2012A&A...548A..32M


Query : 2012A&A...548A..32M

2012A&A...548A..32M - Astronomy and Astrophysics, volume 548A, 32-32 (2012/12-1)

Flat-spectrum radio sources as likely counterparts of unidentified INTEGRAL sources.

MOLINA M., LANDI R., BASSANI L., MALIZIA A., STEPHEN J.B., BAZZANO A., BIRD A.J. and GEHRELS N.

Abstract (from CDS):

Many sources in the fourth INTEGRAL/IBIS catalogue are still unidentified since they lack an optical counterpart. An important tool that can help in identifying and classifying these sources is the cross-correlation with radio catalogues, which are very sensitive and positionally accurate. Moreover, the radio properties of a source, such as the spectrum or morphology, could provide further insight into its nature. In particular, flat-spectrum radio sources at high Galactic latitudes are likely to be AGN, possibly associated to a blazar or to the compact core of a radio galaxy. Here we present a small sample of 6 sources extracted from the fourth INTEGRAL/IBIS catalogue that are still unidentified or unclassified, but which are very likely associated with a bright, flat-spectrum radio object. To confirm the association and to study the source X-ray spectral parameters, we performed X-ray follow-up observations with Swift/XRT of all objects. We report in this note the overall results obtained from this search and discuss the nature of each individual INTEGRAL source. We find that 5 of the 6 radio associations are also detected in X-rays; furthermore, in 3 cases they are the only counterpart found. More specifically, IGR J06073-0024 is a flat-spectrum radio quasar at z=1.08, IGR J14488-4008 is a newly discovered radio galaxy, while IGR J18129-0649 is an AGN of a still unknown type. The nature of two sources (IGR J07225-3810 and IGR J19386-4653) is less well defined, since in both cases we find another X-ray source in the INTEGRAL error circle; nevertheless, the flat-spectrum radio source, likely to be a radio loud AGN, remains a viable and, in fact, a more convincing association in both cases. Only for the last object (IGR J11544-7618) could we not find any convincing counterpart since the radio association is not an X-ray emitter, while the only X-ray source seen in the field is a G star and therefore unlikely to produce the persistent emission seen by INTEGRAL.

Abstract Copyright:

Journal keyword(s): gamma rays: galaxies - X-rays: galaxies - galaxies: active - quasars: general

Simbad objects: 18

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Number of rows : 18
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 ICRF J060657.4-002457 QSO 06 06 57.44358215 -00 24 57.4638852           ~ 20 1
2 IGR J06073-0024 gam 06 07 19 -00 24.9           ~ 3 0
3 NVSS J072215-381459 Rad 07 22 15.19 -38 14 59.1           ~ 1 0
4 PMNM B0720-3809 Rad 07 22 22.4 -38 14 55           ~ 2 1
5 NVSS J072227-381457 Rad 07 22 27.9 -38 14 58           ~ 2 0
6 IGR J07225-3810 gam 07 22 29 -38 10.1           ~ 6 0
7 1RXS J115313.6-761935 X 11 53 13.6 -76 19 35           ~ 1 0
8 HD 103307 PM* 11 53 16.5854801472 -76 18 56.155144824   10.60 9.99     G0/3IV/V 4 0
9 IGR J11544-7618 gam 11 54 22 -76 18.5           ~ 2 0
10 SUMSS J115505-761955 Rad 11 55 05.960 -76 19 55.00           ~ 1 0
11 SUMSS J115509-761736 Rad 11 55 09.340 -76 17 36.40           ~ 1 0
12 SUMSS J115514-761512 Rad 11 55 14.080 -76 15 12.90           ~ 1 0
13 PKS 1153-760 Rad 11 55 46.94 -76 19 08.2           ~ 3 0
14 2MASX J14485095-4008542 G 14 48 50.9 -40 08 52           ~ 3 0
15 2MASS J14485097-4008456 Sy1 14 48 50.9757473760 -40 08 45.711613968   14.7   14.0   ~ 39 0
16 4C -06.53 Bla 18 12 50.94679400 -06 48 25.2867999           ~ 21 2
17 PKS 1934-470 Rad 19 38 24.2 -46 57 39           ~ 1 1
18 IGR J19386-4653 gam 19 38 37 -46 53.2           ~ 3 0

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