A minor problem is found in the header keyword (MJDREF) of PIN background. The HXD team has corrected it to the appropriate keywords (MJDREFI and MJDREFF), and also updated the METHODV keyword to "2.0pre20080404" for all NXB data before 2008-03-15 20:45 (ZETA_OPH). Old files are moved into the "old20080527" directory.
The reproducibility of the HXD-PIN background model for v2 products is described as a suzakumemo (2007-09).
Observation date | Directory | METHOD * | METHODV ** |
---|---|---|---|
After 2005-09-02 | pinnxb_ver2.0 | PINUDLCUNIT | 2.0preYYYYMMDD |
The directory is divided into subdirectories by month. For example, background files for observations carried out in 2006 August can be found in the subdirectory 2006_08. Within these monthly directories, individual background files are listed alphabetically. Note these files are named using the sequence number, e.g., ae100005010hxd_pinnxb_cl.evt.gz.
These files should only be used with version 2.x processed data, and vice versa.
One important change from version 1.x background files is that the
new background files contain events from all units of PIN, regardless
of whether the bias voltage is 500V or 400V. The HXD team defines
4 different epochs (Epoch-1 to 5) referring to the major change
of operation modes (i.e. the PIN bias voltage). Current NXB release
automatically supports these change. However, there are two time
regions (in epoch-1) in which they are known to show some (~10%)
systematic offset caused by minor operation parameter changes. They are
- 2005-07-20 to 2005-09-01 :
"The initial operation period", in which the HXD was in the initial operation phase.
- 2006-03-23 to 2006-05-13 :
"The GSO threshold change period", in which some GSO parameters were changed.
In these two periods, users are suggested to use the "tuned" (METHD=LCFITDT) NXB files, which can be found in the tuned PIN-NXB directory.
A pseudo event file filtered with the same GTI as the cleaned event file can be found in the cleaned event file directory in data processed with version 2.x (event_cl/aeNNNNNNNNNhxd_0_pse_cl.evt.gz). This is the most convenient input to hxddtcor, if you are analyzing the cleaned event files. Otherwise, supply the unscreened event file(s) to hxddtcor. The syntax is:
hxddtcor ae123456789hxd_0_pse_cl.evt ae123456789pin.phaif the spectral file is called ae123456789pin.pha. Note that the EXPOSURE keyword value will be rewritten.
On the other hand, dead time correction is not necessary for the PIN background files.
Guest observers are strongly recommended to verify the reliability of the background model
Epoch | File(s) |
---|---|
2005.8.17 -- 2006.5.13 | ae_hxd_pinXXXXXe1_20080129.rsp (XXXXX=xinom,hxnom,flat) |
2006.5.13 -- 2006.10.2 | ae_hxd_pinXXXXXe2_20080129.rsp (XXXXX=xinom,hxnom,flat) |
2006.10.2 -- 2007.7.28 | ae_hxd_pinXXXXXe3_20080129.rsp (XXXXX=xinom,hxnom,flat) |
2007.7.28 -- 2008.8.31 | ae_hxd_pinXXXXXe4_20080129.rsp (XXXXX=xinom,hxnom,flat) |
2008.9.1 -- 2009.9.30 | ae_hxd_pinXXXXXe5_20080716.rsp (XXXXX=xinom,hxnom,flat) |
2009.10.1 -- 2010.1.16 | ae_hxd_pinXXXXXe6_20090826.rsp (XXXXX=xinom,hxnom,flat) |
2010.1.16 -- 2010.2.1 | ae_hxd_pinXXXXXe7_20100731.rsp (XXXXX=xinom,hxnom,flat) |
2010.2.2 -- 2010.4.3 | ae_hxd_pinXXXXXe8_20100731.rsp (XXXXX=xinom,hxnom,flat) |
2010.4.3 -- 2010.11.30 | ae_hxd_pinXXXXXe9_20100731.rsp (XXXXX=xinom,hxnom,flat) |
2010.12.1 -- 2011.5.24 | ae_hxd_pinXXXXXe10_20101013.rsp (XXXXX=xinom,hxnom,flat) |
2011.5.25 -- | ae_hxd_pinXXXXXe11_20110601.rsp (XXXXX=xinom,hxnom,flat) |
These files are available from the Suzaku CALDB (2009-12-07 version or later).
If you have any questions, please contact Suzaku Help Desk.