Search Publications

Redshift and stellar mass dependence of intrinsic shapes of disc-dominated galaxies from COSMOS observations below z = 1.0
DOI: 10.1093/mnras/stac1988 Bibcode: 2022MNRAS.515.3603H

Tallada-Crespí, P.; Teyssier, R.; Laigle, C. +4 more

The high abundance of disc galaxies without a large central bulge challenges predictions of current hydrodynamic simulations of galaxy formation. We aim to shed light on the formation of these objects by studying the redshift and mass dependence of their intrinsic 3D shape distributions in the COSMOS galaxy survey below redshift z = 1.0. This dist…

2022 Monthly Notices of the Royal Astronomical Society
eHST 5
NuSTAR discovery of the hard X-ray emission and a wide-band X-ray spectrum from the Pictor A western hotspot
DOI: 10.1093/pasj/psac022 Bibcode: 2022PASJ...74..602S

Katsuda, Satoru; Sato, Kosuke; Tashiro, Makoto S. +5 more

Utilizing Chandra, XMM-Newton, and NuSTAR, a wide-band X-ray spectrum from 0.2 to 20 keV is reported from the western hotspot of Pictor A. In particular, the X-ray emission is significantly detected in the 3 to 20 keV band at 30σ by NuSTAR. This is the first detection of hard X-rays with energies above 10 keV from a jet termination hotspot of acti…

2022 Publications of the Astronomical Society of Japan
XMM-Newton 5
SPHERE adaptive optics performance for faint targets
DOI: 10.1051/0004-6361/202243820 Bibcode: 2022A&A...667A.114J

Jones, M. I.; Milli, J.; Blanchard, I. +4 more

Context. High-contrast imaging is a powerful technique for detecting and characterizing planetary companions at orbital separations ≳100 mas from their parent stars.
Aims: We aim to study the limiting magnitude of the VLT/SPHERE adaptive optics (AO) system and the corresponding instrument performance for faint targets (G ≥ 11.0 mag).
Met…

2022 Astronomy and Astrophysics
Gaia 5
Multi-Spacecraft Observations of an Interplanetary Coronal Mass Ejection Interacting with Two Solar-Wind Regimes Observed by the Ulysses and Twin-STEREO Spacecraft
DOI: 10.1007/s11207-022-02077-3 Bibcode: 2022SoPh..297..148M

Foullon, Claire; Barnes, David; Davies, Jackie +2 more

We present a combined study of a coronal mass ejection (CME), revealed in a unique orbital configuration that permits the analysis of remote-sensing observations on 27 June 2007 from the twin Solar Terrestrial Relations Observatory (STEREO)-A and -B spacecraft and of its subsequent in situ counterpart outside the ecliptic plane, the interplanetary…

2022 Solar Physics
Ulysses 5
Complex Catalogue of High Speed Streams Associated with Geomagnetic Storms During Solar Cycle 24
DOI: 10.1007/s11207-022-01998-3 Bibcode: 2022SoPh..297...65B

Besliu-Ionescu, Diana; Maris Muntean, Georgeta; Dobrica, Venera

A complex catalogue of high speed streams produced by coronal holes and their effects in the terrestrial magnetosphere - the so-called geomagnetic storms - for Solar Cycle 24 (2009 to 2019) is presented here. This catalogue is structured in three parts describing the high-speed stream characteristics, the interplanetary magnetic field state, and t…

2022 Solar Physics
SOHO 5
He II Lyα Transmission Spikes and Absorption Troughs in Eight High-resolution Spectra Probing the End of He II Reionization
DOI: 10.3847/1538-4357/ac524a Bibcode: 2022ApJ...927..175M

Richter, Philipp; Hennawi, Joseph F.; Worseck, Gábor +3 more

We present statistics of He II Lyα transmission spikes and large-scale absorption troughs using archival high-resolution (R = λ/Δλ ≃ 12,500-18,000) far-UV spectra of eight He II-transparent quasars obtained with the Cosmic Origins Spectrograph on the Hubble Space Telescope. The sample covers the redshift range 2.5 ≲ z ≲ 3.8, thereby probing the ra…

2022 The Astrophysical Journal
eHST 5
Spectral Signs of Simultaneous Sublimation Activity and the Appearance of a Dust Exosphere on Eight Asteroids of the Main Belt Near Perihelion
DOI: 10.1134/S0038094622020022 Bibcode: 2022SoSyR..56...84B

Shcherbina, M. P.; Busarev, V. V.; Savelova, A. A. +1 more

In December 2020, at the 2-m telescope of the Terskol branch of the Institute of Astronomy, we carried out spectrophotometric observations in the range of ~0.36-0.95 µm of nine asteroids of the Main Belt (19 Fortuna, 52 Europa, 102 Miriam, 177 Irma, 203 Pompeja, 250 Bettina, 266 Aline, 379 Huenna, and 383 Janina), which were near perihelia o…

2022 Solar System Research
SOHO 5
Herschel Investigation of Cores and Filamentary Structures in the Perseus Molecular Cloud
DOI: 10.1088/1674-4527/ac5bc7 Bibcode: 2022RAA....22e5012Z

Zhang, Guo-Yin; Zhang, Chang; Li, Jin-Zeng +1 more

Cores and filamentary structures are the prime birthplaces of stars, and play key roles in the process of star formation. Latest advances in the methods of multi-scale source and filament extraction, and in making high-resolution column density map from Herschel multi-wavelength observations enable us to detect the filamentary network structures i…

2022 Research in Astronomy and Astrophysics
Herschel 5
An Efficient High-Resolution Global-Local Network to Detect Lunar Features for Space Energy Discovery
DOI: 10.3390/rs14061391 Bibcode: 2022RemS...14.1391J

Liu, Lei; Jia, Yutong; Peng, Siqing +2 more

Lunar craters and rilles are significant topographic features on the lunar surface that will play an essential role in future research on space energy resources and geological evolution. However, previous studies have shown low efficiency in detecting lunar impact craters and poor accuracy in detecting lunar rilles. There is no complete automated …

2022 Remote Sensing
MEx 5
Direct Evidence of Magnetic Reconnection Onset via the Tearing Instability
DOI: 10.3389/fspas.2022.869491 Bibcode: 2022FrASS...9.9491B

Verscharen, Daniel; Walsh, Andrew P.; Forsyth, Colin +4 more

Magnetic reconnection is a sporadic process responsible for energy release in space and laboratory plasmas. It is believed that the tearing mode instability may be responsible for the onset of reconnection in the magnetotail. However, due to its elusive nature, there is an absence of in-situ observations of the tearing instability prior to magneti…

2022 Frontiers in Astronomy and Space Sciences
Cluster 5