Weak-lensing mass calibration of the Atacama Cosmology Telescope equatorial Sunyaev-Zeldovich cluster sample with the Canada-France-Hawaii telescope stripe 82 survey

Battaglia; A. Leauthaud; H. Miyatake; M. Hasselfield; M. B. Gralla; R. Allison; J. R. Bond; E. Calabrese; D. Crichton; M. J. Devlin; J. Dunkley; R. Dünner; T. Erben; S. Ferrara; M. Halpern; M. Hilton; J. C. Hill; A. D. Hincks; R. Hložek; K. M. Huffenberger; J. P. Hughes; J. P. Kneib; A. Kosowsky; M. Makler; T. A. Marriage; F. Menanteau; L. Miller; K. Moodley; B. Moraes; M. D. Niemack; L. Page; H. Shan; N. Sehgal; B. D. Sherwin; J. L. Sievers; C. Sifón; D. N. Spergel; S. T. Staggs; J. E. Taylor; R. Thornton; L. Van Waerbeke; E. J. Wollack

doi:10.1088/1475-7516/2016/08/013

Weak-lensing mass calibration of the Atacama Cosmology Telescope equatorial Sunyaev-Zeldovich cluster sample with the Canada-France-Hawaii telescope stripe 82 survey

Battaglia, A. Leauthaud, H. Miyatake, M. Hasselfield, M. B. Gralla, R. Allison, J. R. Bond, E. Calabrese, D. Crichton, M. J. Devlin, J. Dunkley, R. Dünner, T. Erben, S. Ferrara, M. Halpern, M. Hilton, J. C. Hill, A. D. Hincks, R. Hložek, K. M. HuffenbergerJ. P. Hughes, J. P. Kneib, A. Kosowsky, M. Makler, T. A. Marriage, F. Menanteau, L. Miller, K. Moodley, B. Moraes, M. D. Niemack, L. Page, H. Shan, N. Sehgal, B. D. Sherwin, J. L. Sievers, C. Sifón, D. N. Spergel, S. T. Staggs, J. E. Taylor, R. Thornton, L. Van Waerbeke, E. J. Wollack

Research output: Contribution to journal › Review article › peer-review

31 Scopus citations

Abstract

Mass calibration uncertainty is the largest systematic effect for using clusters of galaxies to constrain cosmological parameters. We present weak lensing mass measurements from the Canada-France-Hawaii Telescope Stripe 82 Survey for galaxy clusters selected through their high signal-to-noise thermal Sunyaev-Zeldovich (tSZ) signal measured with the Atacama Cosmology Telescope (ACT). For a sample of 9 ACT clusters with a tSZ signal-to-noise greater than five the average weak lensing mass is (4.8±0.8) ×10¹⁴ M_o, consistent with the tSZ mass estimate of (4.70±1.0) ×10¹⁴ M_o which assumes a universal pressure profile for the cluster gas. Our results are consistent with previous weak-lensing measurements of tSZ-detected clusters from the Planck satellite. When comparing our results, we estimate the Eddington bias correction for the sample intersection of Planck and weak-lensing clusters which was previously excluded.

Original language	English (US)
Article number	013
Journal	Journal of Cosmology and Astroparticle Physics
Volume	2016
Issue number	8
DOIs	https://doi.org/10.1088/1475-7516/2016/08/013
State	Published - Aug 8 2016

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics

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10.1088/1475-7516/2016/08/013

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Battaglia, Leauthaud, A., Miyatake, H., Hasselfield, M., Gralla, M. B., Allison, R., Bond, J. R., Calabrese, E., Crichton, D., Devlin, M. J., Dunkley, J., Dünner, R., Erben, T., Ferrara, S., Halpern, M., Hilton, M., Hill, J. C., Hincks, A. D., Hložek, R., ... Wollack, E. J. (2016). Weak-lensing mass calibration of the Atacama Cosmology Telescope equatorial Sunyaev-Zeldovich cluster sample with the Canada-France-Hawaii telescope stripe 82 survey. Journal of Cosmology and Astroparticle Physics, 2016(8), Article 013. https://doi.org/10.1088/1475-7516/2016/08/013

