Search Publications

An X-Ray Detected Group of Quiescent Early-Type Galaxies at z = 1.6 in the Chandra Deep Field South
DOI: 10.1093/pasj/65.1.17 Bibcode: 2013PASJ...65...17T

Brandt, William N.; Mulchaey, John S.; Ueda, Yoshihiro +6 more

We report the discovery of an X-ray group of galaxies located at a high redshift of $ z$ $ =$ 1.61 in the Chandra Deep Field South. Based on 4 Ms Chandra data, the group is first identified…

2013 Publications of the Astronomical Society of Japan
XMM-Newton eHST 43
X-Ray and Optical Monitoring of a Gamma-Ray-Emitting Radio Galaxy, NGC 1275
DOI: 10.1093/pasj/65.2.30 Bibcode: 2013PASJ...65...30Y

Fukazawa, Yasushi; Yamazaki, Syoko; Sasada, Mahito +7 more

We performed monitoring observations of a gamma-ray-emitting radio galaxy, NGC 1275, in the X-ray and optical bands with the Suzaku/XIS, Kanata telescope, and the Okayama telescope. The X-ray flux of the nucleus was estimated by imaging spectroscopy in the hard X-ray band. In the optical band, a continuum flux, a broad Hα line flux, and the polari…

2013 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 20
An X-Ray Study of the Galactic-Scale Starburst-Driven Outflow in NGC 253
DOI: 10.1093/pasj/65.2.44 Bibcode: 2013PASJ...65...44M

Yamasaki, Noriko Y.; Mitsuishi, Ikuyuki; Takei, Yoh

The X-ray properties of hot interstellar gas in a bright, nearby edge-on starburst galaxy, NGC 253, were investigated so as to gain a further understanding of starburst-driven outflow activity by utilizing XMM-Newton and Suzaku. Spectroscopic analyses for three regions of the galaxy characterized by multiwavelength observations, i.e., the superwin…

2013 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 17
Distribution of Si, Fe, and Ni in the Intracluster Medium of the Coma Cluster
DOI: 10.1093/pasj/65.1.10 Bibcode: 2013PASJ...65...10M

Sato, Kosuke; Matsushita, Kyoko; Sato, Takuya +1 more

We studied the distributions of Si, Fe, and Ni in the intracluster medium (ICM) of the Coma cluster, one of the largest clusters in the nearby universe, using XMM-Newton data up to 0.5 r180 and Suzaku data of the central region up to 0.16 r180. Using the flux ratios of the Lyα line of H-like Si and the 7.8 keV line blend to t…

2013 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 14
Suzaku Detection of Thermal X-Ray Emission Associated with the Western Radio Lobe of Fornax A
DOI: 10.1093/pasj/65.5.106 Bibcode: 2013PASJ...65..106S

Tashiro, Makoto S.; Inoue, Susumu; Seta, Hiromi

We present the results of X-ray mapping observations of the western radio lobe of the Fornax A galaxy, using the X-ray Imaging Spectrometer (XIS) onboard the Suzaku satellite with a total exposure time of 327 ks. The purpose of this study is to investigate the nature and spatial extent of the diffuse thermal emission around the lobe by exploiting …

2013 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 11
An X-Ray Counterpart of HESS J1427-608 Discovered with Suzaku
DOI: 10.1093/pasj/65.3.61 Bibcode: 2013PASJ...65...61F

Dotani, Tadayasu; Terada, Yukikatsu; Matsumoto, Hironori +9 more

We report on the discovery of an X-ray counterpart of the unidentified very high-energy gamma-ray source HESS J1427-608. In the sky field coincident with HESS J1427-608, an extended source was found in the 2-8 keV band, and was designated as Suzaku J1427-6051. Its X-ray radial profile has an extension of σ = 0.'9 ± 0.'1 if approximated by a Gaussi…

2013 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 9
Two Power-Law States of the Ultraluminous X-Ray Source IC 342 X-1
DOI: 10.1093/pasj/65.2.48 Bibcode: 2013PASJ...65...48Y

Isobe, Naoki; Kubota, Aya; Mineshige, Shin +3 more

In order to elucidate the emission properties of ultraluminous X-ray sources (ULXs) during their power-law (PL) state, we examined long-term X-ray spectral data of IC 342 X-1 during its PL state by using our own Suzaku data and archival data by XMM-Newton, Chandra, and Swift observations. The PL state of this source seems to be classified into two…

2013 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 9
X-Ray Observation of the Galactic Supernova Remnant G355.6-0.0 with Suzaku
DOI: 10.1093/pasj/65.5.99 Bibcode: 2013PASJ...65...99M

Koyama, Katsuji; Ota, Naomi; Yamauchi, Shigeo +1 more

We present results of the Galactic supernova remnant (SNR) G355.6-0.0 observed with Suzaku. We resolved diffuse emission detected with ASCA into two objects, G355.6-0.0 and a point-like source, Suzaku J173530-3236. The X-ray emission from G355.6-0.0 exhibits a center-filled morphology within the radio shell. The X-ray spectrum is well-represented …

2013 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 8
Detection of a 522 s Pulsation from the Transient X-Ray Source Suzaku J0102.8-7204 (SXP 523) in the Small Magellanic Cloud
DOI: 10.1093/pasj/65.2.L2 Bibcode: 2013PASJ...65L...2W

Miller, Eric D.; Tsujimoto, Masahiro; Wada, Qazuya +1 more

During a routine calibration observation of 1E 0102.2-7219 in the Small Magellanic Cloud (SMC), carried out in 2012 October for the Suzaku satellite, we detected a transient X-ray source at (RA, Dec) = (01h 02m47s, - 72°04m54s) in the equinox J2000.0 with a positional uncertainty of ∼1.4". We …

2013 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 3
Metals in the Intracluster Medium of MS 1512.4+3647 Observed with Suzaku: Implications for the Metal Enrichment History
DOI: 10.1093/pasj/65.5.111 Bibcode: 2013PASJ...65..111S

Sato, Kosuke; Tashiro, Makoto S.; Ohashi, Takaya +5 more

The cluster of galaxies MS 1512.4+3647 (z = 0.372) was observed with Suzaku for 270 ks. Besides the Fe abundance, the abundances of Mg, Si, S, and Ni were separately determined for the first time in a medium redshift cluster (z > 0.3). The derived abundance pattern of MS 1512.4+3647 is consistent with those of nearby clusters, suggesting that t…

2013 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 0