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Every paper Pith has read. Search by title, abstract, or pith.
717 papers in astro-ph.EP · page 2
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FastChem 4 stabilizes chemistry calculations for carbon-rich cases
FastChem 4: New chemical elements and improved convergence behaviour
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Strangelets form ultra-compact objects of 0.01-0.1 solar masses
Sub-stellar Strange Quark Matter Objects: Predicting a New Class of Highly-Compact Candidates
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Kinematics sharpen ML predictions of stellar C
Inferring stellar metallicity and elemental abundances from kinematic and spectroscopic data using machine learning -- Implications for exoplanet host stars
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Acetylene-water flux ratio traces inner-disk elemental makeup
Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties
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Solar C/O explains acetylene fluxes in T Tauri disks
Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties
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Hycean model fits K2-18b spectra using only H2
A Hycean Interpretation of K2-18b Supported by Photochemical Atmospheric Compositional
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DTC Starlink satellites brighter in eclipse than sunlight
A reversed solar illumination dependence of unintended emission from Starlink Direct-to-Cell satellites at 72-234 MHz with the EDA2
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Alpha-slope test on TNO data uncovers calibration offsets
A Framework for Applying the Loeb-Turner $\alpha$-Slope Test to Archival Photometry of Trans-Neptunian Objects
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Systematic search finds 7 new microlensing planets in 2021 data
Systematic KMTNet Planetary Anomaly Search. XIII. Complete Sample of 2021 Prime Field Planets
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Pneumatic CO2 drill achieves 74-360 MJ/m3 in Mars rock tests
Evaluation and Modeling of Pneumatic Percussive Drill for Martian Subsurface Access
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First biosignature likely from detectable outlier
The First Remotely Detected Biosignature May Not Be the Most Common: Implications for JWST and HWO
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RV reanalysis cuts GJ 3378b mass to 2.3 Earth masses and period to 21.45 days
A Revised Mass and Period for the Habitable Zone super-Earth GJ 3378b: A Planet Straddling the Cosmic Shoreline
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Stars pass within 1 parsec of Sun every 95,000 years on average
Stellar encounters in the solar neighbourhood and the special case of GJ~710
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Rotational broadening hides exoplanet reflection signals
Spinning out of focus: The challenge of rotational line broadening in exoplanet reflection spectroscopy
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Hybrid model forecasts MeV electrons at average R2 of 0.9
Forecasting megaelectron-volt electron flux in the Earth's outer radiation belt using supervised machine learning algorithms and a timeseries foundation model
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ILMT detects 152 asteroids and one new transient
Performance of the 4-m International Liquid Mirror Telescope tested in two fields at high and low ecliptic and galactic latitudes
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Bacterial spores could survive Mars-to-Earth trip in one year
Could life have been transferred from Mars to Earth? Laboratory and computational simulations of Martian ejecta
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Juno shows Jupiter north pole 6-7 K warmer than equator
Juno Microwave Radiometer Observations Reveal A Warmer Polar Atmosphere on Jupiter
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Abiotic uncertainties block clear biosignature detection on Enceladus
A framework for evaluating biosignature potential against the abiotic baseline on ocean worlds
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C/O ratio and SiH4 mark ice line origins in sub-Neptune atmospheres
The Role of Formation Location in Shaping Sulfur-, Nitrogen-, and Carbon-Bearing Species in Super-Earth and Sub-Neptune Atmospheres
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Common formulas underestimate disk millimeter emission by 10-15%
Millimeter dust continuum and polarization in protoplanetary disks with scattering: A slab model
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JWST spectrum of LTT 1445 A b shows no atmospheric features
JWST COMPASS Program: The 3--5$\mu$m transmission spectrum of LTT 1445 A b
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This paper introduces a Bayesian analysis framework that uses self-consistent climate…
A Climate-Constrained Bayesian Inverse Method for JWST Rocky Exoplanet Eclipse Spectra: A Case Study of LTT 1445A b
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Cores let giant planets survive close tidal encounters
Where Do Hot Jupiters Come From? Revisiting Tidal Disruption and Ejection in High-Eccentricity Migration
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Proto-satellite collisions form new moons
Dynamical Evolution of V-Shaped Collision Debris
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Debris from proto-satellite collisions reaccretes near impact site
Dynamical Evolution of V-Shaped Collision Debris
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Outgassing sustains thin atmospheres on TRAPPIST-1 planets
Coupled Photochemical-Climate Modeling of Plausible Tenuous Outgassed Atmospheres on the TRAPPIST-1 Planets
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Pulsar planet could emit detectable radio waves
Planets in Pulsar Winds
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Calibrated GWs shrink Moon elastic errors tenfold
Gravitational-wave Tomography of the Moon: Constraining Lunar Structure with Calibrated Gravitational Waves
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Calibrated GWs cut Moon elastic errors by factor of ten
Gravitational-wave Tomography of the Moon: Constraining Lunar Structure with Calibrated Gravitational Waves
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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
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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
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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
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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
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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
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Catalog supplies ages for 659 HWO stars but covers only 25 percent
The HAges Catalog: Stellar Ages for High Priority HWO Target Stars
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18 hot Ariel stars receive uniform parameters
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample
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Eta Tel disk gas has low C/O like solar system comets
Revisiting the ultraviolet spectroscopy of the eta Tel edge-on debris disk
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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
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Capture can stabilize pulsar planets at low eccentricity
Formation of stable exoplanetary systems around pulsars by capture: An exercise in computational classical mechanics
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Asteroid dust flux matches models at inner planets
Modeling and Analysis of Main-Belt Asteroidal Dust Flux and Velocity Distribution at Inner Planets
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1923 Newtonian estimate gave 49 hours to the Moon
On the Anticipation of Lunar Travel in the Early 20th Century: A Pedagogical Exercise
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W-Net spots asteroids in TESS data regardless of path
Trajectory-Agnostic Asteroid Detection in TESS with Deep Learning
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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
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Molten cores turn asteroid collisions into iron-rich rubble piles
Reaccumulation process after a catastrophic disruption event on a differentiated asteroid
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Tidal models fix rotation states for six Kepler exoplanets
Simulation of the spin evolution of some selected exoplanets and inferences on their climate
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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
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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
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Engulfed planets dissolve steadily inside stars
Continuous mass ablation of planets engulfed in stellar envelopes
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RV curvature suggests distant giant around 51 Pegasi
An Outer Giant Planet or Brown Dwarf in the 51 Pegasi System?