Search Publications

Widespread 1-2 MeV Energetic Particles Associated with Slow and Narrow Coronal Mass Ejections: Parker Solar Probe and STEREO Measurements
DOI: 10.3847/1538-4357/ac3af2 Bibcode: 2022ApJ...925...96Z

Lugaz, Noé; Zhuang, Bin; Lario, David

Suprathermal ions in the corona are thought to serve as seed particles for large gradual solar energetic particle (SEP) events associated with fast and wide coronal mass ejections (CMEs). A better understanding of the role of suprathermal particles as seed populations for SEP events can be made by using observations close to the Sun. We study a se…

2022 The Astrophysical Journal
SOHO 4
Polarization Spectrum of Near-Infrared Zodiacal Light Observed with CIBER
DOI: 10.3847/1538-4357/ac416f Bibcode: 2022ApJ...926....6T

Shirahata, Mai; Cooray, Asantha; Matsuura, Shuji +14 more

We report the first measurement of the zodiacal light (ZL) polarization spectrum in the near-infrared between 0.8 and 1.8 µm. Using the low-resolution spectrometer on board the Cosmic Infrared Background Experiment, calibrated for absolute spectrophotometry and spectropolarimetry, we acquire long-slit polarization spectral images of the tota…

2022 The Astrophysical Journal
AKARI 4
X-Ray and Radio Studies of the Candidate Millisecond Pulsar Binary 4FGL J0935.3+0901
DOI: 10.1088/1674-4527/ac3e5e Bibcode: 2022RAA....22b5012Z

Zheng, Dong; Wang, Zhong-Xiang; Xing, Yi +1 more

4FGL J0935.5+0901, a γ-ray source recently identified as a candidate redback-type millisecond pulsar (MSP) binary, shows an interesting feature of having double-peaked emission lines in its optical spectrum. This feature would further suggest the source is a transitional MSP system in the sub-luminous disk state. We have observed the source with X…

2022 Research in Astronomy and Astrophysics
XMM-Newton 4
Discovery of the most luminous quasar of the last 9 Gyr
DOI: 10.1017/pasa.2022.36 Bibcode: 2022PASA...39...37O

Fan, Xiaohui; Wolf, Christian; Lai, Samuel +8 more

We report the discovery of a bright ( g = 14.5 mag (AB), K = 11.9 mag (Vega)) quasar at redshift z=0.83 — the optically brightest (unbeamed) quasar at z>0.4. SMSS J114447.77-430859.3, at a Galactic latitude of b=+18.1°, was identified by its optical colours from the SkyMapper Southern Survey (SMSS) during a search for symbiotic binary stars. Op…

2022 Publications of the Astronomical Society of Australia
Gaia 4
Infrared Excess of a Large OB Star Sample
DOI: 10.3847/1538-4357/ac8168 Bibcode: 2022ApJ...935..175D

Jiang, Biwei; Deng, Dingshan; Wang, Yuxi +2 more

The infrared (IR) excess from OB stars is commonly considered to be a contribution from ionized stellar wind or circumstellar dust. With the newly published Large Sky Area Multi-Object Fiber Spectroscopy Telescope (LAMOST)-OB catalog and Galactic O-Star Spectroscopic Survey data, this work steps further on understanding the IR excess of OB stars. …

2022 The Astrophysical Journal
AKARI Gaia Herschel 4
Precursory Signals of Forbush Decreases Not Connected with Shock Waves
DOI: 10.1007/s11207-022-01951-4 Bibcode: 2022SoPh..297...24L

Mavromichalaki, H.; Belov, A.; Eroshenko, E. +4 more

Forbush decreases (FDs) are sharp reductions of the cosmic-ray (CR) intensity, following intense solar activity such as coronal mass ejections (CMEs) and their corresponding interplanetary shocks. In some cases, shocks create sudden storm commencements (SSCs) at the Earth's magnetosphere with significant interest for space-weather studies. Preincr…

2022 Solar Physics
SOHO 4
Effects of Spectral Resolution on Simple Magnetic Field Diagnostics of the Mg II H and K Lines
DOI: 10.3847/1538-4357/ac886f Bibcode: 2022ApJ...936..115C

Rempel, Matthias; Centeno, Rebecca; del Pino Alemán, Tanausú +1 more

We study the effects of finite spectral resolution on the magnetic field values retrieved through the weak-field approximation (WFA) from the cores of the Mg II h and k lines. The retrieval of the line-of-sight component of the magnetic field, B LOS, from synthetic spectra generated in a uniformly magnetized FAL-C atmosphere is accurate…

2022 The Astrophysical Journal
IRIS 4
The GALAH Survey: improving our understanding of confirmed and candidate planetary systems with large stellar surveys
DOI: 10.1093/mnras/stab3498 Bibcode: 2022MNRAS.510.2041C

Lewis, Geraint F.; Casey, Andrew R.; Wittenmyer, Robert A. +24 more

Pioneering photometric, astrometric, and spectroscopic surveys is helping exoplanetary scientists better constrain the fundamental properties of stars within our galaxy and the planets these stars host. In this study, we use the third data release from the stellar spectroscopic GALAH Survey, coupled with astrometric data of eDR3 from the Gaia sate…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 4
The young Galactic cluster NGC 225: binary stars' content and total mass estimate
DOI: 10.1093/mnras/stac1199 Bibcode: 2022MNRAS.513.5299Y

Munari, U.; Ochner, P.; Carraro, G. +2 more

Galactic star clusters are known to harbour a significant amount of binary stars, yet their role in the dynamical evolution of the cluster as a whole is not comprehensively understood. We investigated the influence of binary stars on the total mass estimate for the case of the moderately populated Galactic star cluster NGC 225. The analysis of mul…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 4
A search for hot subdwarf binaries in data from the Transiting Exoplanet Survey Satellite
DOI: 10.1093/mnras/stac2088 Bibcode: 2022MNRAS.516.1509K

Siwak, M.; Zola, S.; Krzesinski, J. +1 more

We present the results of a search for binary hot subdwarf stars in photometric data from the Transiting Exoplanet Survey Satellite (TESS). The sample of objects used in this work was a byproduct of another search for pulsating hot subdwarfs, which resulted in the discovery of nearly 400 non-pulsating variable candidates. The periodogram for each …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 4