archive
Every paper Pith has read. Search by title, abstract, or pith.
383 papers in astro-ph.EP · page 1
-
Mars dust storms create 100-1000 V/m electric fields in southern belts
Global evolution of electric fields during planet encircling dust storms on Mars
-
Bessel kernel resolves convergence in 2D disc gravity simulations
Self-gravity in thin protoplanetary discs: 2. Numerical convergence solved and revealing the overestimation in mass of formed planets with softening
-
Halley fits 15 orbits into 1,151-year solar cycle
Comet 1P/Halley Completes 15 Orbits in 1,151 Years: Commensurability with the Solar System Quasi-Period and Evidence for Jupiter-Saturn Dynamical Coupling
-
Spread in CO2 sticking energies extends gas in disks
Fizzy water ice in space: CO$_2$ adsorption, binding energies and its fate in a protoplanetary disk
-
Hot cores near supernova show unchanged molecular ratios
Survival of Molecular Complexity under Recent Supernova Feedback: Detection of Hot Cores in RX J1713.7-3946
-
Catalog supplies ages for 659 HWO stars but covers only 25 percent
The HAges Catalog: Stellar Ages for High Priority HWO Target Stars
-
18 hot Ariel stars receive uniform parameters
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample
-
Eta Tel disk gas has low C/O like solar system comets
Revisiting the ultraviolet spectroscopy of the eta Tel edge-on debris disk
-
Shocks dominate planet wave damping but cooling rivals them for small planets
$\alpha\beta q_\mathrm{th}$-mapping of planet-induced density wave damping in protoplanetary discs
-
Capture can stabilize pulsar planets at low eccentricity
Formation of stable exoplanetary systems around pulsars by capture: An exercise in computational classical mechanics
-
Asteroid dust flux matches models at inner planets
Modeling and Analysis of Main-Belt Asteroidal Dust Flux and Velocity Distribution at Inner Planets
-
1923 Newtonian estimate gave 49 hours to the Moon
On the Anticipation of Lunar Travel in the Early 20th Century: A Pedagogical Exercise
-
W-Net spots asteroids in TESS data regardless of path
Trajectory-Agnostic Asteroid Detection in TESS with Deep Learning
-
Dense super-Earth around K dwarf may upend formation theories
An Ultra-Short Period Super-Earth and a Sub-Neptune Orbiting the K dwarf TOI-4311
-
Molten cores turn asteroid collisions into iron-rich rubble piles
Reaccumulation process after a catastrophic disruption event on a differentiated asteroid
-
Tidal models fix rotation states for six Kepler exoplanets
Simulation of the spin evolution of some selected exoplanets and inferences on their climate
-
H2 broadening data for CO2 lines now spans 200-1000 K
Measurements and predictions of H2 pressure-broadening coefficients of CO2 absorption lines for exoplanet atmosphere studies
-
Hybrid model explains distant disk rings in V1094 Sco
A Hybrid Origin for the Multiple Ring-Gap Structures in the Large Protoplanetary Disk V1094 Sco: A Low-Mass Planet and Secular Gravitational Instability
-
Engulfed planets dissolve steadily inside stars
Continuous mass ablation of planets engulfed in stellar envelopes
-
RV curvature suggests distant giant around 51 Pegasi
An Outer Giant Planet or Brown Dwarf in the 51 Pegasi System?
