AGN STORM 2. XII. Ground-Based Optical Photometry and Lag Measurements of Mrk 817

Kavli Affiliate: Erin Kara | Summary:We present the ground-based imaging campaign and light curves of Markarian 817 as part of the multiwavelength monitoring program AGN STORM,2. Observations were carried out over 1.4 years in emphuBgVriz filters, with a median cadence of 0.4 days in emphg. Reverberation lags are measured using three methods (ICCF, JAVELIN, and […]


Continue.. AGN STORM 2. XII. Ground-Based Optical Photometry and Lag Measurements of Mrk 817

JWST unveils a high mean molecular weight atmosphere for mini-Neptune TOI-1130b: Evidence for formation beyond the water ice line

Kavli Affiliate: Andrew Vanderburg | Summary:We present the combined JWST/NIRSpec G395H and NIRISS SOSS transmission spectrum of a warm mini-Neptune, TOI-1130b (3.66 R$_oplus$, 19.8 M$_oplus$, $T_eqsim825$ K). It is part of a rare and unique multi-planet system TOI-1130, which hosts an inner mini-Neptune and an outer hot Jupiter locked in a 2:1 mean motion resonance. […]


Continue.. JWST unveils a high mean molecular weight atmosphere for mini-Neptune TOI-1130b: Evidence for formation beyond the water ice line

XRISM/Resolve observations of Hercules X-1: a pulsating, highly broadened Fe K emission line from the neutron star accretion column

Kavli Affiliate: Erin Kara | Summary:The study of X-ray pulsar accretion columns helps us characterize accretion physics in this extreme regime of strong gravity and strong magnetic fields. Previous observations of the X-ray pulsar Hercules X-1 revealed a highly broadened Fe K emission line, associated with Doppler motions exceeding 0.1c, suggesting its origin in the […]


Continue.. XRISM/Resolve observations of Hercules X-1: a pulsating, highly broadened Fe K emission line from the neutron star accretion column

Formation and Redshift Evolution of Dark Matter Spikes

Kavli Affiliate: Lina Necib | Summary:Dark matter density spikes forming around adiabatically growing black holes can dramatically enhance indirect and direct detection signals. Canonical predictions, however, assume a zero-mass seed in a purely dark matter environment and do not track the long-term dynamical impact of surrounding stars. We present a semi-analytic framework that first generalizes […]


Continue.. Formation and Redshift Evolution of Dark Matter Spikes

Discovery of Quasar Variability and Early Accretion Disk Signatures at Cosmic Dawn

Kavli Affiliate: Erin Kara | Summary:In the nearby universe, quasars are well known to exhibit variability in their brightness over time, offering a powerful tool to probe the physics of accretion onto the SMBH and directly measure the mass of the SMBH. However, detecting variability in early quasars remains challenging. Here, we report the detection […]


Continue.. Discovery of Quasar Variability and Early Accretion Disk Signatures at Cosmic Dawn

A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications

Kavli Affiliate: Mark Vogelsberger | Summary:Precession is a very common phenomenon for small-scale astronomical objects. However, the precession of galactic disks, occurring on a scale larger than kilo-parsec, has barely been studied in the literature. Quantifying this precession in observations remains challenging due to the lack of high-resolution dynamical data. Cosmological simulations, where gravitational interactions […]


Continue.. A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications

A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications

Kavli Affiliate: Mark Vogelsberger | Summary:Precession is a very common phenomenon for small-scale astronomical objects. However, the precession of galactic disks, occurring on a scale larger than kilo-parsec, has barely been studied in the literature. Quantifying this precession in observations remains challenging due to the lack of high-resolution dynamical data. Cosmological simulations, where gravitational interactions […]


Continue.. A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications

The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries

Kavli Affiliate: Mark Vogelsberger | Summary:In the hierarchical paradigm of galaxy formation, central massive black holes (MBHs) are expected to coalesce after the merger of their host galaxies. One of the main goals of the Laser Interferometer Space Antenna (LISA) is to constrain the origin and growth of MBHs through their merger rates and mass […]


Continue.. The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries

Fast radio burst dispersion is an unbiased tracer of matter on large scales

Kavli Affiliate: Kiyoshi Masui | Summary:The dispersion of fast radio bursts (FRBs) measures the column density of free electrons, tracing the diffuse ionized gas that contains more than $90%$ of all baryons. On linear scales the FRB dispersion field is an approximately unbiased tracer of the matter distribution, an idea long assumed in the FRB […]


Continue.. Fast radio burst dispersion is an unbiased tracer of matter on large scales

Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation

Kavli Affiliate: Mark Vogelsberger | Summary:The origin and structure of the hot ($Tgtrsim10^6$ K) gaseous halo around Milky Way (MW)-mass galaxies provide a critical test for galaxy formation models. We perform a comprehensive comparison for a sample of MW analogues from the TNG50 cosmological simulation by generating synthetic soft X-ray emission and O VII/O VIII […]


Continue.. Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation