Search Publications

Testing the Kerr Black Hole Hypothesis Using X-Ray Reflection Spectroscopy and a Thin Disk Model with Finite Thickness
DOI: 10.3847/1538-4357/aba625 Bibcode: 2020ApJ...899...80A

Tripathi, Ashutosh; Abdikamalov, Askar B.; Ayzenberg, Dimitry +5 more

X-ray reflection spectroscopy is a powerful tool for probing the strong gravity region of black holes and can be used for testing general relativity in the strong field regime. Simplifications of the available relativistic reflection models limit the capability of performing accurate measurements of the properties of black holes. In this paper, we…

2020 The Astrophysical Journal
Suzaku 61
The Variable and Non-variable X-Ray Absorbers in Compton-thin Type II Active Galactic Nuclei
DOI: 10.3847/1538-4357/ab92ab Bibcode: 2020ApJ...897...66L

Nikutta, Robert; Laha, Sibasish; Markowitz, Alex G. +3 more

We have conducted an extensive X-ray spectral variability study of a sample of 20 Compton-thin type II galaxies using broadband spectra from XMM-Newton, Chandra, and Suzaku. The aim is to study the variability of the neutral intrinsic X-ray obscuration along the line of sight and investigate the properties and location of the dominant component of…

2020 The Astrophysical Journal
Suzaku XMM-Newton 44
Application of an X-Ray Clumpy Torus Model (XCLUMPY) to 10 Obscured Active Galactic Nuclei Observed with Suzaku and NuSTAR
DOI: 10.3847/1538-4357/ab96bc Bibcode: 2020ApJ...897....2T

Tanimoto, Atsushi; Ueda, Yoshihiro; Odaka, Hirokazu +4 more

We apply XCLUMPY, an X-ray spectral model from a clumpy torus in an active galactic nucleus (AGN), to the broadband X-ray spectra of 10 obscured AGNs observed with both Suzaku and NuSTAR. The infrared spectra of these AGNs were analyzed by Ichikawa et al. with the CLUMPY code. Because XCLUMPY adopts the same clump distribution as that in the CLUMP…

2020 The Astrophysical Journal
Suzaku 25
A Hard Look at Local, Optically Selected, Obscured Seyfert Galaxies
DOI: 10.3847/1538-4357/abb29f Bibcode: 2020ApJ...901..161K

Kaastra, J. S.; Stern, D.; Brandt, W. N. +11 more

We study the X-ray spectra of a sample of 19 obscured, optically selected Seyfert galaxies (Sy 1.8, 1.9, and 2) in the local universe (d ≤ 175 Mpc), drawn from the CfA Seyfert sample. Our analysis is driven by the high sensitivity of NuSTAR in the hard X-rays, coupled with soft X-ray spectra using XMM-Newton, Chandra, Suzaku, and Swift/XRT. We als…

2020 The Astrophysical Journal
Suzaku XMM-Newton 23
Inverse First Ionization Potential Effects in Giant Solar Flares Found from Earth X-Ray Albedo with Suzaku/XIS
DOI: 10.3847/1538-4357/ab7207 Bibcode: 2020ApJ...891..126K

Maeda, Yoshitomo; Katsuda, Satoru; Sato, Kosuke +21 more

We report X-ray spectroscopic results for four giant solar flares that occurred on 2005 September 7 (X17.0), 2005 September 8 (X5.4), 2005 September 9 (X6.2), and 2006 December 5 (X9.0), obtained from Earth albedo data with the X-ray Imaging Spectrometer (XIS) on board Suzaku. The good energy resolution of the XIS (FWHM ∼ 100 eV) enables us to sep…

2020 The Astrophysical Journal
Suzaku 23
Nature of Compton-thick Active Galactic Nuclei in "Nonmerging" Luminous Infrared Galaxies UGC 2608 and NGC 5135 Revealed with Broadband X-Ray Spectroscopy
DOI: 10.3847/1538-4357/ab94b1 Bibcode: 2020ApJ...897..107Y

Imanishi, Masatoshi; Tanimoto, Atsushi; Ueda, Yoshihiro +4 more

We have analyzed the broadband X-ray spectra of active galactic nuclei (AGNs) in two "nonmerging" luminous infrared galaxies (LIRGs), UGC 2608 and NGC 5135, utilizing the data of Nuclear Spectroscopic Telescope Array, Suzaku, XMM-Newton, and Chandra. Applying the X-ray clumpy-torus model (XCLUMPY), we find that both sources have similar spectra ch…

2020 The Astrophysical Journal
Suzaku XMM-Newton 22
Is Superorbital Modulation in SMC X-1 Caused by Absorption in a Warped Precessing Accretion Disk?
DOI: 10.3847/1538-4357/ab8224 Bibcode: 2020ApJ...895...10P

Maitra, Chandreyee; Paul, Biswajit; Pradhan, Pragati

We present a broadband spectral-timing analysis of SMC X-1 at different intensity states of its superorbital variation using 10 Suzaku and 6 Nuclear Spectroscopic Telescope Array (NuSTAR) observations. The spectrum in all the states can be described by an absorbed power law with a high-energy cutoff and a blackbody component along with an iron emi…

2020 The Astrophysical Journal
Suzaku 18
Uncovering the Primary X-Ray Emission and Possible Starburst Component in the Polarized NLS1 Mrk 1239
DOI: 10.3847/1538-4357/abb08a Bibcode: 2020ApJ...901..118B

Komossa, S.; Gallo, Luigi C.; Grupe, Dirk +2 more

X-ray observations of the unique NLS1 galaxy Mrk 1239 spanning 18 yr are presented. Data from XMM-Newton, Suzaku, Swift, and NuSTAR are combined to obtain a broadband, multi-epoch view of the source. There is spectral variability in the 3-10 keV band over the 18 yr. An analysis of the NuSTAR and Suzaku lightcurves also suggests rapid variability i…

2020 The Astrophysical Journal
Suzaku XMM-Newton 9
Suzaku Measurements of Hot Halo Emission at Outskirts for Two Poor Galaxy Groups: NGC 3402 and NGC 5129
DOI: 10.3847/1538-4357/aba691 Bibcode: 2020ApJ...899..160N

Sun, Ming; Dai, Xinyu; Nugent, Jenna M.

We present Suzaku off-center observations of two poor galaxy groups, NGC 3402 and NGC 5129, with temperatures below 1 keV. Through spectral decomposition, we measured their surface brightnesses and temperatures out to 530 and 1430 times the critical density of the universe for NGC 3402 and NGC 5129, respectively. These quantities are consistent wi…

2020 The Astrophysical Journal
Suzaku 8