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TESS discovery of a super-Earth and two sub-Neptunes orbiting the bright, nearby, Sun-like star HD 22946
DOI: 10.1051/0004-6361/202243565 Bibcode: 2022A&A...668A..85C

Kostov, Veselin B.; Barclay, Thomas; Lester, Kathryn V. +51 more

We report the Transiting Exoplanet Survey Satellite (TESS) discovery of a three-planet system around the bright Sun-like star HD 22946 (V ≈ 8.3 mag), also known as TIC 100990000, located 63 pc from Earth. The system was observed by TESS in Sectors 3, 4, 30, and 31 and two planet candidates, labeled TESS Objects of Interest (TOIs) 411.01 (planet c)…

2022 Astronomy and Astrophysics
Gaia 4
The Principal Astrophysical Parameters of the Open Clusters Gulliver 18 and Gulliver 58 Determined Using Gaia EDR3 Data
DOI: 10.22201/ia.01851101p.2022.58.02.17 Bibcode: 2022RMxAA..58..387T

Tadross, A. L.; Elhosseiny, E. G.

A photometric and astrometric study of the two open star clusters Gulliver 18 and Gulliver 58 was carried out for the first time using the early third data release of the Gaia space observatory (Gaia-EDR3). By studying the proper motions, parallaxes, and color-magnitude diagrams of the two clusters, we determined their actual cluster membership. T…

2022 Revista Mexicana de Astronomia y Astrofisica
Gaia 4
Distances to Local Group Galaxies via Population II, Stellar Distance Indicators. I. The Sculptor Dwarf Spheroidal
DOI: 10.3847/1538-4357/ac6fe0 Bibcode: 2022ApJ...935...34T

Madore, Barry F.; Freedman, Wendy L.; Cerny, William +5 more

We determine the distance to the Sculptor Dwarf Spheroidal via three Population II stellar distance indicators: (a) the Tip of the Red Giant Branch (TRGB), (b) RR Lyrae variables (RRLs), and (c) the ridgeline of the blue horizontal branch (HB). High signal-to-noise, wide-field VI imaging that covers an area $48^{\prime} \,\times \,48^{\prime} $ an…

2022 The Astrophysical Journal
Gaia eHST 4
An empirical model of the current sheet in Jupiter's magnetosphere
DOI: 10.1016/j.pss.2021.105395 Bibcode: 2022P&SS..21105395W

Zhang, Lei; Wang, Jian-zhao; Huo, Zhuo-xi

Based on the Magnetometer data from the Galileo and Juno mission, we construct an analytical ring current model that provides the azimuthal current (Jφ) distribution in radial (ρ), height (z), and local time (LT) dimensions. After binning the in-situ magnetic field data into 2 RJ × 2 RJ × 3 h (RJ is the …

2022 Planetary and Space Science
Ulysses 4
Cometary plasma science
DOI: 10.1007/s10686-021-09783-z Bibcode: 2022ExA....54.1129G

Gunell, H.; Glassmeier, K. -H.; Andre, N. +27 more

Comets hold the key to the understanding of our Solar System, its formation and its evolution, and to the fundamental plasma processes at work both in it and beyond it. A comet nucleus emits gas as it is heated by the sunlight. The gas forms the coma, where it is ionised, becomes a plasma, and eventually interacts with the solar wind. Besides thes…

2022 Experimental Astronomy
Rosetta 4
A compact symmetric ejection from the low mass AGN in the LINER galaxy NGC 4293
DOI: 10.1093/mnras/stac2990 Bibcode: 2022MNRAS.517.4959Y

Yang, Xiaolong; Wang, Ruiling; Guo, Quan

We conducted a Very Long Baseline Array (VLBA) observation of the low mass active galactic nucleus (AGN) in galaxy NGC 4293 (z = 0.003). The object is associated with a low-ionization nuclear emission-line region (LINER). Its black hole mass is estimated as ~105 or ${\sim}10^7 \, \mathrm{M}_\odot$. The VLBA 1.5 GHz image shows an invers…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 4
A cosmological distance measure using radio-loud quasars
DOI: 10.1093/mnras/stac1451 Bibcode: 2022MNRAS.515.1358H

Huang, L.; Chang, Z. X.

We use the X-ray luminosity relation of radio-loud quasars (RLQs) to measure these luminosity distances as well as estimate cosmological parameters. We adopt four parametric models of X-ray luminosity to test luminosity correlation for RLQs and radio-intermediate quasars (RIQs) and give these cosmological distances. By Bayesian information criteri…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4
TIC 257060897b: An inflated, low-density, hot-Jupiter transiting a rapidly evolving subgiant star
DOI: 10.1093/mnras/stab2923 Bibcode: 2022MNRAS.509.2908M

Montalto, M.; Piotto, G.; Nascimbeni, V. +7 more

We report the discovery of a new transiting exoplanet orbiting the star TIC 257060897 and detected using TESS full frame images. We acquired HARPS-N time-series spectroscopic data, and ground-based photometric follow-up observations from which we confirm the planetary nature of the transiting body. For the host star we determined: Teff

2022 Monthly Notices of the Royal Astronomical Society
Gaia 4
Star Cluster Formation and Evolution in M101: An Investigation with the Legacy Extragalactic UV Survey
DOI: 10.3847/1538-4357/ac7c07 Bibcode: 2022ApJ...935..166L

Sabbi, E.; Dale, D. A.; Calzetti, D. +13 more

We present Hubble Space Telescope WFC3/UVIS (F275W, F336W) and ACS/WFC optical (F435W, F555W, and F814W) observations of the nearby grand-design spiral galaxy M101 as part of the Legacy Extragalactic UV Survey (LEGUS). Compact sources detected in at least four bands were classified by both human experts and the convolutional neural network STARCNE…

2022 The Astrophysical Journal
eHST 4
NICMOS Kernel-phase Interferometry. I. Catalogue of Brown Dwarfs Observed in F110W and F170M
DOI: 10.3847/1538-3881/ac88d3 Bibcode: 2022AJ....164..244F

Kraus, Adam L.; Factor, Samuel M.

Filling out the dearth of detections between direct imaging and radial velocity surveys will test theories of planet formation and (sub)stellar binarity across the full range of semimajor axes, connecting formation of close- to wide-separation gas giants and substellar companions. Direct detection of close-in companions is notoriously difficult: c…

2022 The Astronomical Journal
Gaia eHST 4