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An imaged 15 MJup companion within a hierarchical quadruple system
DOI: 10.1051/0004-6361/202347044 Bibcode: 2023A&A...676L..10C

Henning, T.; Janson, M.; Langlois, M. +20 more

Context. Since 2019, the direct imaging B-star Exoplanet Abundance STudy (BEAST) at SPHERE@VLT has been scanning the surroundings of young B-type stars in order to ascertain the ultimate frontiers of giant planet formation. Recently, the 17−4+3 Myr HIP 81208 was found to host a close-in (∼50 au) brown dwarf and a wider (∼230 …

2023 Astronomy and Astrophysics
Gaia 5
A survey for variable young stars with small telescopes: VI - Analysis of the outbursting Be stars NSW 284, gaia 19eyy, and VES 263
DOI: 10.1093/mnras/stad407 Bibcode: 2023MNRAS.520.5413F

De, Kishalay; Hillenbrand, Lynne A.; Eislöffel, Jochen +44 more

This paper is one in a series reporting results from small telescope observations of variable young stars. Here, we study the repeating outbursts of three likely Be stars based on long-term optical, near-infrared, and mid-infrared photometry for all three objects, along with follow-up spectra for two of the three. The sources are characterized as …

2023 Monthly Notices of the Royal Astronomical Society
Gaia 5
Artificial neural network for star tracker centroid computation
DOI: 10.1016/j.asr.2022.11.023 Bibcode: 2023AdSpR..71.3917Z

Zapevalin, P. R.; Novoselov, A.; Zharov, V. E.

We propose a unique dataset with star images, their centroids, and a new centroid algorithm based on machine learning, that significantly improves star image centroid performance. The centroid of the star image is the subpixel coordinates on the image plane corresponding to the assumed point source of the light (a star). We have compiled and open-…

2023 Advances in Space Research
Gaia 5
White-light Superflare and Long-term Activity of the Nearby M7-type Binary EI Cnc Observed with GWAC System
DOI: 10.3847/1538-4357/ace59b Bibcode: 2023ApJ...954..142L

Wang, Jing; Liang, En-Wei; Wang, Xiang-Gao +14 more

Stellar white-light flares are believed to play an essential role in the physical and chemical properties of the atmosphere of the surrounding exoplanets. Here we report an optical monitoring campaign on the nearby flaring system EI Cnc carried out by the Ground-based Wide Angle Camera (GWAC) and its dedicated follow-up telescope. A superflare, co…

2023 The Astrophysical Journal
Gaia 5
Thermal emission from the hot Jupiter WASP-103 b in J and Ks bands
DOI: 10.1093/mnras/stad891 Bibcode: 2023MNRAS.522.1491S

Henning, Thomas; Zhao, Gang; Wang, Wei +9 more

Hot Jupiters, particularly those with temperature higher than 2000 K, are the best sample of planets that allow in-depth characterization of their atmospheres. We present here a thermal emission study of the ultrahot Jupiter WASP-103 b observed in two secondary eclipses with CFHT/WIRCam in J and Ks bands. By means of high precision diff…

2023 Monthly Notices of the Royal Astronomical Society
eHST 5
Exploring the potential of Twinkle to unveil the nature of LTT 1445 Ab
DOI: 10.1093/mnras/stad2822 Bibcode: 2023MNRAS.526.2251P

Gaudi, B. Scott; Wang, Ji; Phillips, Caprice L. +3 more

We explore the prospects for Twinkle to determine the atmospheric composition of the nearby terrestrial-like planet LTT 1445 Ab, including the possibility of detecting the potential biosignature ammonia (NH3). At a distance of 6.9 pc, this system is the second closest known transiting system and will be observed through transmission spe…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 5
Near-infrared evolution of the equatorial ring of SN 1987A
DOI: 10.1051/0004-6361/202245829 Bibcode: 2023A&A...675A.166K

Larsson, J.; Lundqvist, P.; Fransson, C. +4 more

We used adaptive optics imaging and integral field spectroscopy from the Very Large Telescope, together with images from the Hubble Space Telescope, to study the near-infrared (NIR) evolution of the equatorial ring (ER) of SN 1987A. We studied the NIR flux and morphology over time in order to lay the groundwork for James Webb Space Telescope obser…

2023 Astronomy and Astrophysics
eHST 5
CO enhancement by magnetohydrodynamic waves. Striations in the Polaris Flare
DOI: 10.1051/0004-6361/202345880 Bibcode: 2023A&A...673A..76S

Panopoulou, G. V.; Goldsmith, P. F.; Pelgrims, V. +4 more

Context. The formation of molecular gas in interstellar clouds is a slow process, but can be enhanced by gas compression. Magneto-hydrodynamic (MHD) waves can create compressed quasi-periodic linear structures, referred to as striations. Striations are observed at the column densities at which the transition from atomic to molecular gas takes plac…

2023 Astronomy and Astrophysics
Gaia Herschel 5
Spins and shapes of basaltic asteroids and the missing mantle problem
DOI: 10.1016/j.icarus.2023.115520 Bibcode: 2023Icar..39715520O

Hasegawa, Sunao; Oszkiewicz, Dagmara; Skiff, Brian A. +31 more

Basaltic V-type asteroids are common in the inner part of the Main Asteroid Belt and much less abundant in the mid and outer parts. They are of scientific interest because they sample crusts and mantles of theoretically plentiful differentiated planetesimals that existed in the Solar System four billion years ago. Some Solar System theories sugges…

2023 Icarus
Gaia 5
Unusual Hard X-Ray Flares Caught in NICER Monitoring of the Binary Supermassive Black Hole Candidate AT2019cuk/Tick Tock/SDSS J1430+2303
DOI: 10.3847/2041-8213/acbea9 Bibcode: 2023ApJ...945L..34M

Fabian, Andrew C.; Remillard, Ronald A.; Arzoumanian, Zaven +17 more

The nuclear transient AT2019cuk/Tick Tock/SDSS J1430+2303 has been suggested to harbor a supermassive black hole (SMBH) binary near coalescence. We report results from high-cadence NICER X-ray monitoring with multiple visits per day from 2022 January to August, as well as continued optical monitoring during the same time period. We find no evidenc…

2023 The Astrophysical Journal
XMM-Newton 5