Search Publications

The Subaru-XMM-Newton Deep Survey (SXDS). VIII. Multi-wavelength identification, optical/NIR spectroscopic properties, and photometric redshifts of X-ray sources
DOI: 10.1093/pasj/psv050 Bibcode: 2015PASJ...67...82A

Ouchi, Masami; Simpson, Chris; Curtis-Lake, Emma +27 more

We report on the multi-wavelength identification of the X-ray sources found in the Subaru-XMM-Newton Deep Survey (SXDS) using deep imaging data covering the wavelength range between the far-UV and mid-IR (MIR). We select a primary counterpart of each X-ray source by applying the likelihood ratio method to R-band, 3.6 µm, near-UV, and 24 &mic…

2015 Publications of the Astronomical Society of Japan
ISO XMM-Newton 31
Discovery of a nearby early-phase major cluster merger CIZA J1358.9-4750
DOI: 10.1093/pasj/psv029 Bibcode: 2015PASJ...67...71K

Makishima, Kazuo; Nakazawa, Kazuhiro; Gu, Liyi +4 more

CIZA J1358.9-4750 is a nearby (z = 0.074) pair of clusters of galaxies located close to the Galactic plane. It consists of two X-ray extended humps at the northwest and the southeast separated by 14' (∼ 1.2 Mpc), and an X-ray bright bridgelike structure in between. With Suzaku, the south east hump was shown to have a temperature of 5.6 ± 0.2 keV a…

2015 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 13
Suzaku observations of the old pulsar wind nebula candidate HESS J1356-645
DOI: 10.1093/pasj/psv013 Bibcode: 2015PASJ...67...43I

Dotani, Tadayasu; Bamba, Aya; Hiraga, Junko S. +3 more

A largely extended X-ray emission was discovered around the pulsar PSR J1357-6429 with the Suzaku deep observations. The pulsar, whose characteristic age is 7.3 kyr, is located within the TeV γ-ray source HESS J1356-645. The extended emission is found to have a 1 σ X-ray size of ∼ 4', or ∼ 3 pc at 2.4 kpc, with a small offset from the pulsar. Its …

2015 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 3