Van der Waals pi Josephson junctions

Kavli Affiliate: Jie Shan | First 5 Authors: Kaifei Kang, Helmuth Berger, Kenji Watanabe, Takashi Taniguchi, Laszlo Forro | Summary: Proximity-induced superconductivity in a ferromagnet can induce Cooper pairs with a finite center-of-mass momentum. The resultant spatially modulated superconducting order parameter is able to stabilize Josephson junctions (JJs) with pi phase difference in superconductor-ferromagnet heterostructures […]


Continue.. Van der Waals pi Josephson junctions

Magnetic Spirals in Accretion Flows Originated from Misaligned Magnetic Field

Kavli Affiliate: Feng Yuan | First 5 Authors: Weixiao Wang, Miikka S. Väisälä, Hsien Shang, Ruben Krasnopolsky, Zhi-Yun Li | Summary: Misalignment between rotation and magnetic field has been suggested to be one type of physical mechanisms which can easen the effects of magnetic braking during collapse of cloud cores leading to formation of protostellar […]


Continue.. Magnetic Spirals in Accretion Flows Originated from Misaligned Magnetic Field

A Robust Hot Subdwarfs Identification Method Based on Deep Learning

Kavli Affiliate: Feng Wang | First 5 Authors: Lei Tan, Ying Mei, Zhicun Liu, Yangping Luo, Hui Deng | Summary: Hot subdwarf star is a particular type of star that is crucial for studying binary evolution and atmospheric diffusion processes. In recent years, identifying Hot subdwarfs by machine learning methods has become a hot topic, […]


Continue.. A Robust Hot Subdwarfs Identification Method Based on Deep Learning

Development and characterization of a fast and low noise readout for the next generation X-ray CCDs

Kavli Affiliate: Marshall Bautz | First 5 Authors: Tanmoy Chattopadhyay, Sven Herrmann, Peter Orel, R. Glenn Morris, Gregory Prigozhin | Summary: The broad energy response, low electronic read noise, and good energy resolution have made X-ray Charge-Coupled Devices (CCDs) an obvious choice for developing soft X-ray astronomical instruments over the last half century. They also […]


Continue.. Development and characterization of a fast and low noise readout for the next generation X-ray CCDs

Development and characterization of a fast and low noise readout for the next generation X-ray CCDs

Kavli Affiliate: Marshall Bautz | First 5 Authors: Tanmoy Chattopadhyay, Sven Herrmann, Peter Orel, R. Glenn Morris, Gregory Prigozhin | Summary: The broad energy response, low electronic read noise, and good energy resolution have made X-ray Charge-Coupled Devices (CCDs) an obvious choice for developing soft X-ray astronomical instruments over the last half century. They also […]


Continue.. Development and characterization of a fast and low noise readout for the next generation X-ray CCDs

Development and characterization of a fast and low noise readout for the next generation X-ray CCDs

Kavli Affiliate: Sven Herrmann | First 5 Authors: Tanmoy Chattopadhyay, Sven Herrmann, Peter Orel, R. Glenn Morris, Gregory Prigozhin | Summary: The broad energy response, low electronic read noise, and good energy resolution have made X-ray Charge-Coupled Devices (CCDs) an obvious choice for developing soft X-ray astronomical instruments over the last half century. They also […]


Continue.. Development and characterization of a fast and low noise readout for the next generation X-ray CCDs

Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Jubee Sohn, Margaret J. Geller, Mark Vogelsberger, Ivana Damjanov, | Summary: We use the IllustrisTNG simulations to explore the dynamic scaling relation between massive clusters and their central galaxies (BCGs). The Illustris TNG300-1 simulation we use includes 280 massive clusters with $M_{200} > 10^{14}$ M$_{odot}$ enabling a […]


Continue.. Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG

Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in Illustris-TNG

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Jubee Sohn, Margaret J. Geller, Mark Vogelsberger, Ivana Danjanov, | Summary: We use the Illustris-TNG simulations to explore the dynamic scaling relation between massive clusters and their central galaxies (BCGs). The Illustris TNG300-1 simulation we use includes 280 massive clusters with $M_{200} > 10^{14}$ M$_{odot}$ enabling a […]


Continue.. Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in Illustris-TNG

The Origin of the Relation Between Stellar Angular Momentum and Stellar Mass in Nearby Disk-dominated galaxies

Kavli Affiliate: Luis C. Ho | First 5 Authors: Min Du, Luis C. Ho, Hao-Ran Yu, Victor P. Debattista, | Summary: The IllustrisTNG simulations reproduce the observed scaling relation between stellar specific angular momentum (sAM) $j_{rm s}$ and mass $M_{rm s}$ of central galaxies. We show that the local $j_{rm s}$-$M_{rm s}$ relation ${rm log} […]


Continue.. The Origin of the Relation Between Stellar Angular Momentum and Stellar Mass in Nearby Disk-dominated galaxies

The Origin of the Stellar Angular Momentum-Mass Relation: Connecting Galaxies and Halos in IllustrisTNG

Kavli Affiliate: Luis C. Ho | First 5 Authors: Min Du, Luis C. Ho, Hao-Ran Yu, Victor P. Debattista, | Summary: The IllustrisTNG simulations reproduce well the observed scaling relation between specific angular momentum (sAM) $j_{rm s}$ and mass $M_{rm s}$ of galaxies, i.e., the $j_{rm s}$-$M_{rm s}$ relation. This relation develops in disk galaxies […]


Continue.. The Origin of the Stellar Angular Momentum-Mass Relation: Connecting Galaxies and Halos in IllustrisTNG