Prépublication
· 2026 arXiv
EN
RTL repair benchmarks should measure whether a model can fix broken RTL given a specification. To this end, we construct and hash-bind RTLRepairDataset, 5,784 (broken, fixed) training pairs; RTLRepairBench, 459 held-out cases with 374 syntactic and 85 behavior...
Yeyin Eva Zhu, Rishabh Ranawat
#cs.AI
Prépublication
· 2026 arXiv
EN
Simulation is a powerful tool for robotics, but building diverse, simulation-ready scenes at scale remains difficult. Reconstructing scenes from single images is a promising alternative, but visual similarity alone is insufficient: objects must also be recover...
Rundong Luo, Yunong Liu et al.
#cs.RO
Prépublication
· 2026 arXiv
EN
Small planets transiting the nearest M dwarfs are the terrestrial planets most accessible to detailed characterisation. We report a sub-Earth-sized transiting planet candidate in the wide (17.6") M-dwarf binary GJ 774 at 12.86 pc, most likely orbiting the M2.5...
Jaden Tripp
#astro-ph.EP
Prépublication
· 2026 arXiv
EN
We first derived the formulae of recursive reduction and dlog-form differential equations for arbitrary tree-level cosmological correlator, taking the external relations of massless bulk propagators into consideration. The differential equations could be syste...
Jiaqi Chen, Yi-Xiao Tao et al.
#hep-ph
Prépublication
· 2026 arXiv
EN
The TESS mission is designed to survey the entire sky to find planets most amenable to follow-up observations, and transit searches have therefore focused specifically on bright targets. Faint stars ($T_{mag}>13.5$) have not been systematically searched for pl...
Matthew Lastovka, Thomas Barclay et al.
#astro-ph.EP
Prépublication
· 2026 arXiv
EN
Precision spectroscopy underpins quantum sensing, atomic timekeeping, and the search for terrestrial-mass exoplanets. Finding an Earth-Sun analog requires fractional splitting of spectral features that rivals the precision of the best laboratory spectroscopy....
Connor Fredrick, Ryan K. Cole et al.
#astro-ph.IM
Prépublication
· 2026 arXiv
EN
The NSF-DOE Vera C. Rubin Observatory will complete its ten-year Legacy Survey of Space and Time (LSST) in the mid-2030s. Its 8.4 m aperture and 9.6 square degree field of view give it an étendue unmatched by any facility planned for that era. The Rubin 2036:...
Andrés Alejandro Plazas Malagón, Steve Allen et al.
#astro-ph.IM
Prépublication
· 2026 arXiv
EN
We present a technique using integral-field spectroscopy to kinematically isolate intracluster light (ICL) from the brightest cluster galaxy (BCG), enabling insights into their contrasting stellar populations and the inner dark matter halo profile. Applying th...
Callum Bellhouse, Steven Bamford et al.
#astro-ph.GA
Prépublication
· 2026 arXiv
EN
Asteroseismology relies on disk-integrated photometry or radial velocities, in which geometric cancellation suppresses modes of high spherical degree ($l\geq4$). Observations are thus limited to deeply penetrating, low-degree modes, leaving the outer envelope...
Marcus L. Marcussen, Mikkel N. Lund
#astro-ph.SR
Document numérisé
· 1642 Gallica (BnF)
FR
Document numérisé par la Bibliothèque nationale de France, publié en 1642. Thème : géographie. Consultable en ligne sur Gallica.
Bibliothèque nationale de France
#Géographie
Document numérisé
· 1644 Gallica (BnF)
FR
Document numérisé par la Bibliothèque nationale de France, publié en 1644. Thème : géographie. Consultable en ligne sur Gallica.
Bibliothèque nationale de France
#Géographie
Document numérisé
· 1644 Gallica (BnF)
FR
Document numérisé par la Bibliothèque nationale de France, publié en 1644. Thème : géographie. Consultable en ligne sur Gallica.
Bibliothèque nationale de France
#Géographie