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
Sign of Hard-X-Ray Pulsation from the γ -Ray Binary System LS 5039
DOI: 10.1103/PhysRevLett.125.111103 Bibcode: 2020PhRvL.125k1103Y

Takahashi, T.; Enoto, T.; Makishima, K. +3 more

To understand the nature of the brightest γ -ray binary system LS 5039, hard x-ray data of the object, taken with the Suzaku and NuSTAR observatories in 2007 and 2016, respectively, were analyzed. The two data sets jointly gave tentative evidence for a hard x-ray periodicity, with a period of ∼9 s and a period increase rate by ∼3 ×10-10

2020 Physical Review Letters
Suzaku 41
Testing general relativity with x-ray reflection spectroscopy: The Konoplya-Rezzolla-Zhidenko parametrization
DOI: 10.1103/PhysRevD.102.124071 Bibcode: 2020PhRvD.102l4071N

Tripathi, Ashutosh; Abdikamalov, Askar B.; Ayzenberg, Dimitry +6 more

X-ray reflection spectroscopy is a promising technique for testing general relativity in the strong-field regime as it can be used to test the Kerr black hole hypothesis. In this context, the parametrically deformed black hole metrics proposed by Konoplya, Rezzolla, and Zhidenko [Phys. Rev. D 93, 064015 (2016), 10.1103/PhysRevD.93.064015] form an …

2020 Physical Review D
Suzaku 35
A Suzaku sample of unabsorbed narrow-line and broad-line Seyfert 1 galaxies - I. X-ray spectral properties
DOI: 10.1093/mnras/staa2783 Bibcode: 2020MNRAS.498.5207W

Gallo, L. C.; Waddell, S. G. H.

A sample of narrow-line Seyfert 1 (NLS1) and broad-line Seyfert 1 (BLS1) galaxies observed with Suzaku is presented. The final sample consists of 22 NLS1s and 47 BLS1s, for a total of 69 active galactic nuclei (AGNs) that are all at low redshift (z < 0.5) and exhibit low host-galaxy column densities (<1022 ${\rm cm}^{-2}\,$ ). The…

2020 Monthly Notices of the Royal Astronomical Society
Suzaku 31
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