arXiver

Twitter feed of the arXiver WordPress --- bringing you the latest astronomy papers uploaded to astro-ph.

[arXiver @arXiver]

We've had a lot of issues with #arXiver lately, most likely due to the size of our @WordPress database (#toomanypapers). It's working again but we don't know for how long... Please give us insight into how important the Wordpress site is to you! (other suggestions welcome)

[arXiver @arXiver]

Revealing mass distributions of dwarf spheroidal galaxies in the Subaru-PFS era [GA] https://t.co/32qQRLNoRy

[arXiver @arXiver]

MUSE AO spectroscopy confirms five dual AGNs and two strongly lensed QSOs at sub-arcsec separation [GA] https://t.co/rPMgmRbfX9

[arXiver @arXiver]

The JCMT BISTRO Survey: Studying the Complex Magnetic Field of L43 [GA] https://t.co/U4gKIEWZVt

[arXiver @arXiver]

Density and magnetic intensity dependence of radio pulses induced by energetic air showers [HEAP] https://t.co/yS5iVlTHoY

[arXiver @arXiver]

A type II solar radio burst without a coronal mass ejection [SSA] https://t.co/3gBa3E7Z1K

[arXiver @arXiver]

Flux Calibration of CHIME/FRB Intensity Data [IMA] https://t.co/hDNzk21niM

[arXiver @arXiver]

A type II solar radio burst without a coronal mass ejection [SSA] https://t.co/OfLUDfM5Uy

[arXiver @arXiver]

Hall effect on the magnetic reconnections during the evolution of a three-dimensional magnetic flux rope... [SSA] https://t.co/OfLUDfM5Uy

[arXiver @arXiver]

Coupled Multi Scalar Field Dark Energy [CEA] https://t.co/itJE3pq530

[arXiver @arXiver]

Planet-disk-wind interaction: the magnetized fate of protoplanets [SSA] https://t.co/5J3krIl7t3

[arXiver @arXiver]

DarkAI: I. Mapping the large-scale density field of dark matter using AI [CEA] https://t.co/5KqU1ws1e6

[arXiver @arXiver]

The 14 Her Planetary System: Companion Masses and Architecture from Radial Velocities and Astrometry [EPA] https://t.co/7v9uqhN7k5

[arXiver @arXiver]

Evidence Networks: simple losses for fast, amortized, neural Bayesian model comparison [CL] https://t.co/s4sBpJYvlh

[arXiver @arXiver]

Planetesimal formation via the streaming instability with multiple grain sizes [EPA] https://t.co/QekLtThTg4

[arXiver @arXiver]

Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions [HEAP] https://t.co/Un9PpmsRaH

[arXiver @arXiver]

CN and CO Features: Key Indicators of Red Giant Evolutionary Phase in Moderate-Resolution X-Shooter... [SSA] https://t.co/8WWlfigZcv

[arXiver @arXiver]

Powerful Radio-Loud Quasars are Triggered by Galaxy Mergers in the Cosmic Bright Ages [GA] https://t.co/tqlz4kebpb

[arXiver @arXiver]

Engineering the sensitivity of macroscopic physical systems to variations in the fine-structure constant... [CL] https://t.co/Q81LJLvMHi

[arXiver @arXiver]

Temperature inhomogeneities cause the abundance discrepancy in H II regions [GA] https://t.co/D3nvlIkiNE

[arXiver @arXiver]

Mass Derivation of planets K2-21b and K2-21c from Transit Timing Variations [EPA] https://t.co/9xF9gKMIxS