Diffuse Galactic emission spectrum between 0.5 and 8.0 MeV

Open Access

Table B.1

Consecutive observation periods selected from the considerations in Sect. 2.1 and Fig. 1. From left to right the columns are the INTEGRAL revolution number, the number of targeted observations (pointings) that are selected in this interval, and the corresponding dead-time-corrected lifetime of a working detector in units of ks. Intervals with zero observations had no exposures within our selected region.

Rev.	n_obs	T_obs	Rev.	n_obs	T_obs
43–75	1351	1754	1057–1074	62	108
77–82	0	0	1076–1076	0	0
84–91	0	0	1078–1091	440	894
97–124	1502	3317	1094–1101	91	132
127–127	0	0	1103–1110	0	0
141–181	1115	2128	1120–1132	0	0
183–204	312	613	1136–1146	464	831
216–-216	0	0	1151–1170	424	657
219–219	0	0	1172–1176	0	0
221–233	580	1354	1185–1187	0	0
237–249	669	1035	1191–1191	0	0
251–252	0	0	1195–1206	142	243
256–275	3	4	1209–1247	1088	2036
283–297	683	1611	1255–1271	506	870
299–314	835	1372	1273–1280	296	569
317–325	0	0	1282–1292	71	119
331–335	0	0	1297–1304	0	0
338–339	0	0	1307–1317	13	22
343–348	107	288	1326–1338	533	872
350–353	90	184	1340–1367	552	907
358–372	650	1412	1369–1370	0	0
374–394	0	0	1378–1387	28	43
401–419	796	1908	1391–1405	96	143
421–445	570	1270	1407–1449	144	237
453–472	405	1109	1456–1506	799	1562
474-505	985	2412	1513–1516	122	193
512–533	219	562	1518–1553	846	1420
535–564	583	1322	1558–1584	506	812
572–640	1243	3066	1591–1603	313	505
648–672	684	1643	1605–1651	1142	1794
674–713	170	387	1657–1671	565	864
721–774	929	1953	1673–1704	163	232
777–795	764	1424	1711–1723	587	886
803–833	0	0	1725–1770	1059	1550
835–856	1135	1820	1777–1838	1241	2010
864–910	1407	2687	1840–1842	55	79
917-928	145	314	1849–1857	168	295
931-973	425	1082	1863–1912	565	931
983–1024	364	773	1919–1973	1005	2135
1027–1029	95	138	1975–1978	0	0
1031–1040	262	387	1985–1986	3	5
1049–1055	4	5	1988–2047	1308	2346

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