Tracing 3-D Magnetic Field Structure Using Dust Polarization and the Zeeman Effect

Kavli Affiliate: Susan E. Clark | First 5 Authors: Brandon Shane, Blakesley Burkhart, Laura Fissel, Susan E. Clark, Philip Mocz | Summary: The characterization of magnetic fields within molecular clouds is fundamental to understanding star formation processes. Accurately gauging the three-dimensional structure of these fields presents a challenge, as observational techniques such as dust polarization […]


Continue.. Tracing 3-D Magnetic Field Structure Using Dust Polarization and the Zeeman Effect

A halo model approach for mock catalogs of time-variable strong gravitational lenses

Kavli Affiliate: Philip J. Marshall | First 5 Authors: Katsuya T. Abe, Masamune Oguri, Simon Birrer, Narayan Khadka, Philip J. Marshall | Summary: Time delays in both galaxy- and cluster-scale strong gravitational lenses have recently attracted a lot of attention in the context of the Hubble tension. Future wide-field cadenced surveys, such as the LSST, […]


Continue.. A halo model approach for mock catalogs of time-variable strong gravitational lenses

A halo model approach for mock catalogs of time-variable strong gravitational lenses

Kavli Affiliate: Philip J. Marshall | First 5 Authors: Katsuya T. Abe, Masamune Oguri, Simon Birrer, Narayan Khadka, Philip J. Marshall | Summary: Time delays in both galaxy- and cluster-scale strong gravitational lenses have recently attracted a lot of attention in the context of the Hubble tension. Future wide-field cadenced surveys, such as the LSST, […]


Continue.. A halo model approach for mock catalogs of time-variable strong gravitational lenses

A halo model approach for mock catalogs of time-variable strong gravitational lenses

Kavli Affiliate: Philip J. Marshall | First 5 Authors: Katsuya T. Abe, Masamune Oguri, Simon Birrer, Narayan Khadka, Philip J. Marshall | Summary: Time delays in both galaxy- and cluster-scale strong gravitational lenses have recently attracted a lot of attention in the context of the Hubble tension. Future wide-field cadenced surveys, such as the LSST, […]


Continue.. A halo model approach for mock catalogs of time-variable strong gravitational lenses

A halo model approach for mock catalogs of time-variable strong gravitational lenses

Kavli Affiliate: Philip J. Marshall | First 5 Authors: Katsuya T. Abe, Masamune Oguri, Simon Birrer, Narayan Khadka, Philip J. Marshall | Summary: Time delays in both galaxy- and cluster-scale strong gravitational lenses have recently attracted a lot of attention in the context of the Hubble tension. Future wide-field cadenced surveys, such as the LSST, […]


Continue.. A halo model approach for mock catalogs of time-variable strong gravitational lenses

Improved Receiver Noise Calibration for ADMX Axion Search: 4.54 to 5.41 $μ$eV

Kavli Affiliate: Chao-Lin Kuo | First 5 Authors: M. Guzzetti, D. Zhang, C. Goodman, C. Hanretty, J. Sinnis | Summary: Axions are a well-motivated candidate for dark matter. The preeminent method to search for axion dark matter is known as the axion haloscope, which makes use of the conversion of axions to photons in a […]


Continue.. Improved Receiver Noise Calibration for ADMX Axion Search: 4.54 to 5.41 $μ$eV

Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data

Kavli Affiliate: Chao-Lin Kuo | First 5 Authors: C. Bartram, C. Boutan, T. Braine, J. H. Buckley, T. J. Caligiure | Summary: From CMB polarization data alone we reconstruct the CMB lensing power spectrum, comparable in overall constraining power to previous temperature-based reconstructions, and an unlensed E-mode power spectrum. The observations, taken in 2019 and […]


Continue.. Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data

Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data

Kavli Affiliate: Chao-Lin Kuo | First 5 Authors: F. Ge, M. Millea, E. Camphuis, C. Daley, N. Huang | Summary: From CMB polarization data alone we reconstruct the CMB lensing power spectrum, comparable in overall constraining power to previous temperature-based reconstructions, and an unlensed E-mode power spectrum. The observations, taken in 2019 and 2020 with […]


Continue.. Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data