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Self-Charge-Filling (SCF) Effect of Suzaku XIS
DOI: 10.1093/pasj/64.5.101 Bibcode: 2012PASJ...64..101T

Kitamoto, Shunji; Murakami, Hiroshi; Yoshida, Yuki +1 more

We demonstrate the importance of the self-charge-filling (SCF) effect for the analysis of bright and line-rich sources with the Suzaku X-ray imaging spectrometer (XIS) if spaced-row charge injection (SCI) is not applied. The SCF-effect changes the central energy of lines depending on the extracted region or the event densities of the images. We pr…

2012 Publications of the Astronomical Society of Japan
Suzaku 3
Suzaku Observations of Abell 1555 and Abell 1558: Searching for Non-Thermal Emission from Large-Scale Structure Formation
DOI: 10.1093/pasj/64.5.113 Bibcode: 2012PASJ...64..113M

Nakazawa, Kazuhiro; Makiya, Ryu; Totani, Tomonori

We report on X-ray observations of two galaxy clusters, Abell 1555 and Abell 1558, with Suzaku, which are included in a large-scale filamentary structure and a supercluster, to search for non-thermal emission driven by shocks produced during structure formation. These two clusters were detected by Suzaku/XIS for the first time in the X-ray band of…

2012 Publications of the Astronomical Society of Japan
Suzaku 2
Chromospheric Running Wave from a Solar Cyclone Produced through the Emergence of a Twisted Magnetic Flux Tube
DOI: 10.1093/pasj/64.5.L4 Bibcode: 2012PASJ...64L...4M

Magara, Tetsuya; Inoue, Satoshi; Lee, Hwanhee +3 more

An innovative solar observing satellite, Hinode, has successfully observed the detailed evolution of an emerging magnetic field, starting from its appearance at the solar surface, to forming a developed bipolar region. The high spatial and temporal resolutions provided by the satellite has enabled us to capture prominent dynamic phenomena caused b…

2012 Publications of the Astronomical Society of Japan
Hinode 1
Erratum: X-Ray Study of the Outer Region of Abell 2142 with Suzaku
DOI: 10.1093/pasj/64.4.90 Bibcode: 2012PASJ...64...90A

Hoshino, Akio; Sato, Kosuke; Ohashi, Takaya +4 more

In the paper [PASJ 63, S1019 (2012)], there was an error in the estimation of gas mass. The correct gas mass at the virial radius is 2.40±0.20 × 1014 M. Thus, the gas mass fraction also changes from 14.4+7.1-4.1% to 21.8+10.7-6.3%. Although this value is still consistent with the w…

2012 Publications of the Astronomical Society of Japan
Suzaku 0