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Spotted eclipsing binary KIC 7023917 with δ-Scuti pulsations
DOI: 10.31577/caosp.2024.54.2.194 Bibcode: 2024CoSka..54b.194G

Parimucha, Š.; Gajdoš, P.; Kamenec, M.

Eclipsing binary KIC 7023917 is one of nearly three thousand other binaries in the well-known Kepler Eclipsing Binary Catalog. However, it has some uncommon features. We focused on this system because we detected fast anti-correlated changes on the O-C diagram which could suggest the presence of apsidal motion. However, these changes are very fast…

2024 Contributions of the Astronomical Observatory Skalnate Pleso
Gaia 0
Investigation of three events of solar parameters and Interplanetary Coronal Mass ejections during the maximum phase of solar cycle 24
Bibcode: 2024BlgAJ..41...27D

Dhaiya, M. S.; Bidhu, S. S.; Sobia, A. Iren

This paper analyzes the Three events of Solar Parameters and Interplanetary Coronal Mass Ejections in the maximum phase of Solar Cycle 24 and focuses on the magnetic activity of interplanetary coronal mass ejection during the solar cycle 24. We investigate the magnetic field magnitude (B), Proton temperature (Tp), Proton density (Np). From this st…

2024 Bulgarian Astronomical Journal
SOHO 0
X-ray Observations of the Very-Faint X-ray Transient XMMSL1 J171900.4-353217: A New Candidate Neutron Star Low-Mass X-ray Binary
DOI: 10.48550/arXiv.2409.19649 Bibcode: 2024RMxAA..60..403A

Degenaar, N.; Wijnands, R.; Armas Padilla, M. +1 more

XMMSL1 J171900.4–353217 is a very-faint X-ray transient that was discovered in 2010 March when it exhibited an outburst. We report on 7 observations, obtained with the X-Ray Telescope (XRT) aboard the Neil Gehrels Swift Observatory between 2010 May and October. By fitting a single absorbed power-law model to the XRT spectra, we infer power-law ind…

2024 Revista Mexicana de Astronomia y Astrofisica
INTEGRAL XMM-Newton 0
Extreme-emission-line galaxies in the MUSE Hubble Ultra Deep Field Survey
DOI: 10.1051/0004-6361/202348185 Bibcode: 2024A&A...688A..28D

Vílchez, J. M.; Iglesias-Páramo, J.; Arroyo-Polonio, A. +1 more


Aims: We aim to apply a methodology to build a sample of extreme-emission-line galaxies (EELGs) using integral field spectroscopy data. In this work, we followed the spectroscopic criteria corresponding to EELG selection and used the MUSE Hubble Ultra-Deep Field Survey, which includes the deepest spectroscopic survey ever performed.
Meth…

2024 Astronomy and Astrophysics
eHST JWST 0
Prediction of Geoeffective CMEs Using SOHO Images and Deep Learning
DOI: 10.1007/s11207-024-02385-w Bibcode: 2024SoPh..299..159A

Jing, Ju; Wang, Haimin; Yurchyshyn, Vasyl +6 more

The application of machine learning to the study of coronal mass ejections (CMEs) and their impacts on Earth has seen significant growth recently. Understanding and forecasting CME geoeffectiveness are crucial for protecting infrastructure in space and ensuring the resilience of technological systems on Earth. Here we present GeoCME, a deep-learni…

2024 Solar Physics
SOHO 0
Double-edged Sword: The Influence of Tidal Interaction on Stellar Activity in Binaries
DOI: 10.3847/1538-4357/ad8eb9 Bibcode: 2024ApJ...976..243D

Fang, Min; Wang, Song; Han, Henggeng +4 more

Using the LAMOST DR7 low-resolution spectra, we carried out a systematic study of stellar chromospheric activity in both single and binary stars. We constructed a binary sample and a single-star sample, mainly using the binary belt and the main sequence in the Hertzsprung–Russell diagram, respectively. By comparing the S indices between single and…

2024 The Astrophysical Journal
Gaia 0
SOHO SWAN Lyα Models Supporting LRO LAMP: 2008–2023
DOI: 10.3847/PSJ/ad7502 Bibcode: 2024PSJ.....5..210P

Pryor, Wayne R.; Gladstone, G. Randall; Quémerais, Eric +5 more

The Lunar Reconnaissance Orbiter Lyman-Alpha Mapping Project (LAMP) has been mapping the Moon since its launch in 2009. Faint ultraviolet illumination of the lunar dark side includes light from stars and from hydrogen Lyα emissions, mostly attributed to sunlight scattered by hydrogen atoms near the Sun with a smaller contribution from the whole Ga…

2024 The Planetary Science Journal
SOHO 0
Spectroscopic and Photometric Study of the S-type Mira V667 Cassiopeiae and the Carbon Star OR Cephei
DOI: 10.48550/arXiv.2407.01719 Bibcode: 2024JAVSO..52...96B

Boyd, D.

We report on spectroscopic and photometric observations of the S-type Mira V667 Cas and the carbon star Mira OR Cep recorded during one pulsation cycle of each star in 2022. Spectra are calibrated in absolute flux using concurrent photometry. We present measurements of V and Ic magnitudes and V-Ic color index, classify spectra in the revised MK sy…

2024 Journal of the American Association of Variable Star Observers (JAAVSO)
Gaia 0
Precise measurement of pion-bump structure using future MeV gamma-ray detectors
DOI: 10.1103/PhysRevD.110.063026 Bibcode: 2024PhRvD.110f3026L

Liu, Jiahao; Liu, Bing; Yang, Ruizhi

The pion-bump structure in the γ-ray spectrum is a direct proof for the hadronic origin of the γ rays, and thus the decisive evidence for the acceleration of hadronic cosmic…

2024 Physical Review D
INTEGRAL 0
The Goldstone Apple Valley Radio Telescope (GAVRT) Search for Extra Terrestrial Intelligence (SETI)
DOI: 10.1088/1538-3873/ad2f4f Bibcode: 2024PASP..136d4502G

Gorjian, Varoujan; Lazio, Joseph; Levin, Steven +6 more

This paper reports the results from a student-led Search for Extraterrestrial Intelligence (SETI), also known as technosignatures, targeting the plane of the Milky Way as a part of the Goldstone Apple Valley Radio Telescope (GAVRT) collaboration between the Lewis Center for Educational Research (LCER) and the Jet Propulsion Laboratory. Students as…

2024 Publications of the Astronomical Society of the Pacific
Gaia 0