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HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details.

Suzaku Guest Observer Facility

HXD/PIN Epochs

Updated 2014 April 15


Epoch No.Date of ObservationResponse Files
12005.8.17 -- 2006.5.25ae_hxd_pinXXXXXe1_20080129.rsp
22006.5.25 -- 2006.10.3ae_hxd_pinXXXXXe2_20080129.rsp
32006.10.3 -- 2007.7.28ae_hxd_pinXXXXXe3_20080129.rsp
42007.7.28 -- 2008.8.31ae_hxd_pinXXXXXe4_20080129.rsp
52008.9.1 -- 2009.9.30ae_hxd_pinXXXXXe5_20080716.rsp
62009.10.1 -- 2010.1.16ae_hxd_pinXXXXXe6_20090826.rsp
72010.1.16 -- 2010.2.2 ae_hxd_pinXXXXXe7_20100731.rsp
82010.2.2 -- 2010.4.3 ae_hxd_pinXXXXXe8_20100731.rsp
92010.4.3 -- 2010.11.30ae_hxd_pinXXXXXe9_20100731.rsp
102010.12.1 -- 2011.05.25ae_hxd_pinXXXXXe10_20101013.rsp
112011.05.25 -- **ae_hxd_pinXXXXXe11_20110601.rsp

(XXXXX=xinom,hxnom,flat)

The HXD team has adjusted the high voltage setting of the PIN diodes and/or the low energy threshold 9 times so far during the mission lifetime. For each epoch, it is necessary to use:

  • the appropriate PIN threshold calibration file with hxdgrade during processing (true for all sequences currently available at HEASARC, proprietary or public)
  • the appropriately created PIN background model files (true for all NXB files currently available); and
  • the appropriate response files in data analysis (user responsibility)

The response files for Epochs 1-11 can be obtained through Suzaku CALDB. Further details regarding epochs can be found in this HXD CALDB Memo. Note, however, that the boundary between Epochs 1 & 2 listed in this memo (2006.05.13) is incorrect, and the value in the table above (2006.06.25) is correct.


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This file was last modified on Tuesday, 15-Apr-2014 15:39:20 EDT

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