5XMM J113142.8-195355

5XMM-DR15 stacked source · SRCID 3004234100100007
Position: 11h31m42.87s -19d53m55.1s (172.92863°, -19.89864°)
EP flux
4.31e-14 ± 4.6e-15 erg cm-2 s-1
CLASSX
AGN (0.92)
Detections
2

SRCID 3004234100100007
IAUNAME 5XMM J113142.8-195355
SC_RA 11h31m42.87s (172.92863°)
SC_DEC -19d53m55.1s (-19.89864°)
RADEC_ERR 0.40 arcsec
LII / BII 278.5130° / 39.1632°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52091.266 (2001-07-01 06:23:10.000 UTC)
MJD_LAST 59032.577 (2020-07-02 13:50:48.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.31e-14 ± 4.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.28 ± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
0.20 ± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38 ± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.44 ± 0.11
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.7) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.105

Class probabilities
Class taxonomy
  • AGN — active galactic nucleus.
  • Bkg_AGN — background AGN.
  • Star — Galactic star.
  • Gal_XRB — Galactic X-ray binary.
  • Extragal_XRB — extragalactic X-ray binary.
  • CV — cataclysmic variable.
  • Extended — cluster or galaxy.

Optical Monitor (OM)
OM Source ID
3063874
Match probability
0.998
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 20.739 0.138
U — —
B — —
V — —
Gaia DR3
Source ID
3545009110687273856
Match probability
0.993
Parallax
-0.462 ± 0.654 mas
Proper motion
(0.77, -0.86) mas/yr
Magnitudes
G=20.23, BP=20.56, RP=19.74
CLASSOPT
Class
QSO
Star
0.00
AGN
1.00
Galaxy
0.00

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 4.48e-14 (+5.1e-14 / −3.9e-14) erg cm−2 s−1
NH 1.32e+20 (+4.7e+20 / −2.2e+19) cm−2
Photon index (Γ) 1.65 (+1.82 / −1.52)
DoF 263
p-value 0.854
Inter-instrument norm. 1.27 (1.06–1.49)
Quality flag 0

APPROX_SOURCE_VAR 6.200 (approximate flux variability amplitude)

No contributing observations found.

Sky view (optical)

DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.

Hardness-ratio diagram

The per-observation light curve is shown in the X-ray properties section above.