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

Quantum Metrology for Gravitational Wave Astronomy

Kavli Affiliate: Nergis Mavalvala | First 5 Authors: Roman Schnabel, Nergis Mavalvala, David E. McClelland, Ping Koy Lam, | Summary: Einstein’s General Theory of Relativity predicts that accelerating mass distributions produce gravitational radiation, analogous to electromagnetic radiation from accelerating charges. These gravitational waves have not been directly detected to date, but are expected to open […]


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PICZL: Image-based Photometric Redshifts for AGN

Kavli Affiliate: Claudio Ricci | First 5 Authors: William Roster, Mara Salvato, Sven Krippendorf, Aman Saxena, Raphael Shirley | Summary: Computing photo-z for AGN is challenging, primarily due to the interplay of relative emissions associated with the SMBH and its host galaxy. SED fitting methods, effective in pencil-beam surveys, face limitations in all-sky surveys with […]


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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

Investigating Differences in the Palomar-Green Blazar Population Using Polarization

Kavli Affiliate: Luis C. Ho | First 5 Authors: Janhavi Baghel, P. Kharb, T. Hovatta, Luis C. Ho, C. Harrison | Summary: We present polarization images with the Karl G. Jansky Very Large Array (VLA) in A and B-array configurations at 6 GHz of 7 radio-loud (RL) quasars and 8 BL Lac objects belonging to […]


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Emergence of steady quantum transport in a superconducting processor

Kavli Affiliate: Ke Wang | First 5 Authors: Pengfei Zhang, Yu Gao, Xiansong Xu, Ning Wang, Hang Dong | Summary: Non-equilibrium quantum transport is crucial to technological advances ranging from nanoelectronics to thermal management. In essence, it deals with the coherent transfer of energy and (quasi-)particles through quantum channels between thermodynamic baths. A complete understanding […]


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Model Editing for LLMs4Code: How Far are We?

Kavli Affiliate: Jing Wang | First 5 Authors: Xiaopeng Li, Shangwen Wang, Shasha Li, Jun Ma, Jie Yu | Summary: Large Language Models for Code (LLMs4Code) have been found to exhibit outstanding performance in the software engineering domain, especially the remarkable performance in coding tasks. However, even the most advanced LLMs4Code can inevitably contain incorrect […]


Continue.. Model Editing for LLMs4Code: How Far are We?