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A3667 is the archetype of a merging cluster with radio relics. The northwest (NW) radio relic is the brightest cluster relic or… Expand We use a long (300 ks), continuous Suzaku X-ray observation of the active nucleus in NGC 1365 to investigate the structure of the… Expand Here we describe the first results of the Advanced Large Homogeneous Area Medium-Band Redshift Astronomical (ALHAMBRA) survey… Expand Aims. This paper's goal is to improve the member census of the NGC 2264 star-forming region and study the origin of X-ray… Expand We search 0.02 deg 2 of the invariable plane for trans-Neptunian objects (TNOs) 25 AU or more distant using the Advanced Camera… Expand We study the long term evolution of the relationship between the root mean square (rms) variability and flux (the "rms-flux… Expand We present preliminary results of a XMM-Newton 50 ks observation of the Perseus Cluster that provides an unprecedented view of… Expand We present a detailed model for the ionized absorbing gas evident in the 900 ks Chandra HETGS spectrum of NGC 3783. The analysis… Expand We present the main results from our 940 ksec observation of the Chandra Deep Field South (CDFS), using the source catalog… Expand Myoglobin rebinding of carbon monoxide and dioxygen after photodissociation has been observed in the temperature range between 40… Expand