Search Publications

Study of the Mass-loss Rate from the Sun
DOI: 10.3847/1538-4357/ac4fcb Bibcode: 2022ApJ...930...74M

Gopalswamy, Nat; Yashiro, Seiji; Michalek, Grzegorz

We investigate the temporal evolution of the yearly total mass-loss rate (YTMLR) from the Sun through coronal mass ejections (CMEs) over solar cycles 23 and 24. The mass determination of CMEs can be subject to significant uncertainty. To minimize this problem, we have used extensive statistical analysis. For this purpose, we employed data included…

2022 The Astrophysical Journal
SOHO 3
Dynamics of Explosive Events Observed by the Interface Region Imaging Spectrograph
DOI: 10.1007/s11207-022-01990-x Bibcode: 2022SoPh..297...76T

Tavabi, E.; Zeighami, S.; Heydari, M.

In this research, we investigate Explosive Events (EEs) in the off-limb solar atmosphere, with simultaneous observations from the Si IV, Mg II k, and slit-jaw images (SJI) of the Interface Region Imaging Spectrograph (IRIS), on 17 August 2014, and 19 February. IRIS data can be investigated to observe the motion of matter, fluctuations, energy abso…

2022 Solar Physics
IRIS 3
Ultraviolet Observations of Comet 96/P Machholz at Perihelion
DOI: 10.3847/1538-4357/ac3cbd Bibcode: 2022ApJ...926...93R

Raymond, J. C.; Bemporad, A.; Giordano, S. +2 more

Ultraviolet spectra of Comet 96/P Machholz were obtained during its 2002 perihelion with the UltraViolet Coronagraph Spectrometer instrument on board the SOHO satellite. Emission from H I, C II, C III, and O I is detected near the nucleus. The outgassing rate is in line with the value extrapolated from rates at larger distances from the Sun, and a…

2022 The Astrophysical Journal
SOHO 3
Solar-Wind High-Speed Stream (HSS) Alfvén Wave Fluctuations at High Heliospheric Latitudes: Ulysses Observations During Two Solar-Cycle Minima
DOI: 10.1007/s11207-022-02070-w Bibcode: 2022SoPh..297..143E

Hajra, Rajkumar; Echer, Ezequiel; Franco, Adriane Marques de Souza +2 more

We study Alfvén wave fluctuations in solar-wind high-speed streams (HSSs) at high heliolatitudes during the last two solar-cycle minima (SCM). Solar-wind plasma and interplanetary magnetic field (IMF) measured by Ulysses during four 50-day intervals in 1994, 1995, 2007, and 2008 were analyzed using wavelet and Fourier analyses, cross-correlation a…

2022 Solar Physics
Ulysses 3
Detection of Martian dust storms using mask regional convolutional neural networks
DOI: 10.1186/s40645-021-00464-1 Bibcode: 2022PEPS....9....4A

Gebhardt, Claus; Alshehhi, Rasha

Martian dust plays a crucial role in the meteorology and climate of the Martian atmosphere. It heats the atmosphere, enhances the atmospheric general circulation, and affects spacecraft instruments and operations. Compliant with that, studying dust is also essential for future human exploration. In this work, we present a method for the deep-learn…

2022 Progress in Earth and Planetary Science
MEx 3
The Quasar Luminosity Function at z 5 via Deep Learning and Bayesian Information Criterion
DOI: 10.3847/1538-4357/ac854b Bibcode: 2022ApJ...937...32S

Im, Myungshin; Shin, Suhyun; Kim, Yongjung

Understanding the faint end of quasar luminosity function (LF) at a high redshift is important since the number density of faint quasars is a critical element in constraining ultraviolet (UV) photon budgets for ionizing the intergalactic medium (IGM) in the early universe. Here, we present quasar LF reaching M 1450 ~ -22.0 AB mag at z ~…

2022 The Astrophysical Journal
eHST 3
The Dust Mass of Supernova Remnants in M31
DOI: 10.3847/1538-3881/ac35db Bibcode: 2022AJ....163...60W

Ren, Yi; Jiang, Biwei; Zhao, He +2 more

The dust temperature and mass of the supernova remnants (SNRs) in M31 are estimated by fitting the infrared spectral energy distribution calculated from the images in the Spitzer/IRAC4 and MIPS24, Herschel/PACS70, 100, and 160, and Herschel/SPIRE 250 and 350 µm bands. Twenty SNRs with relatively reliable photometry exhibit an average dust te…

2022 The Astronomical Journal
Herschel 3
The dynamical state of RXCJ1230.7+3439: A multi-substructured merging galaxy cluster
DOI: 10.1051/0004-6361/202243418 Bibcode: 2022A&A...663A..78B

Böhringer, H.; Chon, G.; Barrena, R.

We analyse the kinematical and dynamical state of the galaxy cluster RXCJ1230.7+3439 (RXCJ1230), at z = 0.332 using 93 new spectroscopic redshifts of galaxies acquired at the Telescopio Nazionale Galileo and from SDSS DR16 public data. We study the density galaxy distribution retrieved from photometric SDSS multiband data and find that RXCJ1230 ap…

2022 Astronomy and Astrophysics
XMM-Newton 3
Detection of highly correlated optical and X-ray variations in SS Cygni with Tomo-e Gozen and NICER
DOI: 10.1093/pasj/psac027 Bibcode: 2022PASJ...74L..17N

Enoto, Teruaki; Takita, Satoshi; Yamada, Shinya +8 more

We report on simultaneous optical and X-ray observations of the dwarf nova SS Cyg with Tomo-e Gozen/1.05 m Kiso Schmidt and Neutron star Interior Composition ExploreR (NICER)/International Space Station (ISS). A total of four observations were carried out in the quiescent state and highly correlated light variations between the two wavelengths wer…

2022 Publications of the Astronomical Society of Japan
Gaia 3
The first photometric investigation of the poor-thermal contact binary V749 Aurigae
DOI: 10.1093/pasj/psac080 Bibcode: 2022PASJ...74.1421C

Zhu, Li-Ying; Sarotsakulchai, Thawicharat; Soonthornthum, Boonrucksar +1 more

The multi-filter light curve analysis of V749 Aurigae (thereinafter V0749 Aur) is conducted for the first time. Its orbital period is improved from P = 0.409873 to 0.409890 d in this work. The photometric data from the All-Sky Automated Survey for SuperNovae (ASAS-SN) were utilized to examine the revised orbital period. Then, the phased multi-filt…

2022 Publications of the Astronomical Society of Japan
Gaia 3