Search Publications

Confirmation of a Sub-Saturn-size Transiting Exoplanet Orbiting a G Dwarf: TOI-1194 b and a Very Low Mass Companion Star: TOI-1251 B from TESS
DOI: 10.1088/1674-4527/ad057b Bibcode: 2024RAA....24c5012W

Zheng, Jie; Bieryla, Allyson; Howell, Steve B. +18 more

We report the confirmation of a sub-Saturn-size exoplanet, TOI-1194 b, with a mass of about M J, and a very low mass companion star with a mass of about 96.5 ± 1.5 M J, TOI-1251 B. Exoplanet candidates provided by the Transiting Exoplanet Survey Satellite (TESS) are suitable for further foll…

2024 Research in Astronomy and Astrophysics
Gaia 2
One-dimensional Microphysics Model of Venusian Clouds from 40 to 100 km: Impact of the Middle-atmosphere Eddy Transport and SOIR Temperature Profile on the Cloud Structure
DOI: 10.3847/PSJ/ad25f3 Bibcode: 2024PSJ.....5...57K

Vandaele, Ann Carine; Terada, Naoki; Imamura, Takeshi +4 more

We conducted a simulation of H2SO4 vapor, H2O vapor, and H2SO4–H2O liquid aerosols from 40 to 100 km, using a 1D Venus cloud microphysics model based on the one detailed in Imamura & Hashimoto. The cloud distribution obtained is in good agreement with in situ observations by Pio…

2024 The Planetary Science Journal
VenusExpress 2
Machine learning applications in studies of the physical properties of active galactic nuclei based on photometric observations
DOI: 10.1051/0004-6361/202346557 Bibcode: 2024A&A...685A.107M

Ackermann, Markus; Kowalski, Marek; Mechbal, Sarah

Context. We investigate the physical nature of active galactic nuclei (AGNs) using machine learning (ML) tools.
Aims: We show that the redshift, z, bolometric luminosity, LBol, central mass of the supermassive black hole (SMBH), MBH, Eddington ratio, λEdd, and AGN class (obscured or unobscured) can be reconstr…

2024 Astronomy and Astrophysics
Gaia 2
Ejection and dynamics of aggregates in the coma of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/202348692 Bibcode: 2024A&A...687A.289L

Agarwal, J.; Lemos, P.; Marschall, R. +1 more

Context. The process of gas-driven ejection of refractory materials from cometary surfaces continues to pose a challenging question in cometary science. The activity modeling of comet 67P/Churyumov-Gerasimenko, based on data from the Rosetta mission, has significantly enhanced our comprehension of cometary activity. But thermophysical models have …

2024 Astronomy and Astrophysics
Rosetta 2
Characterization of aqueous alteration and formation of salty exposures at Ius Chasma, Mars
DOI: 10.1016/j.icarus.2023.115800 Bibcode: 2024Icar..40815800W

Flahaut, Jessica; Weitz, Catherine M.; Bishop, Janice L. +6 more

Intriguing outcrops in Ius Chasma provide a window into past aqueous processes in Valles Marineris, Mars. Hydrous sulfate minerals are abundant throughout this region, but one area in Ius Chasma includes phyllosilicates, opal, and additional materials with unusual spectral features. This study at Geryon Montes, an east-west horst that divides Ius …

2024 Icarus
MEx 2
Variation in the Pedersen Conductance Near Jupiter's Main Emission Aurora: Comparison of Hubble Space Telescope and Galileo Measurements
DOI: 10.1029/2023JA032122 Bibcode: 2024JGRA..12932122R

Nichols, J. D.; Vogt, M. F.; Rutala, M. J. +1 more

We present the first large-scale statistical survey of the Jovian main emission (ME) to map auroral properties from their ionospheric locations out into the equatorial plane of the magnetosphere, where they are compared directly to in-situ spacecraft measurements. We use magnetosphere-ionosphere (MI) coupling theory to calculate currents from the …

2024 Journal of Geophysical Research (Space Physics)
Ulysses eHST 2
Does High-Latitude Ionospheric Electrodynamics Exhibit Hemispheric Mirror Symmetry?
DOI: 10.5194/angeo-42-229-2024 Bibcode: 2024AnGeo..42..229H

Hatch, Spencer Mark; Vanhamäki, Heikki; Magnus Laundal, Karl +6 more

Ionospheric electrodynamics is a problem of mechanical stress balance mediated by electromagnetic forces. Joule heating (the total rate of frictional heating of thermospheric gases and ionospheric plasma) and ionospheric Hall and Pedersen conductances comprise three of the most basic descriptors of this problem. More than half a century after iden…

2024 Annales Geophysicae
Cluster 2
HD 12098: a highly distorted dipole mode in an obliquely pulsating roAp star
DOI: 10.1093/mnras/stae431 Bibcode: 2024MNRAS.529..556K

Saio, H.; Kurtz, D. W.; Joshi, Santosh +2 more

HD 12098 is a rapidly oscillating Ap star pulsating in the most distorted dipole mode yet observed in this class of star. Using Transiting Exoplanet Survey Satellite (TESS) Sector 58 observations, we show that there are photometric spots at both the magnetic poles of this star. It pulsates obliquely primarily in a strongly distorted dipole mode wi…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
Very metal-poor stars I: a catalogue derived from LAMOST DR9
DOI: 10.1093/mnras/stae1567 Bibcode: 2024MNRAS.532.1099H

Zhao, Gang; Li, Haining; Hou, Xiaokun

In this paper, a semisupervised machining learning technique had been utilized to analyse low-resolution stellar spectra from Large sky Area Multi-Object fiber Spectroscopic Telescope (LAMOST) Data Release 9 (DR9). We identified approximately 111 000 potential very metal-poor stars. Estimation of their stellar parameters ($T_{\rm eff}$, ${\rm log}…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
The outflowing ionised gas of I Zw 1 observed by HST COS
DOI: 10.1051/0004-6361/202449544 Bibcode: 2024A&A...686A..99J

Brandt, W. N.; Kriss, G. A.; Costantini, E. +8 more


Aims: We present an analysis of the Hubble Space Telescope Cosmic Origins Spectrograph spectrum of I Zw 1 aiming to probe the absorbing medium associated with the active galactic nucleus (AGN).
Methods: We fitted the emission spectrum and performed spectral analysis of the identified absorption features to derive the corresponding ionic …

2024 Astronomy and Astrophysics
XMM-Newton eHST 2