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L. Balkenhol

Identifiers

  • name variant L. Balkenhol 0.60 · backfill

Papers (20)

  1. Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in 5 year data from the SPT-3G Main Survey astro-ph.CO · 2026 · author #12
  2. Cross-correlation of SPT-3G D1 CMB lensing and DES Y3 galaxy lensing astro-ph.CO · 2026 · author #7
  3. Millimeter-wave Detections of Symbiotic Stars in SPT and ACT Data astro-ph.SR · 2026 · author #7
  4. Characterization of the Polarization Beam Response of SPT-3G Using Point Sources astro-ph.CO · 2026 · author #6
  5. Inflation at the End of 2025: Constraints on $r$ and $n_s$ Using the Latest CMB and BAO Data astro-ph.CO · 2025 · author #1
  6. SPT-3G D1: Axion Early Dark Energy with CMB experiments and DESI astro-ph.CO · 2025 · author #2
  7. SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field astro-ph.CO · 2025 · author #3
  8. A Measurement of the CMB Temperature Power Spectrum and Constraints on Cosmology from the SPT-3G 2018 TT/TE/EE Data Set astro-ph.CO · 2022 · author #1
  9. A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES astro-ph.CO · 2022 · author #5
  10. Searching for axion-like time-dependent cosmic birefringence with data from SPT-3G astro-ph.CO · 2022 · author #7
  11. Asteroid Measurements at Millimeter Wavelengths with the South Pole Telescope astro-ph.EP · 2022 · author #11
  12. Improving cosmological constraints from galaxy cluster number counts with CMB-cluster-lensing data: Results from the SPT-SZ survey and forecasts for the future astro-ph.CO · 2021 · author #6
  13. The Parameter-Level Performance of Covariance Matrix Conditioning in Cosmic Microwave Background Data Analyses astro-ph.CO · 2021 · author #1
  14. The Design and Integrated Performance of SPT-3G astro-ph.IM · 2021 · author #18
  15. Performance and characterization of the SPT-3G digital frequency-domain multiplexed readout system using an improved noise and crosstalk model astro-ph.IM · 2021 · author #9
  16. Constraints on $\Lambda$CDM Extensions from the SPT-3G 2018 $EE$ and $TE$ Power Spectra astro-ph.CO · 2021 · author #1
  17. Detection of Galactic and Extragalactic Millimeter-Wavelength Transient Sources with SPT-3G astro-ph.HE · 2021 · author #13
  18. Measurements of the E-Mode Polarization and Temperature-E-Mode Correlation of the CMB from SPT-3G 2018 Data astro-ph.CO · 2021 · author #2
  19. Searching for Anisotropic Cosmic Birefringence with Polarization Data from SPTpol astro-ph.CO · 2020 · author #7
  20. Extreme Digitisation For Ground-Based Cosmic Microwave Background Experiments astro-ph.IM · 2018 · author #1

Mentions

  • 2212.05642 #1 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2207.11937 #5 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2202.01406 #11 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2203.16567 #7 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2111.07491 #6 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2110.03180 #1 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2106.11202 #18 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2103.16017 #9 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2103.13618 #1 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2103.06166 #13 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2101.01684 #2 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2006.08061 #7 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 1810.03789 #1 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2607.01175 #12 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2512.10613 #1 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2606.26223 #7 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2602.06334 #6 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2605.01022 #7 · arxiv_oai · confidence 0.70 L. Balkenhol
  • 2507.23355 #2 · arxiv_oai · confidence 0.70 L. Balkenhol

Frequent Coauthors