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The NASA Exoplanet Archive and Exoplanet Follow-up Observing Program: Data, Tools, and Usage
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The NASA Exoplanet Archive and the Exoplanet Follow-up Observing Program service are two widely used resources for the exoplanet community. The NASA Exoplanet Archive provides a complete and accurate accounting of exoplanetary systems published by NASA missions and by the community in the refereed literature. In anticipation of continued exponential growth in the number of exoplanetary systems, and the increasing complexity in our characterization of these systems, the NASA Exoplanet Archive has restructured its primary tables and interfaces, as well as extending and standardizing their modes of access. The Exoplanet Follow-up Observing Program service provides the exoplanet community with a venue for coordinating and sharing follow-up and precursor data for exoplanets, their host stars, and stars that might eventually be targets for future planet searches, and recently reached one million files uploaded by the community. In this paper we describe the updates to our data holdings, functionality, accessibility, and tools, as well as future priorities for these two services.
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Cited by 21 Pith papers
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TOI-7169 b: A Hot Jupiter Transiting a Metal-Poor Star
TOI-7169 b is an inflated hot Jupiter (1.475 R_Jup, 0.41 M_Jup, P=3.44 d) around a spectroscopically confirmed metal-poor ([Fe/H]=-0.72), ancient (12.3 Gyr) thin-disk star.
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Stellar Observation Scheduling Optimization for Distributed Space Interferometry Missions
Multi-objective dynamic programming produces globally optimal Pareto fronts balancing ΔV and exoplanet yield for LEO nulling-interferometer observation schedules under realistic ConOps and observability constraints.
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HD 148797: A bright F-type star with two moderate-period low-density sub-Jovian planets. Compact multi-planet architectures are common in the Neptunian savanna
HD 148797 hosts two ~40 ME, ~8.3 RE, low-density savanna planets near a 1.619 period ratio whose anti-correlated TTVs yield masses and support compact multi-planet architectures as typical in the savanna.
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The GAPS Programme with HARPS-N at TNG LXXVII. Occurrence rates of small close-in planets in the presence of cold Jupiters
Close-in small planets occur at ~5–16% around cold-Jupiter hosts, with no strong overall correlation at average stellar mass/metallicity, but elevated rates in dynamically stable inner regions.
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The Longest-period Young Transiting Exoplanets. A Duo of Puffy Giants inside a Debris Disk
HD 114082 hosts two puffy, moderate-to-low-mass giants on nearly circular, coplanar, near-resonant orbits of 225.55 and ~314 days, the longest-period young transiting exoplanets known.
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On the Eccentricity Distribution and Tidal Evolution of Transiting Brown Dwarfs
Short-period (P<16 d) transiting brown dwarfs are low-eccentricity while longer-period ones are more excited; assuming a shared primordial Beta distribution, tidal evolution constrains Q_BD ≈ 10^{7.1–8.1}.
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Chemical Abundances Shape History (CASH). I. A Link between Giant Planets Orbital Periods and Host Stellar C/O Ratios
Higher host-star C/O ratios correlate with longer orbital periods for giant planets, based on spectra from 598 stars and supported by pebble-formation models.
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High five from ASTEP: Three validated planets and two eclipsing binaries in a diverse set of long-period candidates
Three TESS long-period candidates (TOI-4507b, TOI-3457b, TOI-707b) are validated as planets and two (TOI-2404, TOI-4404) are identified as eclipsing binaries.
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An Increase in the Galactic Planet Host Fraction Fails to Reproduce the Galactic Height Trend in Planet Occurrence
Time-dependent increases in the planet host fraction cannot reproduce the steep decline in small-planet occurrence with Galactic height seen by Kepler and K2.
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Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters
Inflated hot Jupiters with outer-envelope heat deposition have suppressed deep convection and surface magnetic fields at or below Jupiter's, which may explain the absence of detected coherent radio emission.
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The GAPS Programme with HARPS-N at TNG LXXVII. Occurrence rates of small close-in planets in the presence of cold Jupiters
Occurrence rates of hot/warm/cool Neptunes and Super-Earths around cold-Jupiter hosts are ~5–16%, higher when the outer giant leaves a stable inner zone, with no strong ISP–CJ correlation at average metallicity.
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Determining the Host Stars of Planets in Binary Star Systems with Asterodensity Profiling: Investigating the Canonical Radius Gap
Probabilistic host-star assignments via asterodensity profiling suggest the exoplanet radius gap is less empty in binary systems once possible circumsecondary planets are included.
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An Aligned Sub-Neptune Revealed with MAROON-X and a Tendency Towards Alignment for Small Planets
The sub-Neptune TOI-1759A b has sky-projected obliquity |λ|=4±18 deg, and small exoplanets with measured obliquities tend toward alignment, especially in compact systems.
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exoatlas: friendly Python code for exoplanet populations
The exoatlas package provides a Python interface for retrieving, deriving, and visualizing exoplanet and Solar System populations.
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The TESS Grand Unified Hot Jupiter Survey. III. Thirty More Giant Planets
Thirty TESS-discovered hot Jupiters around bright FGK stars are validated and characterized, including two with measured non-zero eccentricities.
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TOI-159 b: an eccentric hot-Jupiter planet around a young, pulsating $\gamma$ Doradus star
TOI-159 b is confirmed as the hottest known eccentric hot Jupiter (e = 0.24) with a 13-sigma Keplerian detection around a young gamma Doradus star, including a preliminary low-resolution transmission spectrum.
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The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0
Planet Nine, if it exists, is most likely a mini-Neptune with a radius of 2 to 2.6 Earth radii and an H-He envelope of 0.6 to 3.5 percent by mass, based on a sample of cool exoplanets.
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TOI-1259Ab: A Warm Jupiter Orbiting a K-dwarf White-Dwarf Binary is on a Well-aligned Orbit
The sky-projected obliquity of TOI-1259Ab is measured as λ = 6+21−22° and the true 3D obliquity as ψ = 24+14−12° (ψ < 48° at 95 % confidence), indicating a well-aligned orbit too wide for tidal realignment.
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CARMApy: An Open-Source Python Framework for Simulating Microphysical Clouds in Planetary Atmospheres
CARMApy provides a Python interface to the ExoCARMA microphysics code, enabling simulation of cloud particle size distributions and rates in exoplanet atmospheres with claimed consistency to prior versions and speed g...
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Comparing Results from Two Uniform Phase Curve Surveys
Comparison of two exoplanet phase curve surveys shows population-level consistency but individual variations, plus a Kepler's law inconsistency in archival parameters that warrants routine verification.
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Predictions of Transiting Exoplanet Confirmations from Rubin LSST Surveys
Simulations predict very limited transiting exoplanet confirmations from LSST due to observing cadence constraints, with only a few possible in DDF for hot planets on M dwarfs.
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