Skip to content
DraconiticResearch
Search Sources API
194,230 studies31 sourcesUpdated 21 min ago
PreprintarXiv licencearXiv

CMB Lensing Reconstruction Using Two Years of Temperature Data from the SPT-3G Summer Survey

82 more authors

60 listed; 94 in total.

Abstract

We present the first reconstruction of the cosmic microwave background (CMB) lensing potential from the SPT-3G Summer survey using two years of temperature data. The Summer survey has a total area of approximately 2640 deg2, split into three fields covering 1210, 570, and 860 deg2, respectively. A joint analysis of the three Summer fields yields a lensing amplitude of Acomb = 1.014 ± 0.053 relative to a fiducial Planck 2018 ΛCDM cosmology for the multipole range 50 < L < 2000. These early results from the SPT-3G Summer survey highlight the potential for increasing the signal-to-noise ratio when combining the Summer fields with the SPT-3G Main and Wide fields for a total SPT-3G survey area of ∼ 10,000 deg2.

Related

  1. De-lensing cosmic birefringence with joint reconstruction
    Sebastian Belkner, Julien Carron
    arXivPreprintarXiv licenceFull textCosmologyarXiv
  2. An empirically constrained Covariant Modified Gravity: exact reconstruction of galactic rotation curves and lensing
    Xavier Hérnandez, Sergio Mendoza, Sarahí Silva +1
    arXivPreprintCC BY 4.0Full textCosmologyarXiv
  3. Dark Energy Survey year 6 results: Cosmological constraints from galaxy clustering and weak lensing
    T. M. C. Abbott, T. M. C. Abbott, M. Aguena +97
    Physical review. D/Physical review. D.Peer-reviewedLicence not statedFull text101 citedCosmologyOpenAlex
  4. Finding the distribution of matter using lenses - I: deconvolution-based reconstruction with CMB lensing
    Ajoy Dawn, Jun-Qian Jiang, Dhiraj Kumar Hazra +2
    arXivPreprintarXiv licenceFull textCosmologyComputational physicsarXiv
  5. The BUFFALO Survey : The Subhalo Mass Function for Abell 2744 with Strong+Weak Gravitational Lensing
    Nency R Patel, Mathilde Jauzac, Anna Niemiec +16
    Mon.Not.Roy.Astron.Soc.Peer-reviewedCC BY 4.0Full textCosmologyGeneral physicsHALarXiv
BibTeX
@misc{levy2026lensing,
  title = {{CMB Lensing Reconstruction Using Two Years of Temperature Data from the SPT-3G Summer Survey}},
  author = {K. Levy and S. Raghunathan and F. Guidi and Y. Li and E. Anderes and A. J. Anderson and B. Ansarinejad and M. Archipley and L. Balkenhol and D. R. Barron and K. Benabed and A. N. Bender and B. A. Benson and F. Bianchini and L. E. Bleem and S. Bocquet and F. R. Bouchet and E. Camphuis and M. G. Campitiello and J. E. Carlstrom and J. Carron and C. L. Chang and P. M. Chichura and A. Chokshi and T. -L. Chou and A. Coerver and T. M. Crawford and C. Daley and T. de Haan and K. R. Dibert and M. A. Dobbs and M. Doohan and D. Dutcher and C. Feng and K. R. Ferguson and N. C. Ferree and K. Fichman and A. Foster and S. Galli and A. E. Gambrel and A. K. Gao and F. Ge and S. Guns and N. W. Halverson and E. Hivon and G. P. Holder and W. L. Holzapfel and J. C. Hood and A. Hryciuk and N. Huang and T. Jhaveri and F. Kéruzoré and A. R. Khalife and L. Knox and K. Kornoelje and C. -L. Kuo and A. E. Lowitz and C. Lu and G. P. Lynch and T. J. Maccarone},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2607.05784},
  eprint = {2607.05784},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2607.05784},
}
RIS
TY  - UNPB
TI  - CMB Lensing Reconstruction Using Two Years of Temperature Data from the SPT-3G Summer Survey
AU  - K. Levy
AU  - S. Raghunathan
AU  - F. Guidi
AU  - Y. Li
AU  - E. Anderes
AU  - A. J. Anderson
AU  - B. Ansarinejad
AU  - M. Archipley
AU  - L. Balkenhol
AU  - D. R. Barron
AU  - K. Benabed
AU  - A. N. Bender
AU  - B. A. Benson
AU  - F. Bianchini
AU  - L. E. Bleem
AU  - S. Bocquet
AU  - F. R. Bouchet
AU  - E. Camphuis
AU  - M. G. Campitiello
AU  - J. E. Carlstrom
AU  - J. Carron
AU  - C. L. Chang
AU  - P. M. Chichura
AU  - A. Chokshi
AU  - T. -L. Chou
AU  - A. Coerver
AU  - T. M. Crawford
AU  - C. Daley
AU  - T. de Haan
AU  - K. R. Dibert
AU  - M. A. Dobbs
AU  - M. Doohan
AU  - D. Dutcher
AU  - C. Feng
AU  - K. R. Ferguson
AU  - N. C. Ferree
AU  - K. Fichman
AU  - A. Foster
AU  - S. Galli
AU  - A. E. Gambrel
AU  - A. K. Gao
AU  - F. Ge
AU  - S. Guns
AU  - N. W. Halverson
AU  - E. Hivon
AU  - G. P. Holder
AU  - W. L. Holzapfel
AU  - J. C. Hood
AU  - A. Hryciuk
AU  - N. Huang
AU  - T. Jhaveri
AU  - F. Kéruzoré
AU  - A. R. Khalife
AU  - L. Knox
AU  - K. Kornoelje
AU  - C. -L. Kuo
AU  - A. E. Lowitz
AU  - C. Lu
AU  - G. P. Lynch
AU  - T. J. Maccarone
PY  - 2026
DA  - 2026/10/31
PB  - arXiv
DO  - 10.48550/arxiv.2607.05784
UR  - https://arxiv.org/abs/2607.05784
AB  - We present the first reconstruction of the cosmic microwave background (CMB) lensing potential from the SPT-3G Summer survey using two years of temperature data. The Summer survey has a total area of approximately 2640 deg^2, split into three fields covering 1210, 570, and 860 deg^2, respectively. A joint analysis of the three Summer fields yields a lensing amplitude of A^comb = 1.014 ± 0.053 relative to a fiducial Planck 2018 ΛCDM cosmology for the multipole range 50 < L < 2000. These early results from the SPT-3G Summer survey highlight the potential for increasing the signal-to-noise ratio when combining the Summer fields with the SPT-3G Main and Wide fields for a total SPT-3G survey area of ∼ 10,000 deg^2.
ER  -