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  1. Science in China Series G
  2. Science in China Series G : Volume 53
  3. Science in China Series G : Volume 53, Issue 1, Supplement,January 2010
  4. SVOM gamma ray monitor
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Science in China Series G : Volume 60
Science in China Series G : Volume 59
Science in China Series G : Volume 58
Science in China Series G : Volume 57
Science in China Series G : Volume 56
Science in China Series G : Volume 55
Science in China Series G : Volume 54
Science in China Series G : Volume 53
Science in China Series G : Volume 53, Issue 12, December 2010
Science in China Series G : Volume 53, Issue 11, November 2010
Science in China Series G : Volume 53, Issue 10, October 2010
Science in China Series G : Volume 53, Issue 9, September 2010
Science in China Series G : Volume 53, Issue 8, August 2010
Science in China Series G : Volume 53, Issue 7, July 2010
Science in China Series G : Volume 53, Issue 6, June 2010
Science in China Series G : Volume 53, Issue 5, May 2010
Science in China Series G : Volume 53, Issue 4, April 2010
Science in China Series G : Volume 53, Issue 3, March 2010
Science in China Series G : Volume 53, Issue 2, February 2010
Science in China Series G : Volume 53, Issue 1, Supplement,January 2010
Editorial
Observational features of pulsar glitches
Formation and evolution of X-ray binaries
Gamma-ray bursts in the Swift-Fermi era: Confronting data with theory
Some developments of hot accretion flow theory in the past ten years
Observation constraints of the hard X-ray modulation telescope HXMT
Calibrating the HXMT collimators using diffuse illumination
SVOM gamma ray monitor
Light collection of the POLAR detector
Simulation of the in-flight calibration of the collimator alignment and PSF for HXMT
A fast onboard star-extraction algorithm optimized for the SVOM Visible Telescope
Three years’ systematic GRB follow-up at the Xinglong Observatory and the optical afterglow observations of GRB 080330
The time lag spectrum of Cir X-1 on its normal branch
GRB 090423: Marking the death of a massive star at z=8.2
Correlation between pulse-width and peak luminosity of single-pulse long gamma-ray bursts
Spectral properties of Fermi/GBM gamma-ray bursts and the GeV emission detection rate with Fermi/LAT
The flux-E $_{p}$ relation within GRB060218 in comparison with typical GRB pulses
An analytic relation for the thickness of accretion flows
The rms-flux relation of Cyg X-2 in the horizontal branch
A model for the optical flares from the Galactic transient SWIFT J195509+261406
Afterglow from GRB 070610/Swift J195509.6+261406: An explanation using the fireball model
A toy model for magnetized neutrino-dominated accretion flows
A statistical study of the relation between soft X-ray excess and accretion disk
Energy dissipation and angular momentum transfer within a magnetically torqued accretion disc
The flux modulation of INTEGRAL
The emission positions of kHz QPOs and Kerr spacetime influence
A black hole preying on the star for a gamma-ray burst of GRB080503: Evidence for the second event in this new class
Temporal study of GRS 1915+105 with rms-flux relation: The importance of magnetic activities in the corona
The low-mass X-ray binary-millisecond radio pulsar birthrate problem revisited
An alternative evolution scenario for OAO 1657-415 and IGR J18483-0311
High-energy radiation from old pulsars
On the effect of injection of gas in the numerical simulation of accretion flows
Optical observations of Scorpius X-1 in 2008: Evidence of rapid variability
Spectral states and state preference of galactic X-ray binaries
Hard X-ray lags of Cygnus X-1 on short timescales
Optical results of the black hole microquasar SS 433
The early high-energy afterglow emission from short GRBs
The correlation timescale of the X-ray flux during the outbursts of soft X-ray transients
Numerical simulation of hot accretion flows with thermal conduction
The new model of fitting the spectral energy distributions of Mrk 421 and Mrk 501
Bifurcation timescales in power spectra of black hole binaries and ultraluminous X-ray sources
Deprojection technique for galaxy cluster considering the point spread function
The radio structure of BL Lac object S5 2007+777
Luminosity function of optically-selected type II QSOs
Diagnostics for the structure of AGNs’ broad line regions with reverberation mapping data: confirmation of the two-component broad line region model
Synchrotron peak luminosity, black hole mass and Eddington ratio for SDSS flat-spectrum radio quasars
Multi-epoch X-ray observations of the narrow-line Seyfert 1 galaxy SDSS J160508.87+323921.4 with XMM-Newton
The X-ray emission from the knots in 3C 120
New insights into AGNs with low-mass black holes and high accretion rates: the case of narrow-line Seyfert 1 galaxies
Statistical study of the pulse width distribution for radio pulsars
Discovery of a high confidence soft lag from an X-ray flare of Markarian 421
A mathematical method for the de-dispersion of the pulsar profile
A study of a sequence of blazars from FSRQs to BL Lac objects
Accretion/jet activity and narrow [O III] kinematics in young radio galaxies
The relationship of extended radio power and broad emission line luminosity in blazars
Progress of research on AGNs at the Urumqi Observatory
Predicting neutron star spins from twin kHz QPOs
Decomposition of the X-ray waveform of soft gamma-ray repeaters during giant flares
The periodicity of 3C 273’s radio light curve at 15 GHz found by the wavelet method
Morphology and the M $_{BH}$-σ* relation for NLS1s
Constraint on the counter-jet emission in gamma-ray burst afterglows from GRB 980703
Magnetic energy injection in GRB 080913
Evidence of a two-component jet in the afterglow of GRB 070419A
Spatial distribution of metal emissions in supernova remnant 3C 397 viewed with Chandra and XMM
An MSX infrared analysis of the superbubble around the giant HII region NGC3603
Science in China Series G : Volume 53, Issue 1, January 2010
Science in China Series G : Volume 52
Science in China Series G : Volume 51
Science in China Series G : Volume 50
Science in China Series G : Volume 49
Science in China Series G : Volume 48
Science in China Series G : Volume 47
Science in China Series G : Volume 46

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SVOM gamma ray monitor

Content Provider Springer Nature Link
Author Dong, YongWei Wu, BoBing Li, YanGuo Zhang, YongJie Zhang, ShuangNan
Copyright Year 2010
Abstract The space-based multi-band astronomical Variable Object Monitor (SVOM) mission is dedicated to the detection, localization and broad-band study of gamma-ray bursts (GRBs) and other high-energy transient phenomena. The gamma ray monitor (GRM) onboard is designed to observe GRBs up to 5 MeV. With this instrument, one of the key GRB parameters, E $_{peak}$, can be easily measured in the hard X-ray band. It can achieve a detection rate of 100 GRBs per year which ensures the scientific output of SVOM.
Starting Page 40
Ending Page 42
Page Count 3
File Format PDF
ISSN 16747348
Journal Science in China Series G
Volume Number 53
Issue Number 1
e-ISSN 18622844
Language English
Publisher SP Science China Press
Publisher Date 2010-05-20
Publisher Place Heidelberg
Access Restriction One Nation One Subscription (ONOS)
Subject Keyword gamma-ray burst E $_{peak}$ triple phoswich Astronomy, Observations and Techniques Classical Continuum Physics Physics
Content Type Text
Resource Type Article
Subject Physics and Astronomy
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