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Paper Citation Record · LEDGER

Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 19 inbound Pith citation observations for arXiv:1507.02704.

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1507.02704 v3

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Observation cb3247ab-1ec9-44a1-a62c-c54042f55f29 · inbound

Planck 2018 results. VI. Cosmological parameters cites this paper.

Planck 2018 results. VI. Cosmological parameters Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 283

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CMB constraints on ultra-light primordial black holes with extended mass distributions cites this paper.

CMB constraints on ultra-light primordial black holes with extended mass distributions Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 43

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Cosmological searches for the neutrino mass scale and mass ordering cites this paper.

Cosmological searches for the neutrino mass scale and mass ordering Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 88

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Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy cites this paper.

Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 140

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Observation af08114b-563f-4c33-9120-b1bf0a1b5726 · inbound

Resolving Hubble Tension with Quintom Dark Energy Model cites this paper.

Resolving Hubble Tension with Quintom Dark Energy Model Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 69

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The Hubble Hunter's Guide cites this paper.

The Hubble Hunter's Guide Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 93

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Improving cosmological parameter estimation with the future 21 cm observation from SKA cites this paper.

Improving cosmological parameter estimation with the future 21 cm observation from SKA Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 2

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Oscillating scalar fields and the Hubble tension: a resolution with novel signatures cites this paper.

Oscillating scalar fields and the Hubble tension: a resolution with novel signatures Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 55

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Dark Neutrino interactions phase out the Hubble tension cites this paper.

Dark Neutrino interactions phase out the Hubble tension Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 68

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Reionization optical depth determination from Planck HFI data with ten percent accuracy cites this paper.

Reionization optical depth determination from Planck HFI data with ten percent accuracy Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 34

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Observation 031e4c7b-36c0-47f8-a0dc-ccf97a397da2 · inbound

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? cites this paper.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 20

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Modeling beam chromaticity for high-resolution CMB analyses cites this paper.

Modeling beam chromaticity for high-resolution CMB analyses Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 21

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Impact of reionization history on constraining primordial gravitational waves in future all-sky cosmic microwave background experiments cites this paper.

Impact of reionization history on constraining primordial gravitational waves in future all-sky cosmic microwave background experiments Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 81

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3-dimensional charged black holes in $f({Q})$ gravity cites this paper.

3-dimensional charged black holes in $f({Q})$ gravity Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 5

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Observation 9977a4e9-5b09-4f2e-949d-eb435da15375 · inbound

Direct Detection of Leptophobic Dark Matter with Electronic Collective Excitations cites this paper.

Direct Detection of Leptophobic Dark Matter with Electronic Collective Excitations Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 102

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All-sky modeling of Galactic emission at radio and microwave frequencies cites this paper.

All-sky modeling of Galactic emission at radio and microwave frequencies Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 106

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Detectors for CLASS-W2: The second 90 GHz telescope of the Cosmology Large Angular Scale Surveyor cites this paper.

Detectors for CLASS-W2: The second 90 GHz telescope of the Cosmology Large Angular Scale Surveyor Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 249

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S-PLUS Clusters And Large-scale Environments (SCALE): II. PZWav versus redMaPPer identification of eRosita groups cites this paper.

S-PLUS Clusters And Large-scale Environments (SCALE): II. PZWav versus redMaPPer identification of eRosita groups Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 193

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Unveiling the Vanishing Higgsino-Nucleon Scattering in the MSSM at Next-to-Leading Order cites this paper.

Unveiling the Vanishing Higgsino-Nucleon Scattering in the MSSM at Next-to-Leading Order Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 5

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