Planets Across Space and Time (PAST). V. The evolution of hot Jupiters revealed by the age distribution of their host stars

Kavli Affiliate: Subo Dong | First 5 Authors: Di-Chang Chen, Ji-Wei Xie, Ji-Lin Zhou, Subo Dong, Jia-Yi Yang | Summary: The unexpected discovery of hot Jupiters challenged the classical theory of planet formation inspired by our solar system. Until now, the origin and evolution of hot Jupiters are still uncertain. Determining their age distribution and […]


Continue.. Planets Across Space and Time (PAST). V. The evolution of hot Jupiters revealed by the age distribution of their host stars

Updating the first CHIME/FRB catalog of fast radio bursts with baseband data

Kavli Affiliate: Kiyoshi W. Masui | First 5 Authors: The CHIME/FRB Collaboration, :, Mandana Amiri, Bridget C. Andersen, Shion Andrew | Summary: In 2021, a catalog of 536 fast radio bursts (FRBs) detected with the Canadian Hydrogen Intensity Mapping Experiment (CHIME) radio telescope was released by the CHIME/FRB Collaboration. This large collection of bursts, observed […]


Continue.. Updating the first CHIME/FRB catalog of fast radio bursts with baseband data

Reviving MeV-GeV Indirect Detection with Inelastic Dark Matter

Kavli Affiliate: Gordan Krnjaic | First 5 Authors: Asher Berlin, Gordan Krnjaic, Elena Pinetti, , | Summary: Thermal relic dark matter below $sim 10 text{GeV}$ is excluded by cosmic microwave background data if its annihilation to visible particles is unsuppressed near the epoch of recombination. Usual model-building measures to avoid this bound involve kinematically suppressing […]


Continue.. Reviving MeV-GeV Indirect Detection with Inelastic Dark Matter

Further Development of Event-Based Analysis of X-ray Polarization Data

Kavli Affiliate: Herman L. Marshall | First 5 Authors: Herman L. Marshall, , , , | Summary: An event-based maximum likelihood method for handling X-ray polarimetry data is extended to include the effects of background and nonuniform sampling of the possible position angle space. While nonuniform sampling in position angle space generally introduces cross terms […]


Continue.. Further Development of Event-Based Analysis of X-ray Polarization Data

Further Development of Event-Based Analysis of X-ray Polarization Data

Kavli Affiliate: Herman L. Marshall | First 5 Authors: Herman L. Marshall, , , , | Summary: An event-based maximum likelihood method for handling X-ray polarimetry data is extended to include the effects of background and nonuniform sampling of the possible position angle space. While nonuniform sampling in position angle space generally introduces cross terms […]


Continue.. Further Development of Event-Based Analysis of X-ray Polarization Data

Further Development of Event-Based Analysis of X-ray Polarization Data

Kavli Affiliate: Herman L. Marshall | First 5 Authors: Herman L. Marshall, , , , | Summary: An event-based maximum likelihood method for handling X-ray polarimetry data is extended to include the effects of background and nonuniform sampling of the possible position angle space. While nonuniform sampling in position angle space generally introduces cross terms […]


Continue.. Further Development of Event-Based Analysis of X-ray Polarization Data

Further Development of Event-Based Analysis of X-ray Polarization Data

Kavli Affiliate: Herman L. Marshall | First 5 Authors: Herman L. Marshall, , , , | Summary: An event-based maximum likelihood method for handling X-ray polarimetry data is extended to include the effects of background and nonuniform sampling of the possible position angle space. While nonuniform sampling in position angle space generally introduces cross terms […]


Continue.. Further Development of Event-Based Analysis of X-ray Polarization Data

Co-evolution and Nuclear Structure in the Dwarf Galaxy POX 52 Studied by Multi-wavelength Data From Radio to X-ray

Kavli Affiliate: Claudio Ricci | First 5 Authors: Taiki Kawamuro, Claudio Ricci, Satoshi Yamada, Hirofumi Noda, Ruancun Li | Summary: The nearby dwarf galaxy POX 52 at $z = 0.021$ hosts an active galactic nucleus (AGN) with a black-hole (BH) mass of $M_{rm BH} sim 10^{5-6} M_odot$ and an Eddington ratio of $sim$ 0.1-1. This […]


Continue.. Co-evolution and Nuclear Structure in the Dwarf Galaxy POX 52 Studied by Multi-wavelength Data From Radio to X-ray

Planets Across Space and Time (PAST) IV: The Occurrence and Architecture of Kepler Planetary Systems as a Function of Kinematic Age Revealed by the LAMOST-Gaia-Kepler Sample

Kavli Affiliate: Subo Dong | First 5 Authors: Jia-Yi Yang, Di-Chang Chen, Ji-Wei Xie, Ji-Lin Zhou, Subo Dong | Summary: One of the fundamental questions in astronomy is how planetary systems form and evolve. Measuring the planetary occurrence and architecture as a function of time directly addresses this question. In the fourth paper of the […]


Continue.. Planets Across Space and Time (PAST) IV: The Occurrence and Architecture of Kepler Planetary Systems as a Function of Kinematic Age Revealed by the LAMOST-Gaia-Kepler Sample

Quantum Parton Shower with Kinematics

Kavli Affiliate: Masahito Yamazaki | First 5 Authors: Christian W. Bauer, So Chigusa, Masahito Yamazaki, , | Summary: Parton showers which can efficiently incorporate quantum interference effects have been shown to be run efficiently on quantum computers. However, so far these quantum parton showers did not include the full kinematical information required to reconstruct an […]


Continue.. Quantum Parton Shower with Kinematics