@article{3717af777e4043c6977be5b8f17ae457,

title = "Weak-lensing mass calibration of the Atacama Cosmology Telescope equatorial Sunyaev-Zeldovich cluster sample with the Canada-France-Hawaii telescope stripe 82 survey",

abstract = "Mass calibration uncertainty is the largest systematic effect for using clusters of galaxies to constrain cosmological parameters. We present weak lensing mass measurements from the Canada-France-Hawaii Telescope Stripe 82 Survey for galaxy clusters selected through their high signal-to-noise thermal Sunyaev-Zeldovich (tSZ) signal measured with the Atacama Cosmology Telescope (ACT). For a sample of 9 ACT clusters with a tSZ signal-to-noise greater than five the average weak lensing mass is (4.8±0.8) ×1014 Mo, consistent with the tSZ mass estimate of (4.70±1.0) ×1014 Mo which assumes a universal pressure profile for the cluster gas. Our results are consistent with previous weak-lensing measurements of tSZ-detected clusters from the Planck satellite. When comparing our results, we estimate the Eddington bias correction for the sample intersection of Planck and weak-lensing clusters which was previously excluded.",

author = "Battaglia and A. Leauthaud and H. Miyatake and M. Hasselfield and Gralla, {M. B.} and R. Allison and Bond, {J. R.} and E. Calabrese and D. Crichton and Devlin, {M. J.} and J. Dunkley and R. D{\"u}nner and T. Erben and S. Ferrara and M. Halpern and M. Hilton and Hill, {J. C.} and Hincks, {A. D.} and R. Hlo{\v z}ek and Huffenberger, {K. M.} and Hughes, {J. P.} and Kneib, {J. P.} and A. Kosowsky and M. Makler and Marriage, {T. A.} and F. Menanteau and L. Miller and K. Moodley and B. Moraes and Niemack, {M. D.} and L. Page and H. Shan and N. Sehgal and Sherwin, {B. D.} and Sievers, {J. L.} and C. Sif{\'o}n and Spergel, {D. N.} and Staggs, {S. T.} and Taylor, {J. E.} and R. Thornton and Waerbeke, {L. Van} and Wollack, {E. J.}",

note = "Publisher Copyright: {\textcopyright} 2016 IOP Publishing Ltd and Sissa Medialab srl .",

year = "2016",

month = aug,

day = "8",

doi = "10.1088/1475-7516/2016/08/013",

language = "English (US)",

volume = "2016",

journal = "Journal of Cosmology and Astroparticle Physics",

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Battaglia, Leauthaud, A, Miyatake, H, Hasselfield, M, Gralla, MB, Allison, R, Bond, JR, Calabrese, E, Crichton, D, Devlin, MJ, Dunkley, J, Dünner, R, Erben, T, Ferrara, S, Halpern, M, Hilton, M, Hill, JC, Hincks, AD, Hložek, R, Huffenberger, KM, Hughes, JP, Kneib, JP, Kosowsky, A, Makler, M, Marriage, TA, Menanteau, F, Miller, L, Moodley, K, Moraes, B, Niemack, MD, Page, L, Shan, H, Sehgal, N, Sherwin, BD, Sievers, JL, Sifón, C, Spergel, DN, Staggs, ST, Taylor, JE, Thornton, R, Waerbeke, LV & Wollack, EJ 2016, 'Weak-lensing mass calibration of the Atacama Cosmology Telescope equatorial Sunyaev-Zeldovich cluster sample with the Canada-France-Hawaii telescope stripe 82 survey', Journal of Cosmology and Astroparticle Physics, vol. 2016, no. 8, 013. https://doi.org/10.1088/1475-7516/2016/08/013

Weak-lensing mass calibration of the Atacama Cosmology Telescope equatorial Sunyaev-Zeldovich cluster sample with the Canada-France-Hawaii telescope stripe 82 survey. / Battaglia; Leauthaud, A.; Miyatake, H. et al.
In: Journal of Cosmology and Astroparticle Physics, Vol. 2016, No. 8, 013, 08.08.2016.

