5XMM J224251.0+293647

5XMM-DR15 stacked source · SRCID 3000681010100033
Position: 22h42m51.02s +29d36m47.2s (340.71257°, 29.61312°)
EP flux
8.25e-15 ± 1.8e-15 erg cm-2 s-1
CLASSX
AGN (0.886)
Detections
13

SRCID 3000681010100033
IAUNAME 5XMM J224251.0+293647
SC_RA 22h42m51.02s (340.71257°)
SC_DEC +29d36m47.2s (29.61312°)
RADEC_ERR 0.48 arcsec
LII / BII 92.1132° / -25.4545°
N_CONTRIB 13 (detections)
N_OBS 13 (observations covering the position)
MJD_FIRST 51712.539 (2000-06-17 12:56:51.000 UTC)
MJD_LAST 58456.963 (2018-12-04 23:06:59.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 8.25e-15 ± 1.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.79 ± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
0.38 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.29 ± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.51 ± 0.19
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.5) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.966

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
6484267
Match probability
0.998
FilterMag (AB)Err
UVW2
UVM2
UVW1 20.419 0.120
U
B
V

Spectroscopic (zsp) 2.37300
Photometric (TPZ) 2.4253 (conf 0.81)
Photometric (Le Phare) 2.1790 (conf 0.92)

Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.

Stacked power-law fit
Unabsorbed flux 1.97e-14 (+2.4e-14 / −1.6e-14) erg cm−2 s−1
NH 4.55e+19 (+1.7e+20 / −1.6e+19) cm−2
Photon index (Γ) 1.35 (+1.57 / −1.17)
DoF 142
p-value 0.224
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.