results show that the systematic errors from the PSF modelling are very small over the range of scales that are important for the DES Y3 weak lensing analysis. In particular, the systematic errors from the PSF modelling are significantly smaller than the corresponding results from the DES year one (Y1) analysis. We also briefly describe some planned improvements to piff that we expect to further reduce the modelling errors in future analyses.

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 Dates: 2020-11-26
 Publication Status: Published online
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1093/mnras/staa3679
Other: LOCALID: 3289546
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Title: Monthly Notices of the Royal Astronomical Society
  Other : Mon. Not. R. Astron. Soc.
Source Genre: Journal
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Publ. Info: Oxford : Oxford University Press
Pages: - Volume / Issue: 501 (1) Sequence Number: - Start / End Page: 1282 - 1299 Identifier: ISSN: 1365-8711
CoNE: https://pure.mpg.de/cone/journals/resource/1000000000024150