Paper Citation Record · LEDGER

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky

As of 17 August 2026, this Paper Citation Record lists 73 of 73 outbound references and 2 inbound Pith citation observations for arXiv:2510.24669.

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2510.24669 v3

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Outbound references

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This paper cites an unresolved cited work.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Unresolved cited work

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This paper cites Coadded covariance 17 C.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Coadded covariance 17 C

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This paper cites The comparison of the first two cases allows us to determine the impact of dividing the observed sky in 13 different regions, assuming the same noise levels in the two cases.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky The comparison of the first two cases allows us to determine the impact of dividing the observed sky in 13 different regions, assuming the same noise levels in the two cases

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This paper cites Planck 2018 results.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Planck 2018 results

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky M., Romaniello, M., Murakami, Y

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This paper cites A., Ade, P.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky A., Ade, P

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This paper cites We sample over 33 parameters in total, including the six cosmological parameters and the 27 nuisance parameters defined in Section IIID.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky We sample over 33 parameters in total, including the six cosmological parameters and the 27 nuisance parameters defined in Section IIID

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This paper cites Since Summer a and Summer b have comparable white noise levels asSummer c, we only show Summer c noise curves for comparison purposes with the Wide and Main fields.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Since Summer a and Summer b have comparable white noise levels asSummer c, we only show Summer c noise curves for comparison purposes with the Wide and Main fields

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This paper cites Cosmology from CMB lensing and delensed EE power spectra using 2019–2020 SPT-3G polarization data.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Cosmology from CMB lensing and delensed EE power spectra using 2019–2020 SPT-3G polarization data

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This paper cites SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field

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This paper cites The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky J., Barreiro, R

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky The BAO-CMB Tension and Implications for Inflation

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky A., Anderson, A

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This paper cites Testing the ΛCDM Cosmological Model with Forthcoming Mea- surements of the Cosmic Microwave Background with SPT-3G.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Testing the ΛCDM Cosmological Model with Forthcoming Mea- surements of the Cosmic Microwave Background with SPT-3G

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky For our forecasts, we adopt the same nuisance parameters as assumed in [24] (see Table VIII from that work)

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky The computation correctly accounts for the mode coupling introduced by the apodized footprint masks

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky R., Zanjani, M

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky E., Ade, P

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Constraints on Inflationary Gravitational Waves with Two Years of SPT-3G Data

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky M., Hivon, E., Banday, A

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky J., Leary, C., Maclaurin, D., Necula, G., Paszke, A., VanderPlas, J., Wanderman-Milne, S., &Zhang, Q.2018, JAX: composable transformations of Python+NumPy programs, 0.3.13

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky candl: cosmic microwave background analysis with a differentiable likelihood

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky CosmoPower-JAX: high-dimensional Bayesian inference with differentiable cosmological emulators

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Measurement of the CMB temperature power spectrum and constraints on cosmology from the SPT-3G 2018 T T , T E , and E E dataset

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Accurate cosmic microwave background covariance 20 matrices: Exact calculation and approximations

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Disconnected pseudo-Cl covariances for projected large-scale structure data

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky M., Netterfield, C

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Fast estimation of polarization power spectra using correlation functions

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Super-sample CMB lensing

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Planck 2018 results

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky GetDist: a Python package for analysing Monte Carlo samples

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Varying Constants, Gravitation and Cosmol- ogy

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Early recombination as a solution to the H0 tension

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Dark energy at early times, the Hubble parameter, and the string axiverse

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Marginal unbiased score expan- sion and application to CMB lensing

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky SPT-3G D1: Axion Early Dark Energy with CMB experiments and DESI

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky R., & Galli, S

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This paper cites Revising the Halofit Model for the Nonlinear Matter Power Spectrum.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Revising the Halofit Model for the Nonlinear Matter Power Spectrum

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky J., Peacock, J

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This paper cites L., Karwal, T., & Kamionkowski, M.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky L., Karwal, T., & Kamionkowski, M

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky L., Lucca, M., Poulin, V., Abellan, G

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Towards Early Dark Energy in string theory

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This paper cites G., & Scalisi, M.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky G., & Scalisi, M

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky L., Poulin, V., & Amin, M

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This paper cites L., Grin, D., Karwal, T., & Kamionkowski, M.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky L., Grin, D., Karwal, T., & Kamionkowski, M

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This paper cites L., Patil, S., Ade, P.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky L., Patil, S., Ade, P

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Unresolved cited work

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This paper cites Multiprobe cosmology from the abundance of SPT clusters and DES galaxy clustering and weak lensing.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Multiprobe cosmology from the abundance of SPT clusters and DES galaxy clustering and weak lensing

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This paper cites H., Staveley-Smith, L., Campbell, L., Parker, Q., Saunders, W., & Watson, F.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky H., Staveley-Smith, L., Campbell, L., Parker, Q., Saunders, W., & Watson, F

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This paper cites J., Samushia, L., Howlett, C., Percival, W.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky J., Samushia, L., Howlett, C., Percival, W

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This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

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This paper cites Completed SDSS- IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectro- scopic surveys at the Apache Point Observatory.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Completed SDSS- IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectro- scopic surveys at the Apache Point Observatory

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This paper cites G., Aguilar, J., Ahlen, S., et al.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky G., Aguilar, J., Ahlen, S., et al

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This paper cites M., Jones, D.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky M., Jones, D

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky The Pantheon+ Analysis: Cosmological Constraints

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky C., & Varoquaux, G

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Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky Unresolved cited work

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This paper cites healpy: equal area pixelization and spherical harmonics transforms for data on the sphereinPython.2019, JournalofOpenSourceSoftware, 4, 1298, doi:10.21105/joss.01298.

Towards constraining cosmological parameters with SPT-3G observations of 25% of the sky healpy: equal area pixelization and spherical harmonics transforms for data on the sphereinPython.2019, JournalofOpenSourceSoftware, 4, 1298, doi:10.21105/joss.01298

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