The DOI matches its Crossref record; 32 of the 32 references it cites were found in a registry or an index.
SPT-3G: a next-generation cosmic microwave background polarization experiment on the South Pole telescope
Open accessAbstract
We describe the design of a new polarization sensitive receiver, spt-3g, for the 10-meter South Pole Telescope (spt). The spt-3g receiver will deliver a factor of ~20 improvement in mapping speed over the current receiver, spt-pol. The sensitivity of the spt-3g receiver will enable the advance from statistical detection of B-mode polarization anisotropy power to high signal-to-noise measurements of the individual modes, i.e., maps. This will lead to precise (~0.06 eV) constraints on the sum of neutrino masses with the potential to directly address the neutrino mass hierarchy. It will allow a separation of the lensing and inflationary B-mode power spectra, improving constraints on the amplitude and shape of the primordial signal, either through spt-3g data alone or in combination with bicep2/keck, which is observing the same area of sky. The measurement of small-scale temperature anisotropy will provide new constraints on the epoch of reionization. Additional science from the spt-3g survey will be significantly enhanced by the synergy with the ongoing optical Dark Energy Survey (des), including: a 1% constraint on the bias of optical tracers of large-scale structure, a measurement of the differential Doppler signal from pairs of galaxy clusters that will test General Relativity on ~200Mpc scales, and improved cosmological constraints from the abundance of clusters of galaxies
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Detection ofB-Mode Polarization at Degree Angular Scales by BICEP2
Ade, P. A. R., Aikin, R. W., Barkats, D., Benton, S. J., Bischoff, C. A., Bock, J. J., Brevik, J. A., Buder, I., Bullock, E., Dowell, C. D., et al. (2014) · Physical Review Letters · doi:10.1103/physrevlett.112.241101 · Cited by 1,571
Self-citationThe 10 Meter South Pole Telescope
Carlstrom, J. E., Ade, P. A. R., Aird, K. A., Benson, B. A., Bleem, L. E., Busetti, S., Chang, C. L., Chauvin, E., Cho, H.-M., Crawford, T. M., et al. (2011) · Publications of the Astronomical Society of the Pacific · doi:10.1086/659879 · Cited by 689
Self-citationKeisler, R., Reichardt, C. L., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H. M., Crawford, T. M., Crites, A. T., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/743/1/28 · Cited by 503
Self-citationPlanck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample
Planck Collaboration, Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Balbi, A., Banday, A. J., Barreiro, R. B., et al. (2011) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201116459 · Cited by 412
Self-citationStory, K. T., Reichardt, C. L., Hou, Z., Keisler, R., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H.-M., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/779/1/86 · Cited by 345
Self-citationHanson, D., Hoover, S., Crites, A., Ade, P. A. R., Aird, K. A., Austermann, J. E., Beall, J. A., Bender, A. N., Benson, B. A., Bleem, L. E., et al. (2013) · Physical Review Letters · doi:10.1103/physrevlett.111.141301 · Cited by 335
Self-citationVieira, J. D., Crawford, T. M., Switzer, E. R., Ade, P. A. R., Aird, K. A., Ashby, M. L. N., Benson, B. A., Bleem, L. E., Brodwin, M., Carlstrom, J. E., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/719/1/763 · Cited by 330
Self-citationVanderlinde, K., Crawford, T. M., de Haan, T., Dudley, J. P., Shaw, L., Ade, P. A. R., Aird, K. A., Benson, B. A., Bleem, L. E., Brodwin, M., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/722/2/1180 · Cited by 326
Self-citationDusty starburst galaxies in the early Universe as revealed by gravitational lensing
Vieira, J. D., Marrone, D. P., Chapman, S. C., De Breuck, C., Hezaveh, Y. D., Weiβ, A., Aguirre, J. E., Aird, K. A., Aravena, M., Ashby, M. L. N., et al. (2013) · Nature · doi:10.1038/nature12001 · Cited by 325
Self-citationGALAXY CLUSTERS DISCOVERED WITH A SUNYAEV-ZEL'DOVICH EFFECT SURVEY
Staniszewski, Z., Ade, P. A. R., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H.-M., Crawford, T. M., Crites, A. T., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/701/1/32 · Cited by 322
Self-citation
Cited by
Hubble constant hunter’s guide
Knox, L., & Millea, M. (2020) · Physical Review D · doi:10.1103/physrevd.101.043533 · Cited by 638
Self-citationDutcher, D., Balkenhol, L., Ade, P. A. R., Ahmed, Z., Anderes, E., Anderson, A. J., Archipley, M., Avva, J. S., Aylor, K., Barry, P. S., et al. (2021) · Physical Review D · doi:10.1103/physrevd.104.022003 · Cited by 249
Self-citationAtacama Cosmology Telescope: Constraints on prerecombination early dark energy
Hill, J. C., Calabrese, E., Aiola, S., Battaglia, N., Bolliet, B., Choi, S. K., Devlin, M. J., Duivenvoorden, A. J., Dunkley, J., Ferraro, S., et al. (2022) · Physical Review D · doi:10.1103/physrevd.105.123536 · Cited by 122
The Quantum Memory Matrix: A Unified Framework for the Black Hole Information Paradox
Neukart, F., Brasher, R., & Marx, E. (2024) · Entropy · doi:10.3390/e26121039 · Cited by 12
Metadata
- Authors
- Benson, B. A., Ade, P. A. R., Ahmed, Z., Allen, S. W., Arnold, K., Austermann, J. E., Bender, A. N., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H. M., Cliche, J. F., Crawford, T. M., Cukierman, A., de Haan, T., Dobbs, M. A., Dutcher, D., Everett, W., Gilbert, A., Halverson, N. W., Hanson, D., Harrington, N. L., Hattori, K., Henning, J. W., Hilton, G. C., Holder, G. P., Holzapfel, W. L., Irwin, K. D., Keisler, R., Knox, L., Kubik, D., Kuo, C. L., Lee, A. T., Leitch, E. M., Li, D., McDonald, M., Meyer, S. S., Montgomery, J., Myers, M., Natoli, T., Nguyen, H., Novosad, V., Padin, S., Pan, Z., Pearson, J., Reichardt, C., Ruhl, J. E., Saliwanchik, B. R., Simard, G., Smecher, G., Sayre, J. T., Shirokoff, E., Stark, A. A., Story, K., Suzuki, A., Thompson, K. L., Tucker, C., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Wang, G., Yefremenko, V., & Yoon, K. W.
- Venue
- SPIE Proceedings
- Publisher
- SPIE
- Published
- 2014-07-23
- Volume
- 9153
- Pages
- 91531P
- ISSN
- 0277-786X (ISSN-L)
- OpenAlex
- W2047332897
- Cited by
- 326
- References
- 32
- FWCI
- 81.13
- Type
- conference paper
- Language
- en
- Open access
- green
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: SPT-3G: a next-generation cosmic microwave background polarization experiment on the South Pole telescope. https://app.cochat.ai/papers/10.1117/12.2057305
- The paper
- Benson, B. A., Ade, P. A. R., Ahmed, Z., Allen, S. W., Arnold, K., Austermann, J. E., Bender, A. N., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H. M., Cliche, J. F., Crawford, T. M., Cukierman, A., de Haan, T., Dobbs, M. A., Dutcher, D., Everett, W., Gilbert, A., . . . Yoon, K. W. (2014). SPT-3G: a next-generation cosmic microwave background polarization experiment on the South Pole telescope. SPIE Proceedings. https://doi.org/10.1117/12.2057305
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
