Search Publications

Relativistic Fe Kα line in the composite X-ray spectra of radio-loud active galactic nuclei
DOI: 10.1093/mnras/stz2030 Bibcode: 2019MNRAS.488.4378H

Jin, Chichuan; Liu, Zhu; Yuan, Weimin +1 more

While a broad Fe Kα emission line is generally found in the X-ray spectra of radio quiet (RQ) active galactic nuclei (AGNs), this feature, commonly thought to be broadened by the relativistic effects near the central black hole, appears to be rare in their radio loud (RL) counterparts. In this paper, we carry out a detailed study of the ensemble p…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4
Propagation of Solar Energetic Particles in the Outer Heliosphere: Interplay between Scattering and Adiabatic Focusing
DOI: 10.3847/2041-8213/ab50bd Bibcode: 2019ApJ...885L..28H

Wan, W.; He, H. -Q.

The turbulence and spatial nonuniformity of the guide magnetic field cause two competitive effects, namely, the scattering effect and the adiabatic focusing effect, respectively. In this work, we numerically solve the five-dimensional Fokker-Planck transport equation to investigate the radial evolutions of these important effects undergone by the …

2019 The Astrophysical Journal
Ulysses 4
Potential role of energetic particle observations in geomagnetic storm forecasting
DOI: 10.1016/j.asr.2019.05.012 Bibcode: 2019AdSpR..64..801A

Valtonen, Eino; Ameri, Dheyaa

We have searched for solar proton events consisting of both solar energetic particles (SEPs) accelerated near the Sun and energetic storm particles (ESPs) accelerated by interplanetary shocks driven by coronal mass ejections (CMEs) and observed near the time when the shock passes the observer. The purpose of this study is to investigate the possib…

2019 Advances in Space Research
SOHO 4
The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey - II. X-ray and optical properties of the cluster sample
DOI: 10.1093/mnras/stz1097 Bibcode: 2019MNRAS.486.4863T

Plat, Adèle; Márquez, Isabel; Durret, Florence +3 more

We present X-ray and optical properties of the optically confirmed galaxy cluster sample from the 3XMM/SDSS Stripe 82 cluster survey. The sample includes 54 galaxy clusters in the redshift range of 0.05-1.2, with a median redshift of 0.36. We first present the X-ray temperature and luminosity measurements that are used to investigate the X-ray lum…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4
Constraining the Active Galactic Nucleus and Starburst Properties of the IR-luminous Quasar Host Galaxy APM08279+5255 at Redshift 4 with SOFIA
DOI: 10.3847/1538-4357/ab11ce Bibcode: 2019ApJ...876...48L

Casey, Caitlin M.; Staguhn, Johannes; Dowell, C. Darren +3 more

We present far-IR photometry and the infrared spectrum of the z = 3.9114 quasar/starburst composite system APM 08279+5255, obtained using the Stratospheric Observatory for Infrared Astronomy (SOFIA)/High-resolution Airborne Wideband Camera+ (HAWC+) and the Spitzer Space Telescope Infrared Spectrograph. We decompose the IR-to-radio spectral energy …

2019 The Astrophysical Journal
Herschel 4
X-Ray Spectrum of RBS 315: Absorption or Intrinsic Curvature
DOI: 10.3847/1538-4357/ab340f Bibcode: 2019ApJ...882..130B

Behar, Ehud; Mushotzky, Richard F.; Ben Haim, Sivan

X-ray absorption of high-redshift quasars is enigmatic, because it remains unclear where in the universe the absorbing gas is. If absorption occurs near the high-z host, it could help us understand early stages of galaxy formation. If it is in the intergalactic medium (IGM), it provides a unique way to probe this elusive baryon component. We repor…

2019 The Astrophysical Journal
XMM-Newton 4
Lens Model and Source Reconstruction Reveal the Morphology and Star Formation Distribution in the Cool Spiral LIRG SGAS J143845.1+145407
DOI: 10.3847/1538-4357/ab0d7d Bibcode: 2019ApJ...875...18D

Rigby, Jane R.; Whitaker, Katherine E.; Sharon, Keren +8 more

We present Hubble Space Telescope (HST) imaging and grism spectroscopy of a strongly lensed LIRG at z = 0.816, SGAS 143845.1+145407, and use the magnification boost of gravitational lensing to study the distribution of star formation throughout this galaxy. Based on the HST imaging data, we create a lens model for this system; we compute the mass …

2019 The Astrophysical Journal
eHST 4
A Hubble Space Telescope Survey for Novae in the Globular Clusters of M87
DOI: 10.3847/1538-4357/ab0490 Bibcode: 2019ApJ...874...65D

Shara, Michael M.; Zurek, David; Doyle, Trisha F. +1 more

The giant elliptical galaxy M87 has been imaged over 30 consecutive days in 2001, 60 consecutive days in 2005-2006, and every 5 days over a 265-day span in 2016-2017 with the Hubble Space Telescope, leading to the detection of 137 classical novae throughout M87. We have identified 2134 globular clusters (GC) in M87 in these images and carried out …

2019 The Astrophysical Journal
eHST 4
Relation between solar flares and halo coronal mass ejections
DOI: 10.1007/s12036-018-9570-1 Bibcode: 2019JApA...40....1R

Sankarasubramanian, K.; Rao, V. Koteswara; Gopal, K. Rama +2 more

Solar flares and coronal mass ejections (CMEs) are two very important active events from Sun. Inspite of several theoretical and statistical analyses, the relation between solar flares and CMEs is so far not well established, and strong opinions and arguments still continue. Statistical approaches use a lot of data available from many measurements…

2019 Journal of Astrophysics and Astronomy
Hinode SOHO 4
Automated reconstruction of subsurface interfaces in Promethei Lingula near the Martian south pole by using SHARAD data
DOI: 10.1016/j.pss.2018.08.001 Bibcode: 2019P&SS..166...59X

Muller, J. -P.; Xiong, S.

Subsurface layers are preserved in polar regions on Mars, which are considered to be a record of past climate changes on Mars. Orbital radar instruments like the SHAllow RADar (SHARAD) on board Mars Reconnaissance Orbiter (MRO) transmit radar signals to Mars and receive a set of signals returned from interfaces having a contrast in dielectric prop…

2019 Planetary and Space Science
MEx 4