Data description¶
See also
This chapter provides the detailed description of the CGBM data stored in the CGBM data archive.
The CGBM data archive comprises Scientific data and Auxiliary data.
Scientific data¶
There are two general types of scientific data: Monitor data and Trigger data.
Monitor data¶
Monitor data consist of Time History (TH) data and Pulse Height (PH) data.
Time History (TH) data¶
See also
Each CGBM gamma-ray detector collects TH data data with a 1/8(=0.125) sec time resolution in two overlapping energy ranges which correspond to two different gains: high gain (HG) and low gain (LG). Each range has 4 channels.
The nominal TH energy ranges of the three CGBM gamma-ray detectors are (approximate):
| Detector | Gain | Energy range (keV) |
|---|---|---|
| HXM1, HXM2 | HG | 4 ─ 100 |
| LG | 60 ─ 3000 | |
| SGM | HG | 40 ─ 1000 |
| LG | 550 ─ 28000 |
The nominal TH channel boundaries of the three CGBM gamma-ray detectors are (approximate):
| Detector | Gain | Channel boundaries (keV) | |||
|---|---|---|---|---|---|
| Ch0 | Ch1 | Ch2 | Ch3 | ||
| HXM1, HXM2 | HG | 4 ─ 10 | 10 ─ 25 | 25 ─ 50 | 50 ─ 100 |
| LG | 60 ─ 100 | 100 ─ 170 | 170 ─ 300 | 300 ─ 3000 | |
| SGM | HG | 40 ─ 100 | 100 ─ 230 | 230 ─ 450 | 450 ─ 1000 |
| LG | 55 ─ 830 | 830 ─ 1500 | 1500 ─ 2600 | 2600 ─ 28000 | |
Note
- Since the last channel of the HG range and the first channel of the LG range are partially overlapped, the counts accumulated in these channels are not independent.
EBOUNDSextensions of The TH FITS file contain the same energy boundaries for the entire mission lifetime, i.e. they are not corrected for the gain drift.- TH data are recorded even when HV is off, in which case 0 values are put in the record. There are Good Time Intervals (GTI) fits files which specify the time intervals when HV was above 90% of its nominal value. The TH data near the times where HV was turned on/off are affected by lower HV (HV is increased/decreased gradually near these times).
- There might be gaps in TH data.
Warning
- The
EXPOSUREcolumn of the TH data is not corrected for the deadtime. In a future release, we will provide the deadtime corrected exposure time in theEXPOSUREcolumn. - The TH data (monitor data) have a known issue regarding a jitter in timing.
TIMEcolumn of the data could introduce the systematic jitter of several tens of milliseconds (i.e. the difference between the times of successive bins can differ from the nominal 0.125 s by several tens of milliseconds). Although we understand the cause of this timing issue and the way to correct this, the correction has not been applied to the current version. Please be cautious that the TIME column of the data could introduce the systematic jitter of several tens of milliseconds. - See all important Caveats for the current release.
Pulse Height (PH) data¶
See also
Each CGBM gamma-ray detector collects PH data with a 4 sec time resolution in two overlapping energy ranges which correspond to two different gains: high gain (HG) and low gain (LG). The HG range has 102 channels and the LG range has 410 channels. The LG range includes the entire HG range, but provides coarser energy binning.
The nominal PH energy ranges of the three CGBM gamma-ray detectors are:
| Detector | Gain | Energy range (keV) |
|---|---|---|
| HXM1, HXM2 | HG | 0.0 ─ 98.304 |
| LG | 0.0 ─ 3072.0 | |
| SGM | HG | 0.0 ─ 942.080 |
| LG | 0.0 ─ 28672.0 |
The nominal PH channel boundaries of the three CGBM gamma-ray detectors can be found in the corresponding ascii files:
Note
- Since the LG range includes the entire HG range, the counts accumulated in the overlapped channels are not independent, they correspond to the same events but digitized differently.
- PH data are recorded even when HV is off, in which case 0 values are put in the record. There are Good Time Intervals (GTI) fits files which specify the time intervals when HV was above 90% of its nominal value. The PH data near the times where HV was turned on/off are affected by lower HV (HV is increased/decreased gradually near these times).
- There might be gaps in PH data.
Auxiliary data¶
The detailed description of the auxiliary data will be provided later.
The following table briefly summarizes each file type:
| Type | Name | Description |
| att, iat | cgbm_YYYYMMDD.att, cgbm_YYYYMMDD.iat | contains the attitude information |
| hk | cgbm_YYYYMMDD.hk | contains the housekeeping data related to CGBM detectors |
| orb | cgbm_YYYYMMDD.orb | contains the orbit information |
| tim | cgbm_YYYYMMDD.tim | contains the time correction data |
| gti | cgbm_YYYYMMDD_[det].gti | contains good time intervals for each detector |