Evidence of lensing of the cosmic microwave background by dark matter halos

Mathew Madhavacheril; Neelima Sehgal; Rupert Allison; Nick Battaglia; J. Richard Bond; Erminia Calabrese; Jerod Caligiuri; Kevin Coughlin; Devin Crichton; Rahul Datta; Mark J. Devlin; Joanna Dunkley; Rolando Dünner; Kevin Fogarty; Emily Grace; Amir Hajian; Matthew Hasselfield; J. Colin Hill; Matt Hilton; Adam D. Hincks; Renée Hlozek; John P. Hughes; Arthur Kosowsky; Thibaut Louis; Marius Lungu; Jeff McMahon; Kavilan Moodley; Charles Munson; Sigurd Naess; Federico Nati; Laura Newburgh; Michael D. Niemack; Lyman A. Page; Bruce Partridge; Benjamin Schmitt; Blake D. Sherwin; Jon Sievers; David N. Spergel; Suzanne T. Staggs; Robert Thornton; Alexander Van Engelen; Jonathan T. Ward; Edward J. Wollack

doi:10.1103/PhysRevLett.114.151302

Evidence of lensing of the cosmic microwave background by dark matter halos

Mathew Madhavacheril
, Neelima Sehgal
, Rupert Allison
, Nick Battaglia
, J. Richard Bond
, Erminia Calabrese
, Jerod Caligiuri
, Kevin Coughlin
, Devin Crichton
, Rahul Datta
, Mark J. Devlin
, Joanna Dunkley
, Rolando Dünner
, Kevin Fogarty
, Emily Grace
, Amir Hajian
, Matthew Hasselfield
, J. Colin Hill
, Matt Hilton
, Adam D. Hincks

Renée Hlozek, John P. Hughes, Arthur Kosowsky, Thibaut Louis, Marius Lungu, Jeff McMahon, Kavilan Moodley, Charles Munson, Sigurd Naess, Federico Nati, Laura Newburgh, Michael D. Niemack, Lyman A. Page, Bruce Partridge, Benjamin Schmitt, Blake D. Sherwin, Jon Sievers, David N. Spergel, Suzanne T. Staggs, Robert Thornton, Alexander Van Engelen, Jonathan T. Ward, Edward J. Wollack

Physics and Astronomy

Stony Brook University
University of Oxford
Carnegie Mellon University
University of Toronto
University of Pittsburgh
University of Michigan, Ann Arbor
Johns Hopkins University
University of Pennsylvania
Pontificia Universidad Católica de Chile
Princeton University
Columbia University
University of KwaZulu-Natal
University of British Columbia
Rutgers - The State University of New Jersey, New Brunswick
University of Rome La Sapienza
Cornell University
Haverford College
Lawrence Berkeley National Laboratory
West Chester University
NASA Goddard Space Flight Center

Research output: Contribution to journal › Article › peer-review

79 Scopus citations

Abstract

We present evidence of the gravitational lensing of the cosmic microwave background by 1013 solar mass dark matter halos. Lensing convergence maps from the Atacama Cosmology Telescope Polarimeter (ACTPol) are stacked at the positions of around 12000 optically selected CMASS galaxies from the SDSS-III/BOSS survey. The mean lensing signal is consistent with simulated dark matter halo profiles and is favored over a null signal at 3.2σ significance. This result demonstrates the potential of microwave background lensing to probe the dark matter distribution in galaxy group and galaxy cluster halos.

Original language	English
Article number	151302
Journal	Physical Review Letters
Volume	114
Issue number	15
DOIs	https://doi.org/10.1103/PhysRevLett.114.151302
State	Published - Apr 13 2015

Access to Document

10.1103/PhysRevLett.114.151302

Cite this

Madhavacheril, M., Sehgal, N., Allison, R., Battaglia, N., Bond, J. R., Calabrese, E., Caligiuri, J., Coughlin, K., Crichton, D., Datta, R., Devlin, M. J., Dunkley, J., Dünner, R., Fogarty, K., Grace, E., Hajian, A., Hasselfield, M., Hill, J. C., Hilton, M., ... Wollack, E. J. (2015). Evidence of lensing of the cosmic microwave background by dark matter halos. Physical Review Letters, 114(15), Article 151302. https://doi.org/10.1103/PhysRevLett.114.151302

@article{d302d5a0458743d4ab9d0b218447a19d,

title = "Evidence of lensing of the cosmic microwave background by dark matter halos",

abstract = "We present evidence of the gravitational lensing of the cosmic microwave background by 1013 solar mass dark matter halos. Lensing convergence maps from the Atacama Cosmology Telescope Polarimeter (ACTPol) are stacked at the positions of around 12000 optically selected CMASS galaxies from the SDSS-III/BOSS survey. The mean lensing signal is consistent with simulated dark matter halo profiles and is favored over a null signal at 3.2σ significance. This result demonstrates the potential of microwave background lensing to probe the dark matter distribution in galaxy group and galaxy cluster halos.",

