Search results for "Optical observation"
showing 3 items of 3 documents
Correlated optical and X-ray variability in CTTS
2010
Optical and X-ray emission from classical T Tauri stars (CTTSs) has long been known to be highly variable. Our long, uninterrupted optical observation of the NGC2264 region with CoRoT allows the optical variability in CTTS to be studied with unprecedented accuracy and time coverage. Two short Chandra observations obtained during the CoRoT pointing with a separation of 16 days allow us to study whether there is a correlation between optical and X-ray variability on this timescale, thus probing the physical mechanisms driving the variability in both bands. We have computed the optical and X-ray fractional variability between the two 30 ks duration windows covered by both the Chandra and CoRoT…
Single Gold Nanoparticle Growth Monitored in situ
2012
The novel fastSPS setup is used to study the growth process of rodshaped gold nanoparticles in the presence of surfactant molecules. It is observed that the particles grow mainly in the direction of the short rod axis, resulting in a decrease of the aspect ratio. This is, to the best of my knowledge, the first real-time optical observation of nanoparticle growth on a single-particle level (results were published in reference ). In collaboration with Olaf Schubert the nanoparticle growth was also monitored using the novel RotPOL setup. Here a decrease of the average polarization anisotropy \(PA\) is observed.
REFLEX Galaxy Cluster Survey catalogue
2004
We present the catalogue of the REFLEX Cluster Survey providing information on the X-ray properties, redshifts, and some identification details of the clusters in the REFLEX sample. The catalogue describes a statistically complete X-ray flux-limited sample of 447 galaxy clusters above an X-ray flux of 3x10^-12^erg/s/cm^2^ (0.1 to 2.4keV) in an area of 4.24ster in the southern sky. The cluster candidates were first selected by their X-ray emission in the ROSAT-All Sky Survey and subsequently spectroscopically identified in the frame of an ESO key programme. Previously described tests have shown that the sample is more than 90% complete and there is a conservative upper limit of 9% on the fra…