Search Publications

A Classification Catalog of Periodic Variable Stars for LAMOST DR9 Based on Machine Learning
DOI: 10.3847/1538-4365/ad3452 Bibcode: 2024ApJS..272....1Q

Mei, Ying; Wang, Feng; Deng, Hui +4 more

Identifying and classifying variable stars is essential to time-domain astronomy. The Large Area Multi-Object Fiber Optic Spectroscopic Telescope (LAMOST) acquired a large amount of spectral data. However, there is no corresponding variable source-related information in the data, constraining LAMOST data utilization for scientific research. In thi…

2024 The Astrophysical Journal Supplement Series
Gaia 2
First spectroscopic investigation of anomalous Cepheid variables
DOI: 10.1051/0004-6361/202347991 Bibcode: 2024A&A...682A...1R

Ripepi, V.; Molinaro, R.; Marconi, M. +12 more

Context. Anomalous Cepheids (ACEPs) are intermediate-mass metal-poor pulsators that are mostly discovered in dwarf galaxies of the Local Group. However, recent Galactic surveys, including the Gaia Data Release 3, found a few hundred ACEPs in the Milky Way. Their origin is only poorly understood.
Aims: We aim to investigate the origin and evol…

2024 Astronomy and Astrophysics
Gaia 2
The Complex Star Formation History of the Halo of NGC 5128 (Cen A)
DOI: 10.3847/1538-4357/ad57c0 Bibcode: 2024ApJ...972...47A

Javadi, Atefeh; Saremi, Elham; van Loon, Jacco Th. +6 more

NGC 5128 (Cen A) is the nearest giant elliptical galaxy and one of the brightest extragalactic radio sources in the sky, boasting a prominent dust lane and jets emanating from its nuclear supermassive black hole. In this paper, we construct the star formation history (SFH) of two small fields in the halo of NGC 5128: a northeastern field (Field 1)…

2024 The Astrophysical Journal
Gaia eHST 2
The TESS-SPOC FFI target sample explored with Gaia
DOI: 10.1093/mnras/stae616 Bibcode: 2024MNRAS.529.1802D

Bayliss, Daniel; Armstrong, David J.; Rodel, Toby +2 more

The Transiting Exoplanet Survey Satellite (TESS) mission has provided the community with high-precision times-series photometry for ~2.8 million stars across the entire sky via the full frame image (FFI) light curves produced by the TESS Science Processing Operations Center (SPOC). This set of light curves is an extremely valuable resource for the…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
X-raying the ζ Tau binary system
DOI: 10.1051/0004-6361/202449737 Bibcode: 2024A&A...688A.181N

Smith, Myron A.; Nazé, Yaël; Rauw, Gregor +2 more

Context. The Be star ζ Tau was recently reported to be a γ Cas analog; that is, it displays an atypical (bright and hard) X-ray emission. The origin of these X-rays remains debated.
Aims: The first X-ray observations indicated a very large absorption of the hot plasma component (NH ~ 1023 cm−2). This is most p…

2024 Astronomy and Astrophysics
XMM-Newton 2
The enigmatic multiple star VV Ori
DOI: 10.1093/mnras/stad3586 Bibcode: 2024MNRAS.527.6389B

Blackford, Mark G.; Southworth, John; Budding, Edwin +6 more

New photometry, including TESS data, have been combined with recent spectroscopic observations of the Orion Ib pulsating triple-star system VV Ori. This yields a revised set of absolute parameters with increased precision. Two different programmes were utilized for the light-curve analysis, with results in predictably close agreement. The agreemen…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
Influence of the Jovian Current Sheet Models on the Mapping of the UV Auroral Footprints of Io, Europa, and Ganymede
DOI: 10.1029/2023JA032041 Bibcode: 2024JGRA..12932041R

André, N.; Hue, V.; Rabia, J. +4 more

The in situ characterization of moon-magnetosphere interactions at Jupiter and the mapping of moon auroral footpaths require accurate global models of the magnetospheric magnetic field. In this study, we compare the ability of two widely-used current sheet models, Khurana-2005 (KK2005) and Connerney-2020 (CON2020) combined with the most recent int…

2024 Journal of Geophysical Research (Space Physics)
Ulysses 2
Euclid: High-precision imaging astrometry and photometry from Early Release Observations: I. Internal kinematics of NGC6397 by combining Euclid and Gaia data
DOI: 10.1051/0004-6361/202452295 Bibcode: 2024A&A...692A..96L

Altieri, B.; Cimatti, A.; Baccigalupi, C. +175 more

The instruments at the focus of the Euclid space observatory offer superb, diffraction-limited imaging over an unprecedented (from space) wide field of view of 0.57 deg2. This exquisite image quality has the potential to produce high-precision astrometry for point sources once the undersampling of Euclid's cameras is taken into account …

2024 Astronomy and Astrophysics
Gaia EUCLID 2
The GAPS programme at TNG. LVII. TOI-5076b: A warm sub-Neptune planet orbiting a thin-to-thick-disk transition star in a wide binary system
DOI: 10.1051/0004-6361/202349082 Bibcode: 2024A&A...687A.226M

Scandariato, G.; Pagano, I.; Winn, J. N. +36 more


Aims: We report the confirmation of a new transiting exoplanet orbiting the star TOI-5076.
Methods: We present our vetting procedure and follow-up observations which led to the confirmation of the exoplanet TOI-5076b. In particular, we employed high-precision TESS photometry, high-angular-resolution imaging from several telescopes, and h…

2024 Astronomy and Astrophysics
Gaia 2
Gaia23bab: A New EXor
DOI: 10.3847/1538-4357/ad39e2 Bibcode: 2024ApJ...967...41G

Ábrahám, P.; Nagy, Z.; Schisano, E. +11 more

On 2023 March 6, the Gaia telescope alerted a 2 mag burst from Gaia23bab, a young stellar object in the Galactic plane. We observed Gaia23bab with the Large Binocular Telescope obtaining optical and near-infrared spectra close in time to the peak of the burst, and collected all public multiband photometry to reconstruct the historical light curve.…

2024 The Astrophysical Journal
Gaia Herschel 2