Publicaciones

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  • The eccentricity distribution of warm sub-Saturns in TESS
    We present the eccentricity distribution of warm sub-Saturns (4–8 $R_{\rm{\oplus }}$, 8–200 d periods) as derived from an analysis of transit light curves from NASA's Transiting Exoplanet Survey Satellite (TESS) mission. We use the 'photoeccentric' effect to constrain the eccentricities of 76 planets, comprising 60 and 16 from single and
    Fairnington, Tyler R. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Systematic Reanalysis of KMTNet Microlensing Events. II. Two New Planets in Giant-source Events
    In this work, we continue to apply the updated KMTNet tender-love care photometric pipeline to historical microlensing events. We apply the pipeline to a subsample of events from the KMTNet database, which we refer to as the giant source sample. Leveraging the improved photometric data, we conduct a systematic search for anomalies within this
    Yang, Hongjing et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Small-scale dynamic phenomena associated with interacting fan-spine topologies: Quiet-Sun Ellerman bombs, UV brightenings, and chromospheric inverted-Y-shaped jets
    Context. Quiet-Sun Ellerman bombs (QSEBs) are small-scale magnetic reconnection events in the lower solar atmosphere. Sometimes, they exhibit transition region counterparts, known as ultraviolet (UV) brightenings. Magnetic field extrapolations suggest that QSEBs can occur at various locations of a fan-spine topology, with UV brightening occurring
    Bhatnagar, Aditi et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Revisiting the Li Abundances of Stars with and without Detected Planets from High-resolution Spectroscopy
    Whether the presence of planets affects the lithium (Li) abundance of their host stars is still an open question. To investigate the difference in the Li abundance between planet-host stars (HSs) and isolated stars (ISs) with no detected planets, we analyze a large sample of stars with temperatures ranging from 4600 to 6600 K and metallicity
    Qin, Jinxiao et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Relatively young thick disks in star-forming late-type galaxies
    Aims. We trace the evolution of eight edge-on star-forming disk galaxies by analyzing stellar population properties of their thin and thick disks. These galaxies have relatively low stellar masses (4 × 10 9–6 × 10 10 M ⊙). Methods. We used Multi-Unit Spectroscopic Explorer (MUSE) observations and a full-spectrum fitting to produce spatially
    Sattler, Natascha et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Quiet Sun Magnetism from ViSP Data Multiline Inversions Around 630.1 nm
    Quiet Sun magnetism plays an important role in the global energy balance of the solar atmosphere. The study of the magnetism of the quiet Sun has been a major effort in the last decades, and, as a result, very important advances in our knowledge have been achieved. The recent commissioning of the Daniel K. Inouye Solar Telescope, the largest ground
    Trelles Arjona, J. C.

    Fecha de publicación:

    6
    2025
    Número de citas
    0