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Dark Energy Survey Year 3 Results: Mis-centering calibration and X-ray-richness scaling relations in redMaPPer clusters

Research output: Working paper › Preprint

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Dark Energy Survey Year 3 Results: Mis-centering calibration and X-ray-richness scaling relations in redMaPPer clusters. / Kelly, P.; Jobel, J.; Eiger, O. et al.
Arxiv, 2024.

Research output: Working paper › Preprint

Harvard

Kelly, P, Jobel, J, Eiger, O, Abd, A, Jeltema, TE, Giles, P, Hollowood, DL, Wilkinson, RD, Turner, DJ, Bhargava, S, Everett, S, Farahi, A, Romer, AK, Rykoff, ES, Wang, F, Bocquet, S, Cross, D, Faridjoo, R, Franco, J, Gardner, G, Kwiecien, M, Laubner, D, McDaniel, A, O'Donnell, JH, Sanchez, L, Schmidt, E, Sripada, S, Swart, A, Upsdell, E, Webber, A, Aguena, M, Allam, S, Alves, O, Bacon, D, Brooks, D, Burke, DL, Rosell, AC, Carretero, J, Collins, CA, Costanzi, M, da Costa, LN, Pereira, MES, Davis, TM, Doel, P, Ferrero, I, Frieman, J, García-Bellido, J, Giannini, G, Gruen, D, Gruendl, RA, Hilton, M, Hinton, SR, Honscheid, K, James, DJ, Kuehn, K, Mann, RG, Marshall, JL, Mena-Fernández, J, Miller, CJ, Miquel, R, Myles, J, Palmese, A, Pieres, A, Malagón, AAP, Rooney, PJ, Sahlen, M, Sanchez, E, Cid, DS, Schubnell, M, Sevilla-Noarbe, I, Smith, M, Stott, JP, Suchyta, E, Swanson, MEC, Tarle, G, To, C, Viana, PTP, Weaverdyck, N & Wiseman, P 2024 'Dark Energy Survey Year 3 Results: Mis-centering calibration and X-ray-richness scaling relations in redMaPPer clusters' Arxiv. <https://arxiv.org/abs/2310.13207v1>

APA

Kelly, P., Jobel, J., Eiger, O., Abd, A., Jeltema, T. E., Giles, P., Hollowood, D. L., Wilkinson, R. D., Turner, D. J., Bhargava, S., Everett, S., Farahi, A., Romer, A. K., Rykoff, E. S., Wang, F., Bocquet, S., Cross, D., Faridjoo, R., Franco, J., ... Wiseman, P. (2024). Dark Energy Survey Year 3 Results: Mis-centering calibration and X-ray-richness scaling relations in redMaPPer clusters. Arxiv. https://arxiv.org/abs/2310.13207v1

Vancouver

Kelly P, Jobel J, Eiger O, Abd A, Jeltema TE, Giles P et al. Dark Energy Survey Year 3 Results: Mis-centering calibration and X-ray-richness scaling relations in redMaPPer clusters. Arxiv. 2024 Jul 24.

Author

Kelly, P. ; Jobel, J. ; Eiger, O. et al. / Dark Energy Survey Year 3 Results : Mis-centering calibration and X-ray-richness scaling relations in redMaPPer clusters. Arxiv, 2024.

Bibtex

@techreport{d4645bfd9cbb42ccac8cb3b76993a507,
title = "Dark Energy Survey Year 3 Results: Mis-centering calibration and X-ray-richness scaling relations in redMaPPer clusters",
abstract = "We use Dark Energy Survey Year 3 (DES Y3) clusters with archival X-ray data from XMM-Newton and Chandra to assess the centering performance of the redMaPPer cluster finder and to measure key richness observable scaling relations. In terms of centering, we find that 10-20% of redMaPPer clusters are miscentered with no significant difference in bins of low versus high richness ($2040$) or redshift ($0.2",
keywords = "astro-ph.CO",
author = "P. Kelly and J. Jobel and O. Eiger and A. Abd and Jeltema, {T. E.} and P. Giles and Hollowood, {D. L.} and Wilkinson, {R. D.} and Turner, {D. J.} and S. Bhargava and S. Everett and A. Farahi and Romer, {A. K.} and Rykoff, {E. S.} and F. Wang and S. Bocquet and D. Cross and R. Faridjoo and J. Franco and G. Gardner and M. Kwiecien and D. Laubner and A. McDaniel and O'Donnell, {J. H.} and L. Sanchez and E. Schmidt and S. Sripada and A. Swart and E. Upsdell and A. Webber and M. Aguena and S. Allam and O. Alves and D. Bacon and D. Brooks and Burke, {D. L.} and Rosell, {A. Carnero} and J. Carretero and Collins, {C. A.} and M. Costanzi and {da Costa}, {L. N.} and Pereira, {M. E. S.} and Davis, {T. M.} and P. Doel and I. Ferrero and J. Frieman and J. Garc{\'i}a-Bellido and G. Giannini and D. Gruen and Gruendl, {R. A.} and M. Hilton and Hinton, {S. R.} and K. Honscheid and James, {D. J.} and K. Kuehn and Mann, {R. G.} and Marshall, {J. L.} and J. Mena-Fern{\'a}ndez and Miller, {C. J.} and R. Miquel and J. Myles and A. Palmese and A. Pieres and Malag{\'o}n, {A. A. Plazas} and Rooney, {P. J.} and M. Sahlen and E. Sanchez and Cid, {D. Sanchez} and M. Schubnell and I. Sevilla-Noarbe and M. Smith and Stott, {J. P.} and E. Suchyta and Swanson, {M. E. C.} and G. Tarle and C. To and Viana, {P. T. P.} and N. Weaverdyck and P. Wiseman",
year = "2024",
month = jul,
day = "24",
language = "English",
publisher = "Arxiv",
type = "WorkingPaper",
institution = "Arxiv",

