Masses of Sunyaev-Zel’dovich Galaxy Clusters Detected by The Atacama Cosmology Telescope: Stacked Lensing Measurements with Subaru HSC Year 3 data

Kavli Affiliate: David Spergel | First 5 Authors: Masato Shirasaki, Cristóbal Sifón, Hironao Miyatake, Erwin Lau, Zhuowen Zhang | Summary: We present a stacked lensing analysis of 96 galaxy clusters selected by the thermal Sunyaev-Zel’dovich (SZ) effect in maps of the cosmic microwave background (CMB). We select foreground galaxy clusters with a $5sigma$-level SZ threshold […]


Continue.. Masses of Sunyaev-Zel’dovich Galaxy Clusters Detected by The Atacama Cosmology Telescope: Stacked Lensing Measurements with Subaru HSC Year 3 data

Across the soft gamma-ray regime: utilizing simultaneous detections in the Compton Spectrometer and Imager (COSI) and the Background and Transient Observer (BTO) to understand astrophysical transients

Kavli Affiliate: Tadayuki Takahashi | First 5 Authors: Hannah C. Gulick, Eliza Neights, Samer Al Nussirat, Claire Tianyi Chen, Kaylie Ching | Summary: The Compton Spectrometer and Imager (COSI) is a NASA funded Small Explorer (SMEX) mission slated to launch in 2027. COSI will house a wide-field gamma-ray telescope designed to survey the entire sky […]


Continue.. Across the soft gamma-ray regime: utilizing simultaneous detections in the Compton Spectrometer and Imager (COSI) and the Background and Transient Observer (BTO) to understand astrophysical transients

Across the soft gamma-ray regime: utilizing simultaneous detections in the Compton Spectrometer and Imager (COSI) and the Background and Transient Observer (BTO) to understand astrophysical transients

Kavli Affiliate: Tadayuki Takahashi | First 5 Authors: Hannah C. Gulick, Eliza Neights, Samer Al Nussirat, Claire Tianyi Chen, Kaylie Ching | Summary: The Compton Spectrometer and Imager (COSI) is a NASA funded Small Explorer (SMEX) mission slated to launch in 2027. COSI will house a wide-field gamma-ray telescope designed to survey the entire sky […]


Continue.. Across the soft gamma-ray regime: utilizing simultaneous detections in the Compton Spectrometer and Imager (COSI) and the Background and Transient Observer (BTO) to understand astrophysical transients

Revisiting the Ultraviolet Tail of the Primordial Gravitational Wave

Kavli Affiliate: Misao Sasaki | First 5 Authors: Shi Pi, Misao Sasaki, Ao Wang, Jianing Wang, | Summary: High-frequency primordial gravitational waves (PGWs) with wave numbers larger than the Hubble parameter at the end of inflation are originated from the ultraviolet (UV) modes, which are never stretched out of the horizon. Such a UV tail […]


Continue.. Revisiting the Ultraviolet Tail of the Primordial Gravitational Wave

Revisiting for maximal flavor violating $Z^{‘}_{eμ}$ and its phenomenology constraints

Kavli Affiliate: Jia Liu | First 5 Authors: Jia Liu, Muyuan Song, Haohao Zhang, , | Summary: Lepton flavor violation (LFV), observed conclusively in neutrino oscillations, remains a pivotal area of investigation due to its absence in the Standard Model (SM). Beyond the Standard Model (BSM) physics explores charged lepton flavor violation (CLFV), particularly through […]


Continue.. Revisiting for maximal flavor violating $Z^{‘}_{eμ}$ and its phenomenology constraints

Revisiting for maximal flavor violating $Z^{‘}_{eμ}$ and its phenomenology constraints

Kavli Affiliate: Jia Liu | First 5 Authors: Jia Liu, Muyuan Song, Haohao Zhang, , | Summary: Lepton flavor violation (LFV), observed conclusively in neutrino oscillations, remains a pivotal area of investigation due to its absence in the Standard Model (SM). Beyond the Standard Model (BSM) physics explores charged lepton flavor violation (CLFV), particularly through […]


Continue.. Revisiting for maximal flavor violating $Z^{‘}_{eμ}$ and its phenomenology constraints

Ada-adapter:Fast Few-shot Style Personlization of Diffusion Model with Pre-trained Image Encoder

Kavli Affiliate: Jia Liu | First 5 Authors: Jia Liu, Changlin Li, Qirui Sun, Jiahui Ming, Chen Fang | Summary: Fine-tuning advanced diffusion models for high-quality image stylization usually requires large training datasets and substantial computational resources, hindering their practical applicability. We propose Ada-Adapter, a novel framework for few-shot style personalization of diffusion models. Ada-Adapter […]


Continue.. Ada-adapter:Fast Few-shot Style Personlization of Diffusion Model with Pre-trained Image Encoder

Search for the baryon number and lepton number violating decays $τ^-to Λπ^-$ and $τ^-to barΛπ^-$ at Belle II

Kavli Affiliate: T. Higuchi | First 5 Authors: Belle II Collaboration, I. Adachi, L. Aggarwal, H. Ahmed, H. Aihara | Summary: We present a search for the baryon number $B$ and lepton number $L$ violating decays $tau^- rightarrow Lambda pi^-$ and $tau^- rightarrow bar{Lambda} pi^-$ produced from the $e^+e^-to tau^+tau^-$ process, using a 364 fb$^{-1}$ […]


Continue.. Search for the baryon number and lepton number violating decays $τ^-to Λπ^-$ and $τ^-to barΛπ^-$ at Belle II

Measurement of the integrated luminosity of data samples collected during 2019-2022 by the Belle II experiment

Kavli Affiliate: T. Higuchi | First 5 Authors: The Belle II Collaboration, I. Adachi, L. Aggarwal, H. Ahmed, J. K. Ahn | Summary: A series of data samples was collected with the Belle II detector at the SuperKEKB collider from March 2019 to June 2022. We determine the integrated luminosities of these data samples using […]


Continue.. Measurement of the integrated luminosity of data samples collected during 2019-2022 by the Belle II experiment

Measurement of the integrated luminosity of data samples collected during 2019-2022 by the Belle II experiment

Kavli Affiliate: T. Higuchi | First 5 Authors: The Belle II Collaboration, I. Adachi, L. Aggarwal, H. Ahmed, J. K. Ahn | Summary: A series of data samples was collected with the Belle~II detector at the SuperKEKB collider from March 2019 to June 2022. We determine the integrated luminosities of these data samples using three […]


Continue.. Measurement of the integrated luminosity of data samples collected during 2019-2022 by the Belle II experiment