activity
19962023
most citedThe MAXI Mission on the ISS: Science and Instruments for Monitoring All Sky X-Ray Images

845 citations · 3.4k across the 97 of their papers we have counts for

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12 papers · 1 filter

astro-ph2008★ 27 cited

Suzaku Observations of SGR 1900+14 and SGR 1806-20

Yujin E. Nakagawa, Tatehiro Mihara, Atsumasa Yoshida +8

Spectral and timing studies of Suzaku ToO observations of two SGRs, 1900+14 and 1806-20, are presented. The X-ray quiescent emission spectra were well fitted by a two blackbody fun…

astro-ph2007★ 9 cited

Suzaku Observation of the Anomalous X-ray Pulsar CXOU J164710.2--455216

Sachindra Naik, Tadayasu Dotani, Nobuyuki Kawai +11

Suzaku TOO observation of the anomalous X-ray pulsar CXOU J164710.2-455216 was performed on 2006 September 23--24 for a net exposure of 38.8 ks. During the observation, the XIS was…

astro-ph2007★ 27 cited

Broad band X-ray spectroscopy of A0535+262 with SUZAKU

S. Naik, T. Dotani, Y. Terada +9

The transient X-ray binary pulsar A0535+262 was observed with Suzaku on 2005 September 14 when the source was in the declining phase of the August-September minor outburst. The ~10…

astro-ph2007★ 40 cited

Suzaku Observations of Hercules X-1 : Measurements of the Two Cyclotron Harmonics

Teruaki Enoto, Kazuo Makishima, Yukikatsu Terada +10

The accretion-powered pulsar Her X-1 was observed with Suzaku twice in its main-on state, on 2005 October 5-6 and 2006 March 29-30, for a net exposure of 30.5 ks and 34.4 ks, respe…

astro-ph2004

A search for cyclotron resonance features with INTEGRAL

Y. Okada, H. Niko, M. Kokubun +6

We present an INTEGRAL observation of the Cen-Crux region in order to search the electron cyclotron resonance scattering features from the X-ray binary pulsars. During the AO1 200k…

astro-ph2001★ 41 cited

NGC 4151: an intrinsically average Seyfert 1

Andrzej A. Zdziarski, Karen M. Leighly, Masaru Matsuoka +2

We present a detailed analysis of a long, 100 ksec, observation of NGC 4151 by ASCA, contemporaneous with an observation by the CGRO/OSSE. We fit the data with physical models incl…

astro-ph2001★ 25 cited

A Rapid X-ray Flare in the Radio-loud Narrow Line Quasar PKS 0558-504

T. G. Wang, M. Matsuoka, T. Kubo +2

We report the detection of a very short time scale flare in the radio-loud narrow line quasars PKS 0558-504 by using ASCA. The X-ray count rates increased and decreased by a factor…

astro-ph2000★ 32 cited

Evidence of thick obscuring matter revealed in the X-ray spectrum of the Z=4.28 quasar RXJ1028.6-0844

W. Yuan, M. Matsuoka, T. Wang +3

We report the discovery of an unambiguous, substantial low-energy cutoff in the broad band X-ray spectrum of the radio quasar RXJ1028.6-0844 at a redshift of 4.276 obtained with th…

astro-ph1999★ 6 cited

Detection of Iron Emission Line from the Galaxy Cluster Including the Radio Galaxy 3C220.1 at z=0.62

Naomi Ota, Kazuhisa Mitsuda, Makoto Hattori +1

We have detected an emission line feature at 4 keV in the X-ray emission from a sky region including the distant radio galaxy 3C220.1(z=0.62) obtained with ASCA. The line energy is…

astro-ph1999★ 2 cited

A BeppoSAX study of the pulsating transient X0115+63: the first X-ray spectrum with four cyclotron harmonic features

A. Santangeo, A. Segreto, S. Giarrusso +9

The recurrent hard pulsating X-ray transient §was observed with \B on March 19, when the source was at a 2--10 keV flux level of 310~mCrab. We report on the high energy spect…

astro-ph1998★ 29 cited

ASCA Observations of the Seyfert 2 Galaxy NGC 7582: An Obscured and Scattered View of the Hidden Nucleus

S. -J. Xue, C. Otani, T. Mihara +2

ASCA observations of the Seyfert 2 galaxy NGC 7582 revealed it was highly variable on the timescale of s in the hard X-ray (2-10 keV) band, while the soft X-ray (…

astro-ph1996★ 58 cited

Spectral Variability and iron line emission in the ASCA Observations of the Seyfert 1 Galaxy NGC4051

Matteo Guainazzi, Tatehiro Mihara, Chiko Otani +1

We present the results of an extensive analysis of the ``ASCA'' AO2 observation of the Seyfert 1 galaxy NGC4051. The target exhibits broadband [0.5--10 keV] variability by a factor…