5XMM J021247.3-740337

5XMM-DR15 stacked source · SRCID 3004915010100091
Position: 02h12m47.35s -74d03m37.0s (33.19727°, -74.06028°)
EP flux
1.27e-14 ± 4.8e-15 erg cm-2 s-1
CLASSX
AGN (0.95)
Detections
6

SRCID 3004915010100091
IAUNAME 5XMM J021247.3-740337
SC_RA 02h12m47.35s (33.19727°)
SC_DEC -74d03m37.0s (-74.06028°)
RADEC_ERR 0.68 arcsec
LII / BII 295.5661° / -41.8843°
N_CONTRIB 6 (detections)
N_OBS 9 (observations covering the position)
MJD_FIRST 51730.634 (2000-07-05 15:13:30.000 UTC)
MJD_LAST 53386.433 (2005-01-16 10:23:46.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.27e-14 ± 4.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.37 ± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
0.21 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.58 ± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.22 ± 0.44
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.1) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.601

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
747529
Match probability
0.983
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 22.058 0.133
U 21.959 0.186
B — —
V — —
Gaia DR3
Source ID
4643568664472975360
Match probability
0.994
Magnitudes
G=20.89, BP=21.21, RP=21.03
CLASSOPT
Class
QSO
Star
0.00
AGN
0.99
Galaxy
0.01

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 9.68e-15 (+1.3e-14 / −6.9e-15) erg cm−2 s−1
NH 1.11e+20 (+6.7e+20 / −2.1e+19) cm−2
Photon index (Γ) 1.99 (+2.34 / −1.67)
DoF 82
p-value 0.251
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.