Transient Corotating Clumps Around Adolescent Low-Mass Stars From Four Years of TESS

Kavli Affiliate: Saul Rappaport | First 5 Authors: Luke G. Bouma, Rahul Jayaraman, Saul Rappaport, Luisa M. Rebull, Lynne A. Hillenbrand | Summary: Complex periodic variables (CPVs) are stars that exhibit highly structured and periodic optical light curves. Previous studies have indicated that these stars are typically disk-free pre-main-sequence M dwarfs with rotation periods ranging […]


Continue.. Transient Corotating Clumps Around Adolescent Low-Mass Stars From Four Years of TESS

Transient Corotating Clumps Around Adolescent Low-Mass Stars From Four Years of TESS

Kavli Affiliate: Saul Rappaport | First 5 Authors: Luke G. Bouma, Rahul Jayaraman, Saul Rappaport, Luisa M. Rebull, Lynne A. Hillenbrand | Summary: Complex periodic variables (CPVs) are stars that exhibit highly structured and periodic optical light curves. Previous studies have indicated that these stars are typically disk-free pre-main-sequence M dwarfs with rotation periods ranging […]


Continue.. Transient Corotating Clumps Around Adolescent Low-Mass Stars From Four Years of TESS

Recovering from Privacy-Preserving Masking with Large Language Models

Kavli Affiliate: Zeeshan Ahmed | First 5 Authors: Arpita Vats, Zhe Liu, Peng Su, Debjyoti Paul, Yingyi Ma | Summary: Model adaptation is crucial to handle the discrepancy between proxy training data and actual users data received. To effectively perform adaptation, textual data of users is typically stored on servers or their local devices, where […]


Continue.. Recovering from Privacy-Preserving Masking with Large Language Models

Recovering from Privacy-Preserving Masking with Large Language Models

Kavli Affiliate: Zeeshan Ahmed | First 5 Authors: Arpita Vats, Zhe Liu, Peng Su, Debjyoti Paul, Yingyi Ma | Summary: Model adaptation is crucial to handle the discrepancy between proxy training data and actual users data received. To effectively perform adaptation, textual data of users is typically stored on servers or their local devices, where […]


Continue.. Recovering from Privacy-Preserving Masking with Large Language Models

Hierarchical Conditional Semi-Paired Image-to-Image Translation For Multi-Task Image Defect Correction On Shopping Websites

Kavli Affiliate: Jia Liu | First 5 Authors: Moyan Li, Jinmiao Fu, Shaoyuan Xu, Huidong Liu, Jia Liu | Summary: On shopping websites, product images of low quality negatively affect customer experience. Although there are plenty of work in detecting images with different defects, few efforts have been dedicated to correct those defects at scale. […]


Continue.. Hierarchical Conditional Semi-Paired Image-to-Image Translation For Multi-Task Image Defect Correction On Shopping Websites

Low-Energy Supernovae Bounds on Sterile Neutrinos

Kavli Affiliate: Shunsaku Horiuchi | First 5 Authors: Garv Chauhan, Shunsaku Horiuchi, Patrick Huber, Ian M. Shoemaker, | Summary: Sterile neutrinos can be produced through mixing with active neutrinos in the hot and dense core of a core-collapse supernova (SN). The standard bounds on the active-sterile mixing ($sin^2 theta$) from SN arise from SN1987A energy-loss, […]


Continue.. Low-Energy Supernovae Bounds on Sterile Neutrinos

A rest-frame near-IR study of clumps in galaxies at $1<z<2$ using JWST/NIRCam: connection to galaxy bulges

Kavli Affiliate: Luis C. Ho | First 5 Authors: Boris S. Kalita, John D. Silverman, Emanuele Daddi, Connor Bottrell, Luis C. Ho | Summary: A key question in galaxy evolution has been the importance of the apparent `clumpiness’ of high redshift galaxies. Until now, this property has been primarily investigated in rest-frame UV, limiting our […]


Continue.. A rest-frame near-IR study of clumps in galaxies at $1<z<2$ using JWST/NIRCam: connection to galaxy bulges

A rest-frame near-IR study of clumps in galaxies at 1 < z < 2 using JWST/NIRCam: connection to galaxy bulges

Kavli Affiliate: Luis C. Ho | First 5 Authors: Boris S. Kalita, John D. Silverman, Emanuele Daddi, Connor Bottrell, Luis C. Ho | Summary: A key question in galaxy evolution has been the importance of the apparent `clumpiness’ of high redshift galaxies. Until now, this property has been primarily investigated in rest-frame UV, limiting our […]


Continue.. A rest-frame near-IR study of clumps in galaxies at 1 < z < 2 using JWST/NIRCam: connection to galaxy bulges

GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$

Kavli Affiliate: Roberto Maiolino | First 5 Authors: Eleonora Parlanti, Stefano Carniani, Hannah Übler, Giacomo Venturi, Francesco D’Eugenio | Summary: Dust-obscured galaxies are thought to represent an early evolutionary phase of massive galaxies in which the active galactic nucleus (AGN) is still deeply buried in significant amounts of dusty material and its emission is strongly […]


Continue.. GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$

GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$

Kavli Affiliate: Roberto Maiolino | First 5 Authors: Eleonora Parlanti, Stefano Carniani, Hannah Übler, Giacomo Venturi, Chiara Circosta | Summary: Dust-obscured galaxies are thought to represent an early evolutionary phase of massive galaxies in which the active galactic nucleus (AGN) is still deeply buried in significant amounts of dusty material and its emission is strongly […]


Continue.. GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$