Research output: Contribution to journal › Review article › peer-review

TY - JOUR

T1 - Weak-lensing mass calibration of the Atacama Cosmology Telescope equatorial Sunyaev-Zeldovich cluster sample with the Canada-France-Hawaii telescope stripe 82 survey

AU - Battaglia,

AU - Leauthaud, A.

AU - Miyatake, H.

AU - Hasselfield, M.

AU - Gralla, M. B.

AU - Allison, R.

AU - Bond, J. R.

AU - Calabrese, E.

AU - Crichton, D.

AU - Devlin, M. J.

AU - Dunkley, J.

AU - Dünner, R.

AU - Erben, T.

AU - Ferrara, S.

AU - Halpern, M.

AU - Hilton, M.

AU - Hill, J. C.

AU - Hincks, A. D.

AU - Hložek, R.

AU - Huffenberger, K. M.

AU - Hughes, J. P.

AU - Kneib, J. P.

AU - Kosowsky, A.

AU - Makler, M.

AU - Marriage, T. A.

AU - Menanteau, F.

AU - Miller, L.

AU - Moodley, K.

AU - Moraes, B.

AU - Niemack, M. D.

AU - Page, L.

AU - Shan, H.

AU - Sehgal, N.

AU - Sherwin, B. D.

AU - Sievers, J. L.

AU - Sifón, C.

AU - Spergel, D. N.

AU - Staggs, S. T.

AU - Taylor, J. E.

AU - Thornton, R.

AU - Waerbeke, L. Van

AU - Wollack, E. J.

PY - 2016/8/8

Y1 - 2016/8/8

N2 - Mass calibration uncertainty is the largest systematic effect for using clusters of galaxies to constrain cosmological parameters. We present weak lensing mass measurements from the Canada-France-Hawaii Telescope Stripe 82 Survey for galaxy clusters selected through their high signal-to-noise thermal Sunyaev-Zeldovich (tSZ) signal measured with the Atacama Cosmology Telescope (ACT). For a sample of 9 ACT clusters with a tSZ signal-to-noise greater than five the average weak lensing mass is (4.8±0.8) ×1014 Mo, consistent with the tSZ mass estimate of (4.70±1.0) ×1014 Mo which assumes a universal pressure profile for the cluster gas. Our results are consistent with previous weak-lensing measurements of tSZ-detected clusters from the Planck satellite. When comparing our results, we estimate the Eddington bias correction for the sample intersection of Planck and weak-lensing clusters which was previously excluded.

AB - Mass calibration uncertainty is the largest systematic effect for using clusters of galaxies to constrain cosmological parameters. We present weak lensing mass measurements from the Canada-France-Hawaii Telescope Stripe 82 Survey for galaxy clusters selected through their high signal-to-noise thermal Sunyaev-Zeldovich (tSZ) signal measured with the Atacama Cosmology Telescope (ACT). For a sample of 9 ACT clusters with a tSZ signal-to-noise greater than five the average weak lensing mass is (4.8±0.8) ×1014 Mo, consistent with the tSZ mass estimate of (4.70±1.0) ×1014 Mo which assumes a universal pressure profile for the cluster gas. Our results are consistent with previous weak-lensing measurements of tSZ-detected clusters from the Planck satellite. When comparing our results, we estimate the Eddington bias correction for the sample intersection of Planck and weak-lensing clusters which was previously excluded.

UR - http://www.scopus.com/inward/record.url?scp=84985930146&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84985930146&partnerID=8YFLogxK

U2 - 10.1088/1475-7516/2016/08/013

DO - 10.1088/1475-7516/2016/08/013

M3 - Review article

AN - SCOPUS:84985930146

SN - 1475-7516

VL - 2016

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

IS - 8

M1 - 013

ER -

Weak-lensing mass calibration of the Atacama Cosmology Telescope equatorial Sunyaev-Zeldovich cluster sample with the Canada-France-Hawaii telescope stripe 82 survey

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