SPI processing of SVT-E data

SPI SVT-E data for scientific analysis

Not all science windows from SVT-E contain SPI data which can be analysed using the scientific offline analysis. Only data which where taken in OPERATIONAL mode can be used. The modes of the different science windows can be seen by using IOSM (click on "new Modes, Times" and select SPI). Or you just use the sicence windows listed below.

List of SCWs for scientific analysis
SCW ID Date Source Remarks

000200000082.000 15.1. ¹³⁷Cs To produce a SPISKYMAX "background" image use one energy bin from 650-670 keV. Use this parameter file (copy it to $PFILES/blc_sa.par)

000200000092.000 15.1. ¹³⁷Cs

000200000102.000 15.1. ¹³⁷Cs

000200000112.000 15.1. ¹³⁷Cs

000300000142.000 16.1. no source strong background lines around 1460 keV and 2870 keV

000400000072.000 17.1. no source Use this parameter file (copy it to $PFILES/blc_sa.par) to make an analysis of the background ⁴⁰K line at 1460 keV (SPIROS and SPISKYMAX images).

000400000082.000 17.1. no source

000400000102.000 17.1. no source

List of SCWs for scientific analysis
SCW ID	Date	Source	Remarks
000200000082.000	15.1.	¹³⁷Cs	To produce a SPISKYMAX "background" image use one energy bin from 650-670 keV. Use this parameter file (copy it to $PFILES/blc_sa.par)
000200000092.000	15.1.	¹³⁷Cs
000200000102.000	15.1.	¹³⁷Cs
000200000112.000	15.1.	¹³⁷Cs
000300000142.000	16.1.	no source	strong background lines around 1460 keV and 2870 keV
000400000072.000	17.1.	no source	Use this parameter file (copy it to $PFILES/blc_sa.par) to make an analysis of the background ⁴⁰K line at 1460 keV (SPIROS and SPISKYMAX images).
000400000082.000	17.1.	no source
000400000102.000	17.1.	no source

In case of questions and comments: contact me at GSFC.