Time-variable Scattered Light in Herbig Disks Observed with Subaru/SCExAO

Kavli Affiliate: Ruobing Dong | Summary:Using the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument, we present near-infrared K-band polarimetric imaging of nine Herbig stars selected from a volume-limited sample within 200 pc. We detect the disks around MWC 480, HD 163296, and HD 143006 for the first time with SCExAO, and compare these observations with […]


Continue.. Time-variable Scattered Light in Herbig Disks Observed with Subaru/SCExAO

Time-variable Scattered Light in Herbig Disks Observed with Subaru/SCExAO

Kavli Affiliate: Ruobing Dong | Summary:Using the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument, we present near-infrared K-band polarimetric imaging of nine Herbig stars selected from a volume-limited sample within 200 pc. We detect the disks around MWC 480, HD 163296, and HD 143006 for the first time with SCExAO, and compare these observations with […]


Continue.. Time-variable Scattered Light in Herbig Disks Observed with Subaru/SCExAO

Time-variable Scattered Light in Herbig Disks Observed with Subaru/SCExAO

Kavli Affiliate: Ruobing Dong | Summary:Using the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument, we present near-infrared K-band polarimetric imaging of nine Herbig stars selected from a volume-limited sample within 200 pc. We detect the disks around MWC 480, HD 163296, and HD 143006 for the first time with SCExAO, and compare these observations with […]


Continue.. Time-variable Scattered Light in Herbig Disks Observed with Subaru/SCExAO

BASS LV. Connecting X-ray variability with AGN physical properties and a new path to Cosmological distances

Kavli Affiliate: Claudio Ricci | Summary:X-ray variability is a well-established characteristic of active galactic nuclei (AGN), known to correlate inversely with both the supermassive black hole mass and luminosity, although the degree of each remains a topic of debate. The potential of X-ray variability as a proxy for MBH or for intrinsic LX has led […]


Continue.. BASS LV. Connecting X-ray variability with AGN physical properties and a new path to Cosmological distances

BASS LVI. Connecting X-ray variability with AGN physical properties and a new path to Cosmological distances

Kavli Affiliate: Claudio Ricci | Summary:X-ray variability is a well-established characteristic of active galactic nuclei (AGN), known to correlate inversely with both the supermassive black hole mass and luminosity, although the degree of each remains a topic of debate. The potential of X-ray variability as a proxy for MBH or for intrinsic LX has led […]


Continue.. BASS LVI. Connecting X-ray variability with AGN physical properties and a new path to Cosmological distances

A non-invasive method to genotype cephalopod sex by quantitative PCR

Kavli Affiliate: Scott Small | Authors: Frederick A. Rubino, Gabrielle C. Coffing, Connor J. Gibbons, Scott T. Small, Thomas Desvignes, Jeffery Pessutti, Ann M. Petersen, Alexander Arkhipkin, Zhanna Shcherbich, John H. Postlethwait, Andrew D. Kern and Tessa G. Montague | Summary: Coleoid cephalopods (cuttlefish, octopus, and squid) are emerging model organisms in neuroscience, development, and […]


Continue.. A non-invasive method to genotype cephalopod sex by quantitative PCR

Neural Bayesian updates to populations with growing gravitational-wave catalogs

Kavli Affiliate: Salvatore Vitale | Summary:As gravitational-wave catalogs grow, they will become increasingly computationally expensive to analyze in their entirety, especially when inferring astrophysical source populations with high-dimensional, flexible models. Bayesian statistics offers a natural remedy, letting us update our knowledge of physical models as new data arrive, without re-analyzing existing data. However, doing so […]


Continue.. Neural Bayesian updates to populations with growing gravitational-wave catalogs

The ALPINE-CRISTAL-JWST Survey: Chemical Abundance Comparison Between the ISM and CGM of Main-Sequence Galaxies at z=4-6

Kavli Affiliate: John Silverman | Summary:Gaseous halos around galaxies play an important role in galaxy evolution. The exchange of metals from the interstellar medium (ISM) to the circumgalactic medium (CGM) are caused by the formation, feedback, and/or merging history of galaxies. We study the variation in chemical composition between the ISM ($lesssim3,$kpc) and CGM ($sim5-10,$kpc) […]


Continue.. The ALPINE-CRISTAL-JWST Survey: Chemical Abundance Comparison Between the ISM and CGM of Main-Sequence Galaxies at z=4-6

Experimental characterization of coherent and non-Markovian errors using tangent space decomposition

Kavli Affiliate: Birgitta Whaley | Summary:Accurate characterization of coherent and non-Markovian errors remains a central challenge in quantum information processing, as conventional benchmarking techniques typically rely on Markovian and time-independent noise assumptions. In practice, however, quantum devices exhibit both systematic coherent miscalibrations and temporally correlated fluctuations, which complicate error diagnosis and mitigation. Here, we apply […]


Continue.. Experimental characterization of coherent and non-Markovian errors using tangent space decomposition

The Orbital Eccentricity–Radius Distribution for Warm, Single Planets in TESS

Kavli Affiliate: Sara Seager | Summary:We characterize the radius-dependent eccentricity distribution of 347 warm (P = 8-200 days) systems with only one transiting planetary candidate identified during Sectors 1-69 of the TESS mission. Using the “photoeccentric effect” in a hierarchical Bayesian framework, we first model the population using discrete planetary size bins (sub-Neptunes, sub-Saturns, and […]


Continue.. The Orbital Eccentricity–Radius Distribution for Warm, Single Planets in TESS