Searching for Dark Clumps with Gravitational-Wave Detectors

Kavli Affiliate: Peter W. Graham | First 5 Authors: Sebastian Baum, Michael A. Fedderke, Peter W. Graham, , | Summary: Dark compact objects ("clumps") transiting the Solar System exert accelerations on the test masses (TM) in a gravitational-wave (GW) detector. We reexamine the detectability of these clump transits in a variety of current and future […]


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The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

Kavli Affiliate: Eli S. Rykoff | First 5 Authors: The Astropy Collaboration, Adrian M. Price-Whelan, Pey Lian Lim, Nicholas Earl, Nathaniel Starkman | Summary: The Astropy Project supports and fosters the development of open-source and openly-developed Python packages that provide commonly needed functionality to the astronomical community. A key element of the Astropy Project is […]


Continue.. The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

Kavli Affiliate: Eli S. Rykoff | First 5 Authors: The Astropy Collaboration, Adrian M. Price-Whelan, Pey Lian Lim, Nicholas Earl, Nathaniel Starkman | Summary: The Astropy Project supports and fosters the development of open-source and openly-developed Python packages that provide commonly needed functionality to the astronomical community. A key element of the Astropy Project is […]


Continue.. The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

Bandwidth and Aliasing in the Microwave SQUID Multiplexer

Kavli Affiliate: Zeeshan Ahmed | First 5 Authors: Cyndia Yu, Zeeshan Ahmed, Jake A. Connors, J. Mitch D’Ewart, Bradley Dober | Summary: The microwave SQUID multiplexer (umux) has enabled higher bandwidth or higher channel counts across a wide range of experiments in particle physics, astronomy, and spectroscopy. The large multiplexing factor coupled with recent commercial […]


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Formal Analysis of Lending Pools in Decentralized Finance

Kavli Affiliate: James Chiang | First 5 Authors: Massimo Bartoletti, James Chiang, Tommi Junttila, Alberto Lluch Lafuente, Massimiliano Mirelli | Summary: Decentralised Finance (DeFi) applications constitute an entire financial ecosystem deployed on blockchains. Such applications are based on complex protocols and incentive mechanisms whose financial safety is hard to determine. Besides, their adoption is rapidly […]


Continue.. Formal Analysis of Lending Pools in Decentralized Finance

Formal Analysis of Lending Pools in Decentralized Finance

Kavli Affiliate: James Chiang | First 5 Authors: Massimo Bartoletti, James Chiang, Tommi Junttila, Alberto Lluch Lafuente, Massimiliano Mirelli | Summary: Decentralised Finance (DeFi) applications constitute an entire financial ecosystem deployed on blockchains. Such applications are based on complex protocols and incentive mechanisms whose financial safety is hard to determine. Besides, their adoption is rapidly […]


Continue.. Formal Analysis of Lending Pools in Decentralized Finance

The Evolution and Mass Dependence of Galaxy Cluster Pressure Profiles at 0.05 $le z le$ 0.60 and $4 times 10^{14}$ M$_{odot}$ $le textrm{M}_{500} le 30 times 10^{14}$ M$_{odot}$

Kavli Affiliate: Steven W. Allen | First 5 Authors: Jack Sayers, Adam B. Mantz, Elena Rasia, Steven W. Allen, Weiguang Cui | Summary: We have combined X-ray observations from Chandra with Sunyaev-Zel’dovich (SZ) effect data from Planck and Bolocam to measure intra-cluster medium pressure profiles from 0.03R$_{500}$ $le$ R $le$ 5R$_{500}$ for a sample of […]


Continue.. The Evolution and Mass Dependence of Galaxy Cluster Pressure Profiles at 0.05 $le z le$ 0.60 and $4 times 10^{14}$ M$_{odot}$ $le textrm{M}_{500} le 30 times 10^{14}$ M$_{odot}$

The Evolution and Mass Dependence of Galaxy Cluster Pressure Profiles at 0.05 $le z le$ 0.60 and $4 times 10^{14}$ M$_{odot}$ $le textrm{M}_{500} le 30 times 10^{14}$ M$_{odot}$

Kavli Affiliate: Adam B. Mantz | First 5 Authors: Jack Sayers, Adam B. Mantz, Elena Rasia, Steven W. Allen, Weiguang Cui | Summary: We have combined X-ray observations from Chandra with Sunyaev-Zel’dovich (SZ) effect data from Planck and Bolocam to measure intra-cluster medium pressure profiles from 0.03R$_{500}$ $le$ R $le$ 5R$_{500}$ for a sample of […]


Continue.. The Evolution and Mass Dependence of Galaxy Cluster Pressure Profiles at 0.05 $le z le$ 0.60 and $4 times 10^{14}$ M$_{odot}$ $le textrm{M}_{500} le 30 times 10^{14}$ M$_{odot}$

The Evolution and Mass Dependence of Galaxy Cluster Pressure Profiles at 0.05 $le z le$ 0.60 and $4 times 10^14$ M$_odot$ $le textrmM_500 le 30 times 10^14$ M$_odot$

Kavli Affiliate: Adam Mantz | Summary:We have combined X-ray observations from Chandra with Sunyaev-Zel’dovich (SZ) effect data from Planck and Bolocam to measure intra-cluster medium pressure profiles from 0.03R$_500$ $le$ R $le$ 5R$_500$ for a sample of 21 low-$z$ galaxy clusters with a median redshift $langle z rangle = 0.08$ and a median mass $langle […]


Continue.. The Evolution and Mass Dependence of Galaxy Cluster Pressure Profiles at 0.05 $le z le$ 0.60 and $4 times 10^14$ M$_odot$ $le textrmM_500 le 30 times 10^14$ M$_odot$

Effective Field Theory Analysis of CDMSlite Run 2 Data

Kavli Affiliate: Paul Brink | Summary:CDMSlite Run 2 was a search for weakly interacting massive particles (WIMPs) with a cryogenic 600 g Ge detector operated in a high-voltage mode to optimize sensitivity to WIMPs of relatively low mass from 2 – 20 GeV/$c^2$. In this article, we present an effective field theory (EFT) analysis of […]


Continue.. Effective Field Theory Analysis of CDMSlite Run 2 Data