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Kilosecond

Known as: 10^3 sec, ks, ksec 
A unit of time equal to one thousand seconds (10E3 seconds).
National Institutes of Health

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Clinical Data Interchange Standards Consortium Terminology

Papers overview

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Review
2012
Review
2012
CHANDRA OBSERVATIONS OF 3C RADIO SOURCES WITH z < 0.3. II. COMPLETING THE SNAPSHOT SURVEY
We report on the second round of Chandra observations of the 3C snapshot survey developed to observe the complete sample of 3C… 
2012
2012
DISCOVERY OF HIGH-FREQUENCY QUASI-PERIODIC OSCILLATIONS IN THE BLACK HOLE CANDIDATE IGR J17091−3624
We report the discovery of 8.5σ high-frequency quasi-periodic oscillations (HFQPOs) at 66 Hz in the Rossi X-ray Timing Explorer… 
Highly Cited
2010
Highly Cited
2010
XMM-NEWTON OBSERVATION OF THE NORTHWEST RADIO RELIC REGION IN A3667
A3667 is the archetype of a merging cluster with radio relics. The northwest (NW) radio relic is the brightest cluster relic or… 
2009
2009
SUZAKU WIDE BAND ANALYSIS OF THE X-RAY VARIABILITY OF TeV BLAZAR Mrk 421 IN 2006
We present the results of X-ray observations of the well studied TeV blazar Mrk 421 with the Suzaku satellite in 2006 April 28… 
Review
2008
Review
2008
EXPLORING THE SMALL MAGELLANIC CLOUD TO THE FAINTEST X-RAY FLUXES: SOURCE CATALOG, TIMING, AND SPECTRAL ANALYSIS
We present the results of a pair of 100 ks Chandra observations in the Small Magellanic Cloud (SMC) to survey high-mass X-ray… 
2004
2004
Chandra Observations of the Accretion-driven Millisecond X-Ray Pulsars XTE J0929–314 and XTE J1751–305 in Quiescence
We observed the accretion-driven millisecond X-ray pulsars XTE J0929-314 and XTE J1751-305 in their quiescent states using… 
2003
2003
XMM-Newton observations of the Perseus Cluster I: The temperature and surface brightness structure
We present preliminary results of the XMM-Newton 50 ksec observation of the Perseus cluster which provides an unprecedented view… 
Review
2003
Review
2003
A Deep Chandra X-Ray Observation of the Embedded Young Cluster in NGC 2024
We present results of a sensitive 76 ks Chandra observation of the young stellar cluster in NGC 2024, lying at a distance of ~415… 
2001
2001
Identification of the Low-Mass X-Ray Binary and Faint X-Ray Sources in NGC 6652
We have detected three new X-ray point sources, in addition to the known low-mass X-ray binary (LMXB) X1832-330, in the globular… 
1999
1999
Accepted for publication in the Astronomical Journal, February 2000 The Hubble Deep Field South – STIS Imaging 1.
  • 1999
  • Corpus ID: 15724697
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