Search Publications

Suzaku Detection of Extended/Diffuse Hard X-Ray Emission from the Galactic Center
DOI: 10.1093/pasj/60.sp1.S207 Bibcode: 2008PASJ...60S.207Y

Maeda, Yoshitomo; Kokubun, Motohide; Makishima, Kazuo +12 more

Five on-plane regions within ±0°.8 of the galactic center were observed with the Hard X-ray Detector (HXD) and the X-ray Imaging Spectrometer (XIS) aboard Suzaku. From all regions, significant hard X-ray emission was detected with HXD-PIN up to 40keV, in addition to the extended plasma emission which is dominant in the XIS band. The hard X-ray sig…

2008 Publications of the Astronomical Society of Japan
INTEGRAL Suzaku 24
Suzaku Observation of the Metallicity in the Hot Interstellar Medium of the Isolated Elliptical Galaxy NGC 720
DOI: 10.1093/pasj/60.sp1.S307 Bibcode: 2008PASJ...60S.307T

Fukazawa, Yasushi; Anabuki, Naohisa; Matsushita, Kyoko +3 more

The metal abundances in the interstellar medium of the isolated elliptical galaxy NGC 720 were studied with the CCD X-ray Imaging Spectrometer (XIS) aboard the Suzaku satellite. The high detection efficiency along with the excellent spectral resolution of the XIS allowed the K-shell lines of O and Mg to be clearly resolved, and the abundances of O…

2008 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 23
Suzaku X-Ray Spectroscopy of a Peculiar Hot Star in the Galactic Center Region
DOI: 10.1093/pasj/60.sp1.S173 Bibcode: 2008PASJ...60S.173H

Nagata, Tetsuya; Tsujimoto, Masahiro; Koyama, Katsuji +5 more

We present the results of a Suzaku study of a bright point-like source in the 6.7keV intensity map of the Galactic center region. We detected an intense FeXXV 6.7keV line with an equivalent width of ∼1keV as well as emission lines of highly ionized Ar and Ca from a spectrum obtained by the X-ray Imaging Spectrometer. The overall spectrum is descri…

2008 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 20
Performance of an Imaging Fourier Transform Spectrometer with Photoconductive Detector Arrays: An Application for the AKARI Far-Infrared Instrument
DOI: 10.1093/pasj/60.sp2.S389 Bibcode: 2008PASJ...60S.389K

Nakagawa, Takao; Shirahata, Mai; Doi, Yasuo +10 more

We have developed an imaging Fourier transform spectrometer (FTS) for space-based far-infrared astronomical observations. The FTS employs newly developed photoconductive detector arrays with acapacitive trans-impedance amplifier, which makes the FTS acompletely unique instrument. The FTS was installed as afunction of the far-infrared instrument (F…

2008 Publications of the Astronomical Society of Japan
AKARI 18
Galaxy Clusters at 0.9 < z < 1.7 in the AKARI NEP Deep Field
DOI: 10.1093/pasj/60.sp2.S531 Bibcode: 2008PASJ...60S.531G

Goto, Tomotsugu; Inami, Hanae; Nakagawa, Takao +11 more

There is ahuge gap between the properties of red-sequence selected massive galaxy clusters at z < 1 and Lyman-break selected proto-clusters at z > 3. It is important to understand when and how the z > 3 proto-clusters evolve into passive clusters at z < 1. We aim to fill this cluster desert by using space-based N4 (4 µm) imaging …

2008 Publications of the Astronomical Society of Japan
AKARI 17
Abundance Inhomogeneity in the Northeastern Rim of the Cygnus Loop Revealed by the Suzaku Observatory
DOI: 10.1093/pasj/60.sp1.S115 Bibcode: 2008PASJ...60S.115K

Miller, Eric D.; Katsuda, Satoru; Uchida, Hiroyuki +5 more

We present the results of a spatially resolved spectral analysis from four Suzaku observations covering the northeastern rim of the Cygnus Loop. A two-kTe non-ionization equilibrium (NEI) model fairly well represents our data, which confirms the NEI condition of the plasma there. The metal abundances are depleted relative to the solar v…

2008 Publications of the Astronomical Society of Japan
Suzaku 17
Suzaku Observation of G359.79-0.26, a New Supernova Remnant Candidate in the Galactic Center
DOI: 10.1093/pasj/60.sp1.S183 Bibcode: 2008PASJ...60S.183M

Mori, Hideyuki; Koyama, Katsuji; Tsuru, Takeshi Go +2 more

Utilizing Suzaku observations, we obtained the X-ray spectrum of G359.79-0.26, an extended X-ray feature nearby the Galactic center (GC) supernova remnant (SNR) SgrA East. We estimated the contribution from the Galactic center diffuse X-rays, which allows us a proper background subtraction from the faint extended source. A thin thermal plasma with…

2008 Publications of the Astronomical Society of Japan
Suzaku 16
Discovery of a Bright Transient Ultraluminous X-Ray Source, Suzaku J1305-4931 in NGC4945
DOI: 10.1093/pasj/60.sp1.S241 Bibcode: 2008PASJ...60S.241I

Isobe, Naoki; Gandhi, Poshak; Makishima, Kazuo +5 more

An X-ray source, Suzaku J1305-4931, was discovered in the south-west arm of a nearby Seyfert II galaxy, NGC4945, at 0.5-10keV flux of 2.2×10-12erg cm-2 s-1 during a Suzaku observation conducted on 2006 January 15-17. It was undetectable in a shorter observation on 2005 August 22--23, with an upper limit of 1.7×10

2008 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 15
Asymmetric Ejecta Distribution of the Cygnus Loop Revealed with Suzaku
DOI: 10.1093/pasj/60.sp1.S107 Bibcode: 2008PASJ...60S.107K

Miller, Eric D.; Katsuda, Satoru; Mori, Koji +4 more

We observed a linearly sliced area of the Cygnus Loop from the north-east to the south-west with Suzaku in seven pointings. After dividing the entire fields of view (FOV) into 119 cells, we extracted spectra from all of the cells and performed spectral analysis for them. We then applied both one- and two-component non-equilibrium ionization (NEI) …

2008 Publications of the Astronomical Society of Japan
Suzaku 14
An AKARI Search for Intracluster Dust of Globular Clusters
DOI: 10.1093/pasj/60.sp2.S415 Bibcode: 2008PASJ...60S.415M

Yamamura, Issei; Matsunaga, Noriyuki; Mito, Hiroyuki +7 more

We report on observations of 12 globular clusters with the Far-Infrared Surveyor (FIS) aboard the AKARI satellite. Our goal is to search for emission from cold dust within clusters. We detected diffuse emissions toward NGC6402 and 2808, but the IRAS 100µm maps show the presence of strong background radiation. They are likely to have been emi…

2008 Publications of the Astronomical Society of Japan
AKARI eHST 14