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Title: The Atacama Cosmology Telescope: a CMB lensing mass map over 2100 square degrees of sky and its cross-correlation with BOSS-CMASS galaxies

Abstract

In this work, we construct cosmic microwave background lensing mass maps using data from the 2014 and 2015 seasons of observations with the Atacama Cosmology Telescope (ACT). These maps cover 2100 square degrees of sky and overlap with a wide variety of optical surveys. The maps are signal dominated on large scales and have fidelity such that their correlation with the cosmic infrared background is clearly visible by eye. We also create lensing maps with thermal Sunyaev-Zel’dovich contamination removed using a novel cleaning procedure that only slightly degrades the lensing signal-to-noise ratio. The cross-spectrum between the cleaned lensing map and the BOSS CMASS galaxy sample is detected at 10σ significance, with an amplitude of A = 1.02 ± 0.10 relative to the Planck best-fitting Lambda cold dark matter cosmological model with fiducial linear galaxy bias. Our measurement lays the foundation for lensing cross-correlation science with current ACT data and beyond.

Authors:
ORCiD logo [1];  [2];  [3];  [4];  [5];  [6];  [6];  [7];  [8];  [5];  [9];  [10];  [11];  [12];  [6];  [13];  [14];  [15];  [16];  [4] more »;  [17];  [6];  [18];  [7];  [19];  [6];  [20];  [21];  [14];  [6];  [22];  [19];  [16];  [23];  [24];  [18];  [4];  [1];  [25];  [21];  [6];  [26];  [19];  [27];  [1];  [28];  [29];  [30];  [16];  [31];  [32];  [19];  [19];  [33];  [34] « less
  1. Center for Theoretical Cosmology, DAMTP, University of Cambridge, Cambridge CB3 0WA, UK
  2. Perimeter Institute, Centre for the Universe, Waterloo, ON N2L 2Y5, Canada;Department of Astrophysical Sciences, Princeton University, 4 Ivy Lane, Princeton, NJ 08544, USA
  3. Center for Theoretical Cosmology, DAMTP, University of Cambridge, Cambridge CB3 0WA, UK;Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 OHA, UK
  4. Center for Computational Astrophysics, Flatiron Institute, 162 5th Avenue, New York, NY 10010, USA
  5. Department of Astronomy, Cornell University, Ithaca, NY 14853 USA
  6. NIST Quantum Devices Group, 325 Broadway Mailcode 817.03, Boulder, CO 80305, USA
  7. Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St George Street, Toronto, ON M5S 3H8, Canada
  8. School of Physics and Astronomy, Cardiff University, The Parade, Cardiff CF24 3AA, UK
  9. Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA
  10. Department of Astrophysical Sciences, Princeton University, 4 Ivy Lane, Princeton, NJ 08544, USA;Joseph Henry Laboratories of Physics, Jadwin Hall, Princeton University, Princeton, NJ 08544, USA
  11. Instituto de Astrofísica and Centro de Astro-Ingeniería, Facultad de Física, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 7820436 Macul, Chile
  12. Physics Division, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA
  13. Department of Physics, Cornell University, Ithaca, NY 14853 USA
  14. Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260, USA
  15. Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T 1Z1, Canada
  16. Physics and Astronomy Department, Stony Brook University, Stony Brook, NY 11794, USA
  17. Center for Computational Astrophysics, Flatiron Institute, 162 5th Avenue, New York, NY 10010, USA;Department of Physics, Columbia University, 550 West 120th Street, New York, NY 10027, USA;School of Natural Sciences, Institute for Advanced Study, Princeton, NJ 08540, USA
  18. Astrophysics & Cosmology Research Unit, School of Mathematics, Statistics & Computer Science, University of KwaZulu-Natal, Westville Campus, Durban 4041, South Africa
  19. Joseph Henry Laboratories of Physics, Jadwin Hall, Princeton University, Princeton, NJ 08544, USA
  20. Department of Physics and Astronomy, Rutgers University, 136 Frelinghuysen Road, Piscataway, NJ 08854-8019 USA
  21. Department of Physics, Yale University, New Haven, CT 06520, USA
  22. CNRS/IN2P3, IJCLab, Université Paris-Saclay, F-91405 Orsay, France
  23. CNRS, Institut d’astrophysique spatiale, Université Paris-Saclay, F-91405 Orsay, France
  24. Kavli Institute for Cosmological Physics, University of Chicago, 5640 S. Ellis Ave., Chicago, IL 60637, USA;Department of Astronomy and Astrophysics, University of Chicago, 5640 S. Ellis Ave., Chicago, IL 60637, USA;Department of Physics, University of Chicago, Chicago, IL 60637, USA;Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA
  25. Department of Physics, University of Milano-Bicocca Piazza della Scienza 3, I-20126 Milano, Italy
  26. Department of Astronomy, Cornell University, Ithaca, NY 14853 USA;Department of Physics, Cornell University, Ithaca, NY 14853 USA
  27. Department of Physics and Astronomy, Haverford College, Haverford, PA 19041, USA
  28. Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK;Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 OHA, UK
  29. Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
  30. Harvard-Smithsonian Center for Astrophysics, Harvard University, 60 Garden St, Cambridge, MA 02138, USA
  31. Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla 4059, Valparaíso, Chile
  32. Department of Astrophysical Sciences, Princeton University, 4 Ivy Lane, Princeton, NJ 08544, USA;Center for Computational Astrophysics, Flatiron Institute, 162 5th Avenue, New York, NY 10010, USA
  33. School of Earth and Space Exploration and Department of Physics, Arizona State University, Tempe, AZ 85287, USA
  34. NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA
Publication Date:
Research Org.:
Stony Brook Univ., NY (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF)
Contributing Org.:
ACT Collaboration
OSTI Identifier:
2205341
Alternate Identifier(s):
OSTI ID: 1762204
Grant/Contract Number:  
SC0020441; AC02-05CH11231; AST-1440226; AST0965625; AST-0408698; PHY-1214379; PHY-0855887; NNX13AE56G; NNX14AB58G
Resource Type:
Accepted Manuscript
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Volume: 500; Journal Issue: 2; Journal ID: ISSN 0035-8711
Publisher:
Oxford University Press
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; weak gravitational lensing; cosmic background radiation; large-scale structure of universe; cosmology

