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Astronomy from the Moon
CRAWFORD I. & ZARNECKI J.
Astron. & Geophysics
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Refining the properties of the TOI-178 system with CHEOPS and TESS
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Astron. & Astrophys.
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Gaia Astrometry and MIKE+PFS Doppler Data Joint Analysis Reveals that HD 175167b is a Massive Cold Jupiter
GAN T.
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paper arxiv
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Long-term Orbital Period Variation of Hot Jupiters from Transiting Time Analysis using TESS Survey Data
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ApJ Suppl.
, accepted
arxiv
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3D Global Simulations of Accretion onto Gap-opening Planets: Implications for Circumplanetary Disc Structures and Accretion Rates
LI Y.-P., CHEN Y.-X. & LIN D.
MNRAS
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Evidence that the Occurrence Rate of Hot Jupiters around Sun-like Stars Decreases with Stellar Age
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The abundance of dark matter haloes down to Earth mass
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MNRAS
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arxiv
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Breaking up with the continuous exoplanet mass-radius relation
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Opn J. of Astrophys.
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arxiv
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Stability and detectability of exomoons orbiting HIP 41378 f, a temperate Jovian planet with an anomalously low apparent density
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A roadmap to the efficient and robust characterization of temperate terrestrial planet atmospheres with JWST
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arxiv
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The period bouncer system SDSS J105754.25+275947.5: first radial velocity study
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MNRAS
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Time-resolved transmission spectroscopy of the ultra-hot Jupiter WASP-189 b
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Early Planet Formation in Embedded Disks (eDisk) XII: Accretion streamers, protoplanetary disk, and outflow in the Class I source Oph IRS63
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ApJ
, accepted
arxiv
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The Potential of Detecting Nearby Terrestrial Planets in the HZ with Different Methods
HAO Q., ZHOU Sh. & LIU H.
PASP
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Separated twins or just siblings? A multi-planet system around an M dwarf including a cool sub-Neptune
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ApJ. Letters
, accepted
arxiv
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Predicting the phase behaviors of superionic water at planetary conditions
CHENG B., BETHKENHAGEN M., PICKARD Ch. & HAMEL S.
arxiv
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Material Properties for the Interiors of Massive Giant Planets and Brown Dwarfs
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Probing reflection from aerosols with the near-infrared dayside spectrum of WASP-80b
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ApJ. Letters
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Detecting Technosignatures from Earth-scale Civilizations
ASHTARI R.
ApJ
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A Search for Technosignatures Around 11,680 Stars with the Green Bank Telescope at 1.15-1.73 GHz
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