C H A N D R A
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C E N T E R O B S E R V A T I O N C A T A L O G |
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Abstract: XRISM is currently scheduled to observe NGC 4151 on Dec 27, 2023, for 45 ks. This is the first of four planned XRISM exposures; the rest will likely be taken in late April 2024. Below 4 keV, the HETGS offers superior resolution to the Resolve calorimeter. Simultaneous - or at least contemporaneous observations - will provide the best opportunity to study the variable absorption and winds in NGC 4151, the nature and origin of the narrow Fe K line, and to search for relativistic disk reflection. NuSTAR will also observe NGC 4151 providing coverage of the ionizing continuum out to 79 keV, but no coverage below 3 keV. Chandra spectroscopy is essential for characterizing the lines and absorption edges at low energy that ultimately shape the continuum through the Fe K band, where the strongest outflows and relativistic disk reflection are evident. [Submitted on behalf of the XRISM team; additional communication with the Director includes some privileged information.] |
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