17 New Identified INTEGRAL Sources
ATel #232; L. Bassani, A. Malizia, J. B. Stephen (IASF Bologna Italy); A. Bazzano, P. Ubertini (IASF Roma Italy); E. J. Barlow, A. J. Bird, A. J. Dean, A. B. Hill, S. E. Shaw (Southampton University Southampton UK); R. Walter, A. Bodaghee (ISDC Geneva Switzerland); G. Belanger, F. Lebrun, R. Terrier (CEA Saclay France); R. Much (RSSD ESTEC/ESA Nordwijk The Netherlands)
on 13 Feb 2004; 14:01 UT
Credential Certification: Malizia Angela (malizia@bo.iasf.cnr.it)
Subjects: X-ray, Gamma Ray, AGN, Binary, Black Hole, Cataclysmic Variable, Nova, Supernova Remnant, Pulsar
We report the first detection in the hard X-ray band (>20 keV) of 17 known sources.
The sources have been detected by the IBIS/ISGRI instrument on board
INTEGRAL and found in all-sky mosaics built from data of the INTEGRAL
core program accumulated between February 27 and October 19, 2003.
Number
|
ISGRI Ra&Dec(2000)
|
Probable Identification
|
Type
|
Sigma
|
|
|
|
|
|
|
N.1
|
18 55.0
|
-31 09.8
|
4U1849-31
|
Cat Var
|
22
|
N.2
|
18 38.1
|
-06 55.4
|
AXJ1838.0-0655
|
X-ray source
|
7
|
N.3
|
16 49.6
|
-43 49.9
|
PSRJ1649-4349/PMN1649-4352
|
Pulsar/Radio
|
8
|
N.4
|
21 42.8
|
+43 34.2
|
SSCygni
|
Dwarf Nova
|
7
|
N.5
|
17 41.8
|
-12 12.3
|
2E1739.1-1210
|
X-ray source
|
6
|
N.6
|
18 20.5
|
-14 32.9
|
AXJ1820.5-1434
|
HMXRB
|
21
|
N.7
|
17 00.4
|
-42 20.2
|
AXJ1700.2-4220
|
X-ray source
|
7
|
N.8
|
17 45.7
|
-28 59.5
|
2E1742.5-2858
|
LMXRB
|
21
|
N.9
|
01 18.0
|
+65 15.3
|
4U0114+65
|
HMXRB
|
9
|
N.10
|
18 41.3
|
+04 56.1
|
1E1841-045/Kes73
|
SNR/Pulsar
|
10
|
N.11
|
18 46.4
|
-02 57.8
|
AXJ1846.4-0258/Kes75
|
SNR/pulsar
|
9
|
N.12
|
18 33.6
|
-10 33.2
|
SNR021.5-00.9
|
SNR
|
12
|
N.13
|
18 45.7
|
00 51.5
|
Ginga1843+00
|
HMXRB
|
8
|
N.14
|
19 40.1
|
-10 24.4
|
RXJ1940.1-1025
|
Cat Var
|
7
|
N.15
|
19 42.6
|
-10 19.6
|
NGC6814
|
Seyfert1
|
7
|
N.16
|
22 07.9
|
+54 32.5
|
4U2206+54
|
HMXRB
|
22
|
N.17
|
18 07.0
|
-29 25.3
|
XTEJ1807-294
|
Msec
pulsar
|
17
|
The error radius of each position is smaller than 3 arcmin (90% confidence level).
Statistical significances are measured between 20 and 40 keV. Properties of these
sources will be presented in Bird et al. (2004).