author = "Mathew Madhavacheril and Neelima Sehgal and Rupert Allison and Nick Battaglia and Bond, \{J. Richard\} and Erminia Calabrese and Jerod Caligiuri and Kevin Coughlin and Devin Crichton and Rahul Datta and Devlin, \{Mark J.\} and Joanna Dunkley and Rolando D{\"u}nner and Kevin Fogarty and Emily Grace and Amir Hajian and Matthew Hasselfield and Hill, \{J. Colin\} and Matt Hilton and Hincks, \{Adam D.\} and Ren{\'e}e Hlozek and Hughes, \{John P.\} and Arthur Kosowsky and Thibaut Louis and Marius Lungu and Jeff McMahon and Kavilan Moodley and Charles Munson and Sigurd Naess and Federico Nati and Laura Newburgh and Niemack, \{Michael D.\} and Page, \{Lyman A.\} and Bruce Partridge and Benjamin Schmitt and Sherwin, \{Blake D.\} and Jon Sievers and Spergel, \{David N.\} and Staggs, \{Suzanne T.\} and Robert Thornton and \{Van Engelen\}, Alexander and Ward, \{Jonathan T.\} and Wollack, \{Edward J.\}",

note = "Publisher Copyright: {\textcopyright} 2015 American Physical Society.",

year = "2015",

month = apr,

day = "13",

doi = "10.1103/PhysRevLett.114.151302",

language = "English",

volume = "114",

journal = "Physical Review Letters",

issn = "0031-9007",

number = "15",

}

Madhavacheril, M, Sehgal, N, Allison, R, Battaglia, N, Bond, JR, Calabrese, E, Caligiuri, J, Coughlin, K, Crichton, D, Datta, R, Devlin, MJ, Dunkley, J, Dünner, R, Fogarty, K, Grace, E, Hajian, A, Hasselfield, M, Hill, JC, Hilton, M, Hincks, AD, Hlozek, R, Hughes, JP, Kosowsky, A, Louis, T, Lungu, M, McMahon, J, Moodley, K, Munson, C, Naess, S, Nati, F, Newburgh, L, Niemack, MD, Page, LA, Partridge, B, Schmitt, B, Sherwin, BD, Sievers, J, Spergel, DN, Staggs, ST, Thornton, R, Van Engelen, A, Ward, JT & Wollack, EJ 2015, 'Evidence of lensing of the cosmic microwave background by dark matter halos', Physical Review Letters, vol. 114, no. 15, 151302. https://doi.org/10.1103/PhysRevLett.114.151302

TY - JOUR

T1 - Evidence of lensing of the cosmic microwave background by dark matter halos

AU - Madhavacheril, Mathew

AU - Sehgal, Neelima

AU - Allison, Rupert

AU - Battaglia, Nick

AU - Bond, J. Richard

AU - Calabrese, Erminia

AU - Caligiuri, Jerod

AU - Coughlin, Kevin

AU - Crichton, Devin

AU - Datta, Rahul

AU - Devlin, Mark J.

AU - Dunkley, Joanna

AU - Dünner, Rolando

AU - Fogarty, Kevin

AU - Grace, Emily

AU - Hajian, Amir

AU - Hasselfield, Matthew

AU - Hill, J. Colin

AU - Hilton, Matt

AU - Hincks, Adam D.

AU - Hlozek, Renée

AU - Hughes, John P.

AU - Kosowsky, Arthur

AU - Louis, Thibaut

AU - Lungu, Marius

AU - McMahon, Jeff

AU - Moodley, Kavilan

AU - Munson, Charles

AU - Naess, Sigurd

AU - Nati, Federico

AU - Newburgh, Laura

AU - Niemack, Michael D.

AU - Page, Lyman A.

AU - Partridge, Bruce

AU - Schmitt, Benjamin

AU - Sherwin, Blake D.

AU - Sievers, Jon

AU - Spergel, David N.

AU - Staggs, Suzanne T.

AU - Thornton, Robert

AU - Van Engelen, Alexander

AU - Ward, Jonathan T.

AU - Wollack, Edward J.

PY - 2015/4/13

Y1 - 2015/4/13

N2 - We present evidence of the gravitational lensing of the cosmic microwave background by 1013 solar mass dark matter halos. Lensing convergence maps from the Atacama Cosmology Telescope Polarimeter (ACTPol) are stacked at the positions of around 12000 optically selected CMASS galaxies from the SDSS-III/BOSS survey. The mean lensing signal is consistent with simulated dark matter halo profiles and is favored over a null signal at 3.2σ significance. This result demonstrates the potential of microwave background lensing to probe the dark matter distribution in galaxy group and galaxy cluster halos.

AB - We present evidence of the gravitational lensing of the cosmic microwave background by 1013 solar mass dark matter halos. Lensing convergence maps from the Atacama Cosmology Telescope Polarimeter (ACTPol) are stacked at the positions of around 12000 optically selected CMASS galaxies from the SDSS-III/BOSS survey. The mean lensing signal is consistent with simulated dark matter halo profiles and is favored over a null signal at 3.2σ significance. This result demonstrates the potential of microwave background lensing to probe the dark matter distribution in galaxy group and galaxy cluster halos.

UR - https://www.scopus.com/pages/publications/84929587483

U2 - 10.1103/PhysRevLett.114.151302

DO - 10.1103/PhysRevLett.114.151302

M3 - Article

AN - SCOPUS:84929587483

SN - 0031-9007

VL - 114

JO - Physical Review Letters

JF - Physical Review Letters

IS - 15

M1 - 151302

ER -

Evidence of lensing of the cosmic microwave background by dark matter halos

Abstract

Access to Document

Other files and links

Fingerprint

Cite this