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相关论文: Composition of the Chandra ACIS contaminant

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The Chandra X-ray Observatory was launched almost 19 years ago and has been delivering spectacular science over the course of its mission. The Advanced CCD Imager Spectrometer is the prime instrument on the satellite, conducting over 90% of…

天体物理仪器与方法 · 物理学 2018-09-10 Paul P. Plucinsky , Akos Bogdan , Herman L. Marshall , Neil W. Tice

The Advanced CCD Imaging Spectrometer (ACIS) is one of two focal-plane instruments on the Chandra X-ray Observatory. During initial radiation-belt passes, the exposed ACIS suffered significant radiation damage from trapped soft protons…

天体物理仪器与方法 · 物理学 2015-05-19 C. E. Grant , B. LaMarr , M. W. Bautz , S. L. O'Dell

Soon after launch, the Advanced CCD Imaging Spectrometer (ACIS), one of the focal plane instruments on the Chandra X-ray Observatory, suffered radiation damage from exposure to soft protons during passages through the Earth's radiation…

天体物理学 · 物理学 2009-11-11 C. E. Grant , M. W. Bautz , S. M. Kissel , B. LaMarr , G. Y. Prigozhin

As the Advanced CCD Imaging Spectrometer (ACIS) on the Chandra X-ray Observatory enters its fifteenth year of operation on orbit, it continues to perform well and produce spectacular scientific results. The response of ACIS has evolved over…

天体物理仪器与方法 · 物理学 2015-06-22 Catherine E. Grant , Mark W. Bautz , Peter G. Ford , Paul P. Plucinsky

Soon after launch, the Advanced CCD Imaging Spectrometer (ACIS), one of the focal plane instruments on the Chandra X-ray Observatory, suffered radiation damage from exposure to soft protons during passages through the Earth's radiation…

天体物理学 · 物理学 2009-11-10 C. E. Grant , M. W. Bautz , S. M. Kissel , B. LaMarr

An 80 ksec Chandra ACIS observation of the radio galaxy 3C 452 is reported. A diffuse X-ray emission associated with the lobes has been detected with high statistical significance, together with the X-ray nucleus of the host galaxy. The…

天体物理学 · 物理学 2009-11-07 N. Isobe , M. Tashiro , K. Makishima , N. Iyomoto , M. Suzuki , M. M. Murakami , M. Mori , K. Abe

Chandra X-Ray Observatory (CXO) ACIS-S spectra of three quasars which lie behind three foreground damped Lyman alpha (DLA) absorbers are analyzed in order to attempt to determine the amount of photoelectric absorption due to metals present…

天体物理学 · 物理学 2009-11-07 David A. Turnshek , Sandhya M. Rao , Andrew F. Ptak , Richard E. Griffiths , Eric M. Monier

We discuss the flight calibration of the spectral response of the Advanced CCD Imaging Spectrometer (ACIS) on-board the Chandra X-ray Observatory (CXO). The spectral resolution and sensitivity of the ACIS instrument have both been evolving…

Molecules and particles make up $\sim 40 - 70\%$ of carbon in the interstellar medium, yet the exact chemical structure of these constituents remains unknown. We present carbon K-shell absorption spectroscopy of the Galactic Interstellar…

高能天体物理现象 · 物理学 2023-05-31 John Staunton , Frits Paerels

With the recent radioastronomical detection of cis-trans-carbonic acid (H$_2$CO$_3$) in a molecular cloud toward the galactic center, the more stable but currently unobserved cis-cis conformer is shown here to have strong IR features. While…

星系天体物理 · 物理学 2024-01-25 Ryan C. Fortenberry , Vincent J. Esposito

Elemental abundances are key to our understanding of star formation and evolution in the Galactic center. Previous work on this topic has been based on infrared (IR) observations, but X-ray observations have the potential of constraining…

星系天体物理 · 物理学 2023-04-12 Ziqian Hua , Zhiyuan Li , Mengfei Zhang , Zhuo Chen , Mark R. Morris

The Visible-Infrared Mapping Spectrometer (VIR) on board the Dawn spacecraft revealed that aqueous secondary minerals -- Mg-phyllosilicates, NH4-bearing phases, and Mg/Ca carbonates -- are ubiquitous on Ceres. Ceres' low reflectance…

地球与行星天体物理 · 物理学 2020-11-03 H. Kurokawa , B. L. Ehlmann , M. C. De Sanctis , M. G. A. Lapôtre , T. Usui , N. T. Stein , T. H. Prettyman , A. Raponi , M. Ciarniello

Soon after launch, the Advanced CCD Imaging Spectrometer (ACIS), one of the focal plane instruments on the Chandra X-ray Observatory, suffered radiation damage from exposure to soft protons during passages through the Earth's radiation…

天体物理学 · 物理学 2009-11-11 C. E. Grant , M. W. Bautz , S. E. Kissel , B. LaMarr , G. Y. Prigozhin

A Chandra AO1 30ks HETGS observation of the X-ray transient micro-quasar GRS 1915+105 reveals absorption edges and faint line emission over the HETG energy range. We find from a preliminary analysis evidence for prominent neutral K edges…

天体物理学 · 物理学 2007-05-23 J. C. Lee , N. S. Schulz , C. S. Reynolds , A. C. Fabian , E. G. Blackman

An observation of the gravitationally lensed system 2016+112 with the Chandra X-ray Observatory has resolved a mystery regarding the proposed presence of a dark matter object in the lens plane of this system. The Chandra ACIS observation…

天体物理学 · 物理学 2009-11-06 G. Chartas , M. Bautz , G. Garmire , C. Jones , D. P. Schneider

It was observed early on in the Chandra X-ray Observatory mission that the background rates of the Advanced CCD Imaging Spectrometer (ACIS) were highly variable on both short and long timescales. We present analysis of lightcurves of the…

天体物理学 · 物理学 2007-05-23 Catherine E. Grant , Mark W. Bautz , Shanil N. Virani

We present an exploratory Chandra ACIS-S3 study of the diffuse component of the Cosmic X-ray Background in the 0.3-7 keV band for four directions at high Galactic latitudes, with emphasis on details of the ACIS instrumental background…

We present the first results of the Chandra and optical follow-up observations of hard X-ray sources detected in the ASCA Medium Sensitivity Survey (AMSS). Optical identifications are made for five objects. Three of them show either weak or…

Soon after launch, the Advanced CCD Imaging Spectrometer (ACIS), one of the focal plane instruments on the Chandra X-ray Observatory, suffered radiation damage from exposure to soft protons during passages through the Earth's radiation…

天体物理学 · 物理学 2009-11-07 Catherine E. Grant , Gregory Y. Prigozhin , Beverly LaMarr , Mark W. Bautz

We have studied the O and Ne absorption features in the X-ray spectrum of Cyg X-2 observed with the Chandra LETG. The O absorption edge is represented by the sum of three absorption-edge components within the limit of the energy resolution…

天体物理学 · 物理学 2009-11-07 Yoh Takei , Ryuichi Fujimoto , Kazuhisa Mitsuda , Takashi Onaka
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