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Chapter and Conference Paper
Coordinated Optical-Exosat-Tenma Observations of a Burst from 2S1636-536
During a coordinated observations of 2S1636-536 with EXOSAT, Tenma and the 1.4 metre Danish telescope at La Silla, a single burst was detected at all three observatories. The burst was bright with a peak flux ...
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Article
Variations of the pulse profile and the X-ray intensity of GX301-2 (4U1223-62)
Two successive X-ray outbursts of the recurrent X-ray pulsar GX301-2 were observed in April and May, 1982 from Hakucho. Apart from general increase during flares lasting for several days, the X-ray intensity w...
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Chapter and Conference Paper
Subpicosecond Accumulated Photon Echoes with Incoherent Light in Nd3+-Doped Silicate Glass
Since the first observation of accumulated photon echoes by HESSELINK and WIERSMA [1], nearly transform-limited mode-locked pulse trains have been used as the excitation source, and the resolution times have b...
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Article
Hard X-ray structure of the Crab Nebula
Two-dimensional maps of the Crab Nebula have been synthesized in 22–64 keV range through the modulation collimator experiment. The effective angular resolution is about 15″. The result indicates that the Crab ...
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Chapter and Conference Paper
Hard X-Ray Structure of the Crab Nebula
Two-dimensional maps of the Crab Nebula have been synthesized in 22–64 keV range through the modulation collimator experiment. The effective angular resolution is about 15″. The result indicates that the Crab ...
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Article
Backward echo and FID in two-level systems
Generation of backward photon echoes and proposed backward optical free induction decays is discussed in detail. Separation of the signals from excitation pulses by propagation and polarization directions sugg...
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Chapter and Conference Paper
Picosecond Backward Echo in Sodium Vapor — Relaxation and Quantum Beat Modulation
The backward echo [1–3] is a three-pulse stimulated photon echo produced backward to either one or two of the excitation pulses kee** the phase matching conditions among the three excitation pulses and the e...
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Article
The balloon observations of small cosmic X-ray bursts
In the record of the balloon observation which was performed on 27 September, 1970, a transient burst of X-rays was found. This event is concluded to be a cosmic gamma-ray burst of a smaller size or of a large...
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Article
Size of the hard X-ray source in the Crab Nebula
The size of the hard X-ray source in the Crab Nebula was observed with scintillation counters on board two balloons at a lunar occulatation on 24 January, 1975. The Gaussian width of the source is 34″ (+17″, −...
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Article
Time variations of hard X-rays from Sco X-1
Simultaneous hard X-ray and optical observations of Sco X-1 were carried out on 1971 May 1 at Hyderabad, India, when Sco X-1 was optically bright. The X-ray intensity observed by balloon-borne counter telescop...
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Article
Time variation of the X-ray spectrum and optical luminosity of SCO X-1
Results of rocket observations of SCO X-1 over the spectral range of 2∼20 keV are presented. The observations have been performed partly in India and partly in Japan under the collaboration of the three groups...
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Article
Observation of cosmic soft X-rays
Cosmic soft X-rays in the energy range between 0.14 and 7 keV were observed with thin polypropylene window proportional counters on board a sounding rocket. The field of view crossed the galactic plane in the ...
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Article
The location and size of a solar hard X-ray burst on September 27, 1969
The location and size of a solar impulsive hard X-ray burst have been determined in one dimension to a considerable precision with a balloon-borne X-ray modulation collimator. The center of the X-ray source is...
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Chapter
Angular Size and Position of the X-ray Source Cyg-X-1
We performed a couple of balloon experiments to measure the size and the location of Cyg-X-1 using the techniques of the modulation collimator [1]. The angular periods of the modulation collimator were 26′ and...
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Chapter
A Rocket Observation of Cosmic X-rays in the Energy Range between 0.15 and 20 keV
Cosmic X-rays were observed with three sets of proportional counters covering the energy range between 0.15 and 20 keV. The detector born on a spinning rocket scanned a celestial region in which the galactic l...
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Article
Measurement of the absolute intensity of cosmic X-rays
The intensity of the diffuse component of cosmic X-rays was measured with use of a rotating collimator system borne on a sounding rocket. A part of background counts proportional to the field of view of propor...
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Article
Galactic X-rays