EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 507 / No 1 (November III 2009) A&A, 507 1 (2009) 549-571 Full HTML
Free Access

   

Table 1:

The 20 objects investigated in this study and the properties of the corresponding datasets.
Object namea Object typeb RA, Dec (FK5) galactic l, b elapsed effective var.d Data
        time SPI exposurec   Set
    $[^\circ]$ $[^\circ]$ [Ms] [106 cm2 s] [ks]  
Crab PWN 083.6332, +22.0145 184.5575, -05.7843 1.33 22.7 - 1
Vela Pulsar PWN 128.8361, -45.1764 263.5520, -02.7873 3.48 68.9 - 2
NGC 4151 Seyfert 1.5 182.6364, +39.4054 155.0765, +75.0637 0.085 5.2 - 3
NGC 4945 Seyfert 2 196.3587, -49.4708 305.2681, +13.3374 0.53 9.1 - 4
Cen A Radio Gal., Seyf.2 201.3651, -43.01911 309.5159, +19.4173 0.56 11.5 - 5
XTE J1550-564 LMXB, BHC, $\mu$Q 237.7446, -56.4767 325.8822, -01.8271 2.56 42.4 - 6
4U 1630-47 LMXB, BHC 248.5017, -47.3942 336.9081, +00.2519 3.97 154 - 7
Swift J1656.3-3302 Blazar 254.0690, -33.0359 350.5993 +06.3581 10.1 151 - 10
OAO 1657-415 HMXB, Pulsar 255.1996, -41.6731 344.3538, +00.3111 3.97 110 - 7
GX 339-4 LMXB, BHC, $\mu$Q 255.7062, -48.7897 338.9394, -04.3267 3.36 123 - 8
4U 1700-377 HMXB, NS 255.9866, -37.8441 347.7544, +02.1735 3.97 73.5 90, - 7
IGR J17091-3624 LMXB?, BHC 257.275, -36.410 349.519, +02.215 7.08 214 - 9
GX 354-0 LMXB, NS 262.9892, -33.8347 354.3022, -00.1501 7.08 130 - 9
1E 1740.7-2942 LMXB?, BHC, $\mu$Q 265.9785, -29.7452 359.1160, -00.1057 7.08 134 - 9
IGR J17464-3213 LMXB?, BHC, $\mu$Q 266.5650, -32.2335 357.2552, -01.8330 7.08 114 90, - 9
GRS 1758-258 LMXB, BHC, $\mu$Q 270.3012, -25.7433 004.5076, -01.3607 10.1 403 - 10
Ginga 1826-24 LMXB, NS 277.3675, -23.7969 009.2724, -06.0878 10.1 239 - 10
GRS 1915+105 LMXB, BHC, $\mu$Q 288.7983, +10.9456 045.3656, -00.2194 2.83 53.1 90, - 11
Cyg X-1 HMXB, BHC, $\mu$Q 299.5903, +35.2016 071.3350, +03.0668 1.94 32.9 90, 180 12
Cyg X-3 HMXB, BHC, $\mu$Q 308.1074, +40.9578 079.8455, +00.7001 2.79 50.2 90, - 13
Control1e - 259.5000, -40.3500 347.7000, -02.1000 7.08 181 - 9

a See Sect. 2.1 for the selection criteria and Sect. 4 for references concerning the source properties.
b PWN = pulsar wind nebula, $\mu$Q = microquasar, NS = binary containing a neutron star, BHC = containing a black hole candidate, ? = classification uncertain.
c Calculated at 30 keV and taking into account the SPI response.
d Assumed variability timescale in the analysis at E < 144 keV (first number) and at E > 144 keV (second number); ``-'' = the source was assumed constant either because it is known to be steady or because the variability timescale and/or amplitude is too small for SPI to detect significant variability.
e Control position for the assessment of systematic errors in the analysis of crowded fields (see Sects. 3.3 and 4.21).


Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.