Investigation of Real-Space Transfer Noise in InP Quantum Wells

Kavli Affiliate: Austin Minnich | Summary:Indium phosphide (InP) high electron-mobility transistors (HEMTs) are widely used in many fields such as quantum computing because of their unparalleled microwave noise performance. Achieving improved noise performance requires a physical understanding of the noise mechanisms. Here, we experimentally test a theoretical proposal for drain (output) noise as originating in […]


Continue.. Investigation of Real-Space Transfer Noise in InP Quantum Wells

Detailed Chemical Abundance Analysis of the Brightest Stars in the Turranburra and Willka Yaku Stellar Streams

Kavli Affiliate: Alexander Ji | Summary:We present a detailed chemical abundance analysis of the three brightest known stars from each of the Turranburra and Willka Yaku stellar streams using high-resolution Magellan/MIKE spectra. Abundances for 27 elements, ranging from carbon to dysprosium, were derived. Our results support the original classification that Turranburra, with a low average […]


Continue.. Detailed Chemical Abundance Analysis of the Brightest Stars in the Turranburra and Willka Yaku Stellar Streams

GA-NIFS: Powerful and frequent outflows in moderate-luminosity active galactic nuclei at $zsim3-6$

Kavli Affiliate: Roberto Maiolino | Summary:The period between z ~ 3-6, a key transformational phase in galaxy evolution preceding ‘cosmic noon’ (z ~ 1-3), is very poorly explored in terms of feedback from AGN acting through gas outflows. In this work, we study the properties of outflows in AGN (mostly X-ray-selected) from the GOODS-S field, […]


Continue.. GA-NIFS: Powerful and frequent outflows in moderate-luminosity active galactic nuclei at $zsim3-6$

GA-NIFS: Powerful and frequent outflows in moderate-luminosity active galactic nuclei at $zsim3-6$

Kavli Affiliate: Roberto Maiolino | Summary:The period between z ~ 3-6, a key transformational phase in galaxy evolution preceding ‘cosmic noon’ (z ~ 1-3), is very poorly explored in terms of feedback from AGN acting through gas outflows. In this work, we study the properties of outflows in AGN (mostly X-ray-selected) from the GOODS-S field, […]


Continue.. GA-NIFS: Powerful and frequent outflows in moderate-luminosity active galactic nuclei at $zsim3-6$

GA-NIFS: Powerful and frequent outflows in moderate-luminosity AGN at $zsim3-6$

Kavli Affiliate: Roberto Maiolino | Summary:The period between z ~ 3-6, a key transformational phase in galaxy evolution preceding ‘cosmic noon’ (z ~ 1-3), is very poorly explored in terms of feedback from AGN acting through gas outflows. In this work, we study the properties of outflows in AGN (mostly X-ray-selected) from the GOODS-S field, […]


Continue.. GA-NIFS: Powerful and frequent outflows in moderate-luminosity AGN at $zsim3-6$

Planckian Bounds via Spectral Moments of Optical Conductivity

Kavli Affiliate: Debanjan Chowdhury | Summary:The observation of Planckian scattering, often inferred from Drude fits in strongly correlated metals, raises the question of how to extract an intrinsic timescale from measurable quantities in a model-independent way. We address this by focusing on a ratio ($calB$) of spectral moments of the dissipative part of the optical […]


Continue.. Planckian Bounds via Spectral Moments of Optical Conductivity

Scintillation response of cryogenic CsI to few-keV and sub-keV nuclear recoils

Kavli Affiliate: Juan I. Collar | Summary:Monochromatic neutron emissions from photonuclear sources $^88$Y/Be and $^124$Sb/Be are employed to obtain the response of pure (undoped) cesium iodide at 80 K. The use of a low-noise, high-quantum-efficiency avalanche photodiode in combination with a novel waveshifter results in a 70 eV analysis threshold. This reach allows to observe […]


Continue.. Scintillation response of cryogenic CsI to few-keV and sub-keV nuclear recoils

Dynamic stimulated emission for deterministic addition and subtraction of propagating photons

Kavli Affiliate: Mohammad Mirhosseini | Summary:Photon subtraction and addition are essential non-Gaussian processes in quantum optics, where conventional methods using linear optics and number-resolving detection often suffer from low success probability. Here, we introduce the concept of textitdynamic stimulated emission, whereby a quantum emitter undergoes stimulated emission with a time-dependent coupling. We show that, for […]


Continue.. Dynamic stimulated emission for deterministic addition and subtraction of propagating photons

LoGoColor: Local-Global 3D Colorization for 360° Scenes

Kavli Affiliate: Hsiao-Mei (Sherry) Cho| First 5 Authors: [#item_custom_name[1, [#item_custom_name[2, [#item_custom_name[3, [#item_custom_name[4, [#item_custom_name[5| Summary:Single-channel 3D reconstruction is widely used in fields such as robotics and medical imaging. While this line of work excels at reconstructing 3D geometry, the outputs are not colored 3D models, thus 3D colorization is required for visualization. Recent 3D colorization studies […]


Continue.. LoGoColor: Local-Global 3D Colorization for 360° Scenes

Delving into the depths of NGC 3783 with XRISM IV. Mapping of the accretion flow with Fe K$α$ emission lines

Kavli Affiliate: Erin Kara | Summary:Using XRISM/Resolve $439 , rm ks$ time-averaged spectra of the well-known Seyfert-1.5 active galactic nucleus (AGN) in NGC 3783, we investigate the nature of the Fe K$α$ emission line at 6.4 keV, the strongest and most common X-ray line observed in AGN. Even the narrow component of the line is […]


Continue.. Delving into the depths of NGC 3783 with XRISM IV. Mapping of the accretion flow with Fe K$α$ emission lines