-
6.2-Earth-mass planet found in habitable zone of active M-dwarf
Detection and Characterization of the Temperate Super-Earth Ross 318 b
-
Planet-hosting binaries show diverse Tc abundance trends
Chemical signatures of planetary systems in their host stars. Near-infrared spectroscopy of four planet-hosting wide binaries
-
Early Venus sunlight redistributed by season but orbit average stable
Seasonal Insolation Variability on Early Venus: Implications for Energy Budget
-
Alpha elements let giant planets form around iron-poor stars
A Uniform Determination of the Bulk Metallicities and Alpha Enrichments of Confirmed Exoplanet Systems with TRES
-
N2 levels warm or cool Earth-like planets depending on CO2
Revisiting the greenhouse effect of non-greenhouse gases in the atmospheres of Earth-like planets
-
Minerals can mimic the red edge biosignature for exoplanet life
Mineral False Positives in the Search for Exoplanet Surface Biosignatures
-
Two phase curve studies agree broadly but differ individually
Comparing Results from Two Uniform Phase Curve Surveys
-
Photoevaporation clears compact discs from inside out
The dispersal of compact protoplanetary discs
-
The paper presents practical techniques for implementing zero-order-hold transcriptions…
A practical guide to implementing zero-order-hold interplanetary trajectory legs
-
1882 comet fragments reveal pattern to predict future sungrazers
On the Problem of Prognostication of Bright Kreutz Sungrazers
-
15% lunar ejecta explain Moon crater asymmetry
Lunar ejecta as the missing piece to resolve the lunar cratering asymmetry
-
Formula gives eccentricity threshold for Neptune resonance capture
Numerical estimation of the capture ability of Neptunian mean motion resonances
-
Everyday cameras measure eclipse shadow band patterns
Image Processing Framework for Eclipse Shadow Band Analysis
-
Three-point inverse method matches densities for over half of fireballs
Consistency between dynamical modeling and photometrically derived masses of fireballs
-
Ice thickness variations on Enceladus create detectable magnetic signals
Exploring Enceladus's Interior Structure Using Electromagnetic Induction
-
Uruguay places 20 cameras to catch fireballs and recover meteorites
BOCOSUR: An all sky network for fireball detection in Uruguay
-
Swedish fireball originated from Apollo asteroid family
Observations of the 2023 February 27 fireball in northern Sweden using the auroral imaging system ALIS_4D
-
Earth foundation models advance from perception to discovery
Earth Science Foundation Models: From Perception to Reasoning and Discovery
-
New retrieval ties sub-Neptune spectra to magma composition
Coupling magma-ocean and atmospheres in spectral retrievals of sub-Neptunes
-
Bayesian method jointly infers brown dwarf map and geometry
Bayesian Doppler Imaging: Simultaneous Inference of Surface Maps and Geometric Parameters
-
MORIA pipeline cuts microlensing solutions in half with HST data
You Shall Not Pass (Without Modeling): High-Resolution Analysis of KMT-2019-BLG-0253 using MORIA
-
Ionization modeling aligns HAT-P-70b abundances closer to solar
HAT-P-70b through the Eyes of MAROON-X: Constraining Elemental Abundances of Metals and Insights on Atmosphere Dynamics
-
Refractory ratios control sub-Neptune atmospheric C/O and metal content
A New Global Chemical Equilibrium Code: Refractory Element Signatures in Super-Earths and Sub-Neptunes
-
Interstellar comet metals traced to carbonyl sublimation
Origin and evolution of NiI and FeI in the coma of the interstellar comet 3I/ATLAS throughout its trajectory
-
KMTNet data confirms three planets from 2023 microlensing survey
Mass Production of 2023 KMTNet Microlensing Planets. III: Three Planets from the Subprime Field
-
Energy model predicts ice on TRAPPIST-1 e and f
Exploring TRAPPIST-1 Climate States with an Energy Balance Model
-
Filter detects faint moving objects with low false positives
You Only Stack Once (YOSO): A Motion-Filtered, Deep-Learning Framework for Detecting Faint Moving Sources
-
ALMA modeling shows varied millimetre dust heights across discs
Diverse dust vertical height and settling strength conditions in protoplanetary discs
-
Gaia DR3 spectra sort 14042 asteroids into 13 classes
Taxonomy of 14042 asteroids from Gaia DR3 reflectance spectra
-
HST maps 1.1 sq deg of Galactic Bulge ahead of Roman exoplanet survey
An HST Wide Field Survey of the Galactic Bulge: Overview, Strategy, and First Results