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Astrophysics

Papers reviewed in the last 7 days lead, then the papers readers actually read. Ranking is not a quality score.

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Higgsino dark matter faces tension from LZ's empty sideband

Thermal 1.1 TeV higgsino predicts multiple high-energy recoils, but LZ sees none; a ~500 GeV non-thermal higgsino may evade.

· “Confronting the Higgsino Interpretation of the LZ Event with the High-Energy Sideband”

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One dark sector explains both LZ event and gamma-ray excess

A 420-GeV dark photon with a nearly degenerate partner reproduces the 248-keV nuclear recoil while preserving the Sommerfeld-enhanced halo…

· “Inelastic Dark Photon Dark Matter for the LUX-ZEPLIN High-Recoil Event and the Galactic Halo Gamma-Ray Excess”

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X-ray observations of galaxy groups and clusters are used here to measure how much hot…

Fitting a baryonification model to CHEX-MATE and eFEDs X-ray data yields gas fractions of 0.029 and 0.078 at two mass scales and a 6 to 23…

· “Baryonification IV: Constraining baryonic feedback with X-ray gas fractions”

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Galaxies, not 21cm, drive reionization-era seed reconstruction

In the hybrid TILING pipeline, galaxies pin the phases of the early density field while 21cm maps fix the amplitudes, reaching k ≈ 0.2…

· “TILING I: Field-level Bayesian reconstruction of cosmological initial conditions during the epoch of reionization”

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Black-hole merger rates, straight from pulsar timing data

The stochastic background and individual merger bursts constrain the same binary population in one hierarchical model.

· “Hierarchical Inference of the Supermassive Black Hole Binary Merger Rates from Joint Searches using Pulsar Timing Arrays”

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Cold Jupiter eccentricities reveal violent origins for hot Jupiters

A 5.75σ difference in outer companion eccentricity supports divergent formation histories for hot and warm Jupiters.

· “The Discovery of K2-232c: Divergent Formation Histories for Hot and Warm Jupiters Based on Outer Companion Eccentricity”

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95% of radio-loud AGNs in cluster cores are low-excitation

Study of 171 brightest cluster galaxies at z = 0.3–0.8 finds that maintenance-mode feedback was already common by z ~ 1.

· “Active galactic nucleus activity in brightest cluster galaxies at intermediate redshifts in Sunyaev-Zel'dovich--selected clusters”

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This paper reports that regularized kappa distributions (RKDs) unlock a regime of extreme…

Modeling suprathermal tails with RKD reveals extreme aperiodic instability at oblique angles beyond Maxwellian reach.

· “On the modeling of oblique firehose instabilities in regularized Kappa plasmas using ALPS”

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Black hole masses equal pre-collapse core masses of Wolf-Rayet stars

Accounting for wind mass loss, the relation M_BH ≈ M_CO is recovered from observed distributions of 31 WR stars and 53 black holes.

· “Wolf-Rayet stars and black holes: mass distributions and evolutionary connection”

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Researchers analyzed XMM-Newton X-ray data from two epochs (2000 and 2006) of the quasar…

Two distinct ultra-fast outflow components are detected in each of two XMM-Newton observations of Mrk205, with velocities ~0.07–0.1c, and…

· “Detection of episodic Ultra-fast Outflows in the Low-luminosity quasar Mrk 205 using XMM-Newton data”

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Open clusters remain the essential laboratories for calibrating how rotation

Open clusters benchmark rotation, activity, and chemistry, but new results challenge simple models.

· “Open Clusters as Laboratories for Cool Star Evolution: Highlights from the Cool Stars 23 Splinter Session”

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Gaia data yield closed-form equations for Milky Way's local potential

Method avoids degeneracy that plagues joint fits, recovers self-gravitating disk shape and first analytical distribution function.

· “Closed-Form of the Local Galactic Potential and Stellar Distribution Function from Gaia DR3”

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Stacked CMB maps yield optical depths that match kSZ values

New y-tau scaling relations turn ACT Compton-y stacks into cluster optical depths for DESI samples.

· “Optical Depths from the Thermal Sunyaev-Zel'dovich Effect with ACT DR6 and DESI DR1 Spectroscopic Galaxies and Optically-Selected Clusters”

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White dwarfs vanish for years in sudden dust events

Six stars dimmed by 25-100 percent, one fully, pointing to planetesimal collisions near dead stars.

· “Now you see me, now you don't: Deep, long-lived obscuration events of white dwarfs by dust and debris from disintegrating planetesimals”

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UHE emission reveals a conditional EoS window in a gamma-ray binary

Phase-resolved LHAASO data define a narrow boundary where moments of inertia distinguish EoS only under specific engine conditions.

· “Phase-Resolved Ultra-High-Energy Emission Defines an Energetic Boundary for Compact-Object Engines and Dense-Matter Structure”

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Environment alone leaves a central galaxy's gas halo unchanged

A high-resolution simulation shows the extra absorption around group galaxies comes from satellites, not the environment.

· “The environmental dependence of the circumgalactic medium in a high-resolution cosmological simulation”

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External UV leaves a distinct chemical fingerprint on planet-forming disks—until it…

Grid of 45 disk models predicts when JWST sees bright CH3+ and H2 emission and when it does not, separating internal and external…

· “XUE. ProDiMo models of internally and externally irradiated planet-forming disks around 0.3-4.0 solar mass stars (The IRIS project I)”

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Six brown dwarfs confirmed, 13 fakes exposed in Gaia follow-up

Spectroscopic vetting of 20 Gaia DR3 substellar candidates shows that 13 are stellar twins mimicking dark companions and six are genuine…

· “Radial velocity follow-up of textit{Gaia} astrometric substellar companions: six confirmed brown dwarfs and 13 impostor binaries”

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One lens plus stellar kinematics sets dark energy at w = -1.01

Kinematics break the lensing degeneracy so a single double-source system can test evolving dark energy.

· “Harnessing stellar kinematics to constrain dark energy with the double-source-plane gravitational lens SDSS J0946+1006”

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Deconvolution recovers percent-level matter modulations in 3x2pt data

Regularized Richardson-Lucy algorithm detects 1% oscillations at 2.77σ with LSST Y10-like synthetic surveys.

· “Finding the distribution of matter using lenses - II: deconvolution-based reconstruction with 3x2pt measurements”

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