Citation Formats

Darwish, Omar, Madhavacheril, Mathew S., Sherwin, Blake D., Aiola, Simone, Battaglia, Nicholas, Beall, James A., Becker, Daniel T., Bond, J. Richard, Calabrese, Erminia, Choi, Steve K., Devlin, Mark J., Dunkley, Jo, Dünner, Rolando, Ferraro, Simone, Fox, Anna E., Gallardo, Patricio A., Guan, Yilun, Halpern, Mark, Han, Dongwon, Hasselfield, Matthew, Hill, J. Colin, Hilton, Gene C., Hilton, Matt, Hincks, Adam D., Patty Ho, Shuay-Pwu, Hubmayr, J., Hughes, John P., Koopman, Brian J., Kosowsky, Arthur, Van Lanen, J., Louis, Thibaut, Lungu, Marius, MacInnis, Amanda, Maurin, Loïc, McMahon, Jeffrey, Moodley, Kavilan, Naess, Sigurd, Namikawa, Toshiya, Nati, Federico, Newburgh, Laura, Nibarger, John P., Niemack, Michael D., Page, Lyman A., Partridge, Bruce, Qu, Frank J., Robertson, Naomi, Schillaci, Alessandro, Schmitt, Benjamin, Sehgal, Neelima, Sifón, Cristóbal, Spergel, David N., Staggs, Suzanne, Storer, Emilie, van Engelen, Alexander, and Wollack, Edward J. The Atacama Cosmology Telescope: a CMB lensing mass map over 2100 square degrees of sky and its cross-correlation with BOSS-CMASS galaxies. United States: N. p., 2020. Web. doi:10.1093/mnras/staa3438.
Darwish, Omar, Madhavacheril, Mathew S., Sherwin, Blake D., Aiola, Simone, Battaglia, Nicholas, Beall, James A., Becker, Daniel T., Bond, J. Richard, Calabrese, Erminia, Choi, Steve K., Devlin, Mark J., Dunkley, Jo, Dünner, Rolando, Ferraro, Simone, Fox, Anna E., Gallardo, Patricio A., Guan, Yilun, Halpern, Mark, Han, Dongwon, Hasselfield, Matthew, Hill, J. Colin, Hilton, Gene C., Hilton, Matt, Hincks, Adam D., Patty Ho, Shuay-Pwu, Hubmayr, J., Hughes, John P., Koopman, Brian J., Kosowsky, Arthur, Van Lanen, J., Louis, Thibaut, Lungu, Marius, MacInnis, Amanda, Maurin, Loïc, McMahon, Jeffrey, Moodley, Kavilan, Naess, Sigurd, Namikawa, Toshiya, Nati, Federico, Newburgh, Laura, Nibarger, John P., Niemack, Michael D., Page, Lyman A., Partridge, Bruce, Qu, Frank J., Robertson, Naomi, Schillaci, Alessandro, Schmitt, Benjamin, Sehgal, Neelima, Sifón, Cristóbal, Spergel, David N., Staggs, Suzanne, Storer, Emilie, van Engelen, Alexander, & Wollack, Edward J. The Atacama Cosmology Telescope: a CMB lensing mass map over 2100 square degrees of sky and its cross-correlation with BOSS-CMASS galaxies. United States. https://doi.org/10.1093/mnras/staa3438
Darwish, Omar, Madhavacheril, Mathew S., Sherwin, Blake D., Aiola, Simone, Battaglia, Nicholas, Beall, James A., Becker, Daniel T., Bond, J. Richard, Calabrese, Erminia, Choi, Steve K., Devlin, Mark J., Dunkley, Jo, Dünner, Rolando, Ferraro, Simone, Fox, Anna E., Gallardo, Patricio A., Guan, Yilun, Halpern, Mark, Han, Dongwon, Hasselfield, Matthew, Hill, J. Colin, Hilton, Gene C., Hilton, Matt, Hincks, Adam D., Patty Ho, Shuay-Pwu, Hubmayr, J., Hughes, John P., Koopman, Brian J., Kosowsky, Arthur, Van Lanen, J., Louis, Thibaut, Lungu, Marius, MacInnis, Amanda, Maurin, Loïc, McMahon, Jeffrey, Moodley, Kavilan, Naess, Sigurd, Namikawa, Toshiya, Nati, Federico, Newburgh, Laura, Nibarger, John P., Niemack, Michael D., Page, Lyman A., Partridge, Bruce, Qu, Frank J., Robertson, Naomi, Schillaci, Alessandro, Schmitt, Benjamin, Sehgal, Neelima, Sifón, Cristóbal, Spergel, David N., Staggs, Suzanne, Storer, Emilie, van Engelen, Alexander, and Wollack, Edward J. Tue . "The Atacama Cosmology Telescope: a CMB lensing mass map over 2100 square degrees of sky and its cross-correlation with BOSS-CMASS galaxies". United States. https://doi.org/10.1093/mnras/staa3438. https://www.osti.gov/servlets/purl/2205341.
@article{osti_2205341,
title = {The Atacama Cosmology Telescope: a CMB lensing mass map over 2100 square degrees of sky and its cross-correlation with BOSS-CMASS galaxies},
author = {Darwish, Omar and Madhavacheril, Mathew S. and Sherwin, Blake D. and Aiola, Simone and Battaglia, Nicholas and Beall, James A. and Becker, Daniel T. and Bond, J. Richard and Calabrese, Erminia and Choi, Steve K. and Devlin, Mark J. and Dunkley, Jo and Dünner, Rolando and Ferraro, Simone and Fox, Anna E. and Gallardo, Patricio A. and Guan, Yilun and Halpern, Mark and Han, Dongwon and Hasselfield, Matthew and Hill, J. Colin and Hilton, Gene C. and Hilton, Matt and Hincks, Adam D. and Patty Ho, Shuay-Pwu and Hubmayr, J. and Hughes, John P. and Koopman, Brian J. and Kosowsky, Arthur and Van Lanen, J. and Louis, Thibaut and Lungu, Marius and MacInnis, Amanda and Maurin, Loïc and McMahon, Jeffrey and Moodley, Kavilan and Naess, Sigurd and Namikawa, Toshiya and Nati, Federico and Newburgh, Laura and Nibarger, John P. and Niemack, Michael D. and Page, Lyman A. and Partridge, Bruce and Qu, Frank J. and Robertson, Naomi and Schillaci, Alessandro and Schmitt, Benjamin and Sehgal, Neelima and Sifón, Cristóbal and Spergel, David N. and Staggs, Suzanne and Storer, Emilie and van Engelen, Alexander and Wollack, Edward J.},
abstractNote = {In this work, we construct cosmic microwave background lensing mass maps using data from the 2014 and 2015 seasons of observations with the Atacama Cosmology Telescope (ACT). These maps cover 2100 square degrees of sky and overlap with a wide variety of optical surveys. The maps are signal dominated on large scales and have fidelity such that their correlation with the cosmic infrared background is clearly visible by eye. We also create lensing maps with thermal Sunyaev-Zel’dovich contamination removed using a novel cleaning procedure that only slightly degrades the lensing signal-to-noise ratio. The cross-spectrum between the cleaned lensing map and the BOSS CMASS galaxy sample is detected at 10σ significance, with an amplitude of A = 1.02 ± 0.10 relative to the Planck best-fitting Lambda cold dark matter cosmological model with fiducial linear galaxy bias. Our measurement lays the foundation for lensing cross-correlation science with current ACT data and beyond.},
doi = {10.1093/mnras/staa3438},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 2,
volume = 500,
place = {United States},
year = {Tue Nov 10 00:00:00 EST 2020},
month = {Tue Nov 10 00:00:00 EST 2020}
}

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