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Predicting the black hole mass and correlations in X-ray reverberating AGNs using neural networks
DOI: 10.1093/mnras/stac924 Bibcode: 2022MNRAS.513..648C

Chainakun, P.; Young, A. J.; Hancock, S. +1 more

We develop neural network models to predict the black hole mass using 22 reverberating active galactic nucleus (AGN) samples in the XMM-Newton archive. The model features include the fractional excess variance (Fvar) in 2-10 keV band, Fe-K lag amplitude, 2-10 keV photon counts, and redshift. We find that the prediction accuracy of the n…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 9
Non-LTE Inversion of Prominence Spectroscopic Observations in Hα and Mg II h&k lines
DOI: 10.3847/1538-4357/ac6bf5 Bibcode: 2022ApJ...932....3J

Heinzel, Petr; Schmieder, Brigitte; Jejčič, Sonja +4 more

We continued our investigation of the plasma characteristics of a quiescent prominence that occurred on 2017 March 30. The prominence was observed simultaneously by several instruments, including the Interface Region Imaging Spectrograph (IRIS) and the Multichannel Subtractive Double Pass (MSDP) spectrograph operating at the Meudon solar tower. We…

2022 The Astrophysical Journal
IRIS 9
Solenoidal turbulent modes and star formation efficiency in Galactic plane molecular clouds
DOI: 10.1093/mnras/stac1812 Bibcode: 2022MNRAS.515..271R

Rigby, Andrew J.; Eden, David J.; Rani, Raffaele +1 more

It is speculated that the high star formation efficiency observed in spiral-arm molecular clouds is linked to the prevalence of compressive (curl-free) turbulent modes, while the shear-driven solenoidal (divergence-free) modes appear to be the main cause of the low star formation efficiency that characterizes clouds in the Central Molecular Zone. …

2022 Monthly Notices of the Royal Astronomical Society
Herschel 9
Age-morphology dependence of the Milky Way boxy/peanut bulge seen in Mira variables
DOI: 10.1093/mnras/stac3085 Bibcode: 2022MNRAS.517.6060S

Schönrich, Ralph; Dehnen, Walter; Semczuk, Marcin +1 more

We analyse the distribution of Mira variable stars in the central region of the Milky Way. We find that with increasing period, i.e. decreasing age, the Miras shift towards negative Galactic longitudes ℓ. Comparing to a cosmological zoom simulation of a barred galaxy, we find that this shift with age can be explained by an age-morphology dependenc…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 9
An X-Ray Study of Coronally Connected Active Eclipsing Binaries
DOI: 10.3847/1538-4357/ac7716 Bibcode: 2022ApJ...934...20S

Pandey, J. C.; Singh, Gurpreet

We present a detailed X-ray analysis and imaging of stellar coronae of five coronally connected eclipsing binaries, namely, 44 Boo, DV Psc, ER Vul, XY UMa, and TX Cnc. Both components of these binaries are found to be active. The X-ray light curves of detached and semidetached type systems show eclipsed-like features, whereas no evidence for coron…

2022 The Astrophysical Journal
XMM-Newton 9
Absolute calibration of the Colour and Stereo Surface Imaging System (CaSSIS)
DOI: 10.1016/j.pss.2021.105394 Bibcode: 2022P&SS..21105394T

Almeida, Miguel; Cremonese, Gabriele; Thomas, Nicolas +5 more

The Colour and Stereo Surface Imaging System (CaSSIS) onboard the ExoMars Trace Gas Orbiter (TGO) has observed several standard stars and Jupiter with the aim of deriving the absolute calibration factors that convert observed signal into reflectance ("I over F"). The targets were observed through all four colour filters and hence a relative calibr…

2022 Planetary and Space Science
ExoMars-16 9
Multiwavelength study of the gravitationally lensed blazar QSO B0218+357 between 2016 and 2020
DOI: 10.1093/mnras/stab3454 Bibcode: 2022MNRAS.510.2344A

Maraschi, L.; Covino, S.; Antonelli, L. A. +207 more

We report multiwavelength observations of the gravitationally lensed blazar QSO B0218+357 in 2016-2020. Optical, X-ray, and GeV flares were detected. The contemporaneous MAGIC observations do not show significant very high energy (VHE; ≳100 GeV) gamma-ray emission. The lack of enhancement in radio emission measured by The Owens Valley Radio Observ…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 9
Mass-ratio Distribution of Binaries from the LAMOST-MRS Survey
DOI: 10.3847/1538-4357/ac731d Bibcode: 2022ApJ...933..119L

Wang, Luqian; Han, Zhanwen; Chen, Xuefei +7 more

Binary evolution leads to the formation of important objects that are crucial for the development of astrophysics, but the statistical properties of binary populations are still poorly understood. The LAMOST-MRS has provided a large sample of stars to study the properties of binary populations, especially for the mass-ratio distributions and binar…

2022 The Astrophysical Journal
Gaia 9
Polar and mid-latitude vortices and zonal flows on Jupiter and Saturn
DOI: 10.1016/j.icarus.2022.114942 Bibcode: 2022Icar..37914942H

Yadav, Rakesh K.; Featherstone, Nicholas A.; Aurnou, Jonathan M. +1 more

Zonal flow on Jupiter and Saturn consists of equatorial super-rotation and alternating East-West jet streams at higher latitudes. Interacting with these zonal flows, numerous vortices occur with various sizes and lifetimes. The Juno mission and Cassini's grand finale have shown that the zonal jets of Jupiter and Saturn extend deeply into their mol…

2022 Icarus
Cassini 9
Effects of Hydrogen versus Helium on Electromagnetic Black Hole Observables
DOI: 10.3847/1538-4357/ac854d Bibcode: 2022ApJ...937...60W

Gammie, Charles F.; Wong, George N.

The centers of our Galaxy and the nearby Messier 87 are known to contain supermassive black holes, which support accretion flows that radiate across the electromagnetic spectrum. Although the composition of the accreting gas is unknown, it is likely a mix of ionized hydrogen and helium. We use a simple analytic model and a suite of numerical gener…

2022 The Astrophysical Journal
eHST 9