TESS Hunt for Young and Maturing Exoplanets (THYME) XIV: A Comoving-Based Age Constraint for KELT-20

Kavli Affiliate: Andrew Vanderburg | Summary:Young stellar moving groups offer unique opportunities to investigate the early evolution of stellar and planetary systems. In continuation of an ongoing effort to age-date compelling planetary systems, we provide an in-depth age analysis of KELT-20, a young A-type star that hosts a well-aligned ultra-hot Jupiter. This system poses a […]


Continue.. TESS Hunt for Young and Maturing Exoplanets (THYME) XIV: A Comoving-Based Age Constraint for KELT-20

Constraining the mass of the M31 ionized baryon Halo using CHIME/FRB Catalog 2

Kavli Affiliate: Kiyoshi Masui | Summary:The circumgalactic medium (CGM) surrounding galaxies is believed to be a significant reservoir of baryons, yet its total mass remains poorly constrained. We present a novel approach to probe the CGM of the Andromeda galaxy (M31) using fast radio bursts (FRBs) from the CHIME/FRB Catalog 2. By comparing the dispersion […]


Continue.. Constraining the mass of the M31 ionized baryon Halo using CHIME/FRB Catalog 2

Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz

Kavli Affiliate: Peter Fritschel | Summary:Extending the sensitivity of terrestrial gravitational-wave detectors below 20 Hz is a long-standing challenge, limited by ground motion and inertial sensing noise. In this letter, we demonstrate ultra-high-vacuum compatible inertial isolation and position sensing technologies that achieve active platform stabilization down to 10 mHz. Our laser position sensors reach a […]


Continue.. Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz

Variability of the X-ray obscuring wind in Mrk 335 with XMM-Newton/RGS

Kavli Affiliate: Erin Kara | Summary:Transient X-ray obscuration in Seyfert 1 galaxies is thought to arise from clumpy accretion-disk winds near the broad-line region (BLR), but the wind structure and its short-timescale variability are difficult to measure because high-resolution spectra are often suppressed during deep low states. We analyse a coordinated XMM-Newton/NuSTAR campaign on Mrk […]


Continue.. Variability of the X-ray obscuring wind in Mrk 335 with XMM-Newton/RGS

A Decision-Theoretic Formalisation of Steganography With Applications to LLM Monitoring

Kavli Affiliate: Max Tegmark | Summary:Large language models are beginning to show steganographic capabilities. Such capabilities could allow misaligned models to evade oversight mechanisms. Yet principled methods to detect and quantify such behaviours are lacking. Classical definitions of steganography, and detection methods based on them, require a known reference distribution of non-steganographic signals. For the […]


Continue.. A Decision-Theoretic Formalisation of Steganography With Applications to LLM Monitoring

High Spectral Resolution X-ray Observations of the Evolved Supermassive Stellar Binary System $η$ Carinae – Iron K$α$ Band Profile Revealed with XRISM

Kavli Affiliate: Erin Kara | Summary:The supermassive binary system, $η$ Carinae, is experiencing enormous wind-driven mass loss at a rate unparalleled in the rest of the Galaxy. Their wind-wind collision (WWC) continuously produces shock heated, X-ray emitting plasmas. The XRISM X-ray observatory observed the system in 2023 and 2024 when the X-ray emission began to […]


Continue.. High Spectral Resolution X-ray Observations of the Evolved Supermassive Stellar Binary System $η$ Carinae – Iron K$α$ Band Profile Revealed with XRISM

A steadily declining dispersion measure for the repeating fast radio burst FRB 20220529A: Evidence for an FRB engine embedded in an expanding supernova remnant

Kavli Affiliate: Kiyoshi Masui | Summary:We present the discovery and subsequent 3.2 year monitoring campaign of the repeating fast radio burst FRB 20220529A with CHIME/FRB. We observe a gradual dispersion measure (DM) decline of $-0.881pm0.001~mathrmpc~mathrmcm^-3~mathrmyear^-1$ ($-1.235pm0.001~mathrmpc~mathrmcm^-3~mathrmyear^-1$ in the rest frame), implying a $geq3.5pm0.2$% decrease of the total electron column in the source environment, and we […]


Continue.. A steadily declining dispersion measure for the repeating fast radio burst FRB 20220529A: Evidence for an FRB engine embedded in an expanding supernova remnant

AT2024lhc and AT2024kmq in the landscape of featureless tidal disruption events

Kavli Affiliate: Dheeraj Pasham | Summary:We study AT2024kmq and AT2024lhc, two tidal disruption events (TDEs) with blue featureless spectra associated with high-mass black holes ($M_rm BHsim 10^8,M_odot$). Both events show optical precursors consistent with shock dissipation from stream self-intersection. Their X-ray emission is luminous ($L_rm Xsim 10^44,rm erg,s^-1$), highly variable (with minimum observed variability timescales […]


Continue.. AT2024lhc and AT2024kmq in the landscape of featureless tidal disruption events

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 […]


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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