5XMM J011133.3-375427

5XMM-DR15 stacked source · SRCID 3000294230100156
Position: 01h11m33.36s -37d54m27.7s (17.88902°, -37.90769°)
EP flux
6.81e-15 ± 5.2e-15 erg cm-2 s-1
CLASSX
AGN (0.686)
Detections
2

SRCID 3000294230100156
IAUNAME 5XMM J011133.3-375427
SC_RA 01h11m33.36s (17.88902°)
SC_DEC -37d54m27.7s (-37.90769°)
RADEC_ERR 2.46 arcsec
LII / BII 282.7726° / -78.4215°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52253.198 (2001-12-10 04:44:57.000 UTC)
MJD_LAST 54809.311 (2008-12-09 07:28:24.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 6.81e-15 ± 5.2e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.03 ± 0.23
0.2-0.5 / 0.5-1.0 keV
HR2
-0.87 ± 0.36
0.5-1.0 / 1.0-2.0 keV
HR3
0.06 ± 0.61
1.0-2.0 / 2.0-4.5 keV
HR4
0.87 ± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.9) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 1.36

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
541342
Match probability
0.727
FilterMag (AB)Err
UVW2
UVM2
UVW1 20.936 0.152
U
B
V
Gaia DR3
Source ID
4988812871757492608
Match probability
0.991
Parallax
-0.179 ± 0.261 mas
Proper motion
(1.49, -0.42) mas/yr
Magnitudes
G=19.31, BP=19.48, RP=18.88
CLASSOPT
Class
QSO
Star
0.04
AGN
0.92
Galaxy
0.04

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 5.24e-15 (+7.7e-15 / −3.4e-15) erg cm−2 s−1
NH 1.16e+20 (+6.3e+20 / −2.0e+19) cm−2
Photon index (Γ) 2.45 (+2.82 / −1.93)
DoF 89
p-value 0.223
Quality flag 0

No variability data available for this source.

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.