}

RIS

TY - UNPB

T1 - Dark Energy Survey Year 3 Results

T2 - Mis-centering calibration and X-ray-richness scaling relations in redMaPPer clusters

AU - Kelly, P.

AU - Jobel, J.

AU - Eiger, O.

AU - Abd, A.

AU - Jeltema, T. E.

AU - Giles, P.

AU - Hollowood, D. L.

AU - Wilkinson, R. D.

AU - Turner, D. J.

AU - Bhargava, S.

AU - Everett, S.

AU - Farahi, A.

AU - Romer, A. K.

AU - Rykoff, E. S.

AU - Wang, F.

AU - Bocquet, S.

AU - Cross, D.

AU - Faridjoo, R.

AU - Franco, J.

AU - Gardner, G.

AU - Kwiecien, M.

AU - Laubner, D.

AU - McDaniel, A.

AU - O'Donnell, J. H.

AU - Sanchez, L.

AU - Schmidt, E.

AU - Sripada, S.

AU - Swart, A.

AU - Upsdell, E.

AU - Webber, A.

AU - Aguena, M.

AU - Allam, S.

AU - Alves, O.

AU - Bacon, D.

AU - Brooks, D.

AU - Burke, D. L.

AU - Rosell, A. Carnero

AU - Carretero, J.

AU - Collins, C. A.

AU - Costanzi, M.

AU - da Costa, L. N.

AU - Pereira, M. E. S.

AU - Davis, T. M.

AU - Doel, P.

AU - Ferrero, I.

AU - Frieman, J.

AU - García-Bellido, J.

AU - Giannini, G.

AU - Gruen, D.

AU - Gruendl, R. A.

AU - Hilton, M.

AU - Hinton, S. R.

AU - Honscheid, K.

AU - James, D. J.

AU - Kuehn, K.

AU - Mann, R. G.

AU - Marshall, J. L.

AU - Mena-Fernández, J.

AU - Miller, C. J.

AU - Miquel, R.

AU - Myles, J.

AU - Palmese, A.

AU - Pieres, A.

AU - Malagón, A. A. Plazas

AU - Rooney, P. J.

AU - Sahlen, M.

AU - Sanchez, E.

AU - Cid, D. Sanchez

AU - Schubnell, M.

AU - Sevilla-Noarbe, I.

AU - Smith, M.

AU - Stott, J. P.

AU - Suchyta, E.

AU - Swanson, M. E. C.

AU - Tarle, G.

AU - To, C.

AU - Viana, P. T. P.

AU - Weaverdyck, N.

AU - Wiseman, P.

PY - 2024/7/24

Y1 - 2024/7/24

N2 - We use Dark Energy Survey Year 3 (DES Y3) clusters with archival X-ray data from XMM-Newton and Chandra to assess the centering performance of the redMaPPer cluster finder and to measure key richness observable scaling relations. In terms of centering, we find that 10-20% of redMaPPer clusters are miscentered with no significant difference in bins of low versus high richness ($2040$) or redshift ($0.2

AB - We use Dark Energy Survey Year 3 (DES Y3) clusters with archival X-ray data from XMM-Newton and Chandra to assess the centering performance of the redMaPPer cluster finder and to measure key richness observable scaling relations. In terms of centering, we find that 10-20% of redMaPPer clusters are miscentered with no significant difference in bins of low versus high richness ($2040$) or redshift ($0.2

KW - astro-ph.CO

M3 - Preprint

BT - Dark Energy Survey Year 3 Results

PB - Arxiv

ER -