5XMM J132457.6+300912

5XMM-DR15 stacked source · SRCID 3002574020100038
Position: 13h24m57.68s +30d09m12.9s (201.24035°, 30.15360°)
EP flux
2.14e-14 ± 4.5e-15 erg cm-2 s-1
CLASSX
AGN (0.925)
Detections
1

SRCID 3002574020100038
IAUNAME 5XMM J132457.6+300912
SC_RA 13h24m57.68s (201.24035°)
SC_DEC +30d09m12.9s (30.15360°)
RADEC_ERR 0.70 arcsec
LII / BII 57.2635° / 82.0496°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52255.718 (2001-12-12 17:14:17.000 UTC)
MJD_LAST 52256.169 (2001-12-13 04:02:51.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.14e-14 ± 4.5e-15 erg cm-2 s-1

Hardness ratios
HR1
0.15 ± 0.15
0.2-0.5 / 0.5-1.0 keV
HR2
0.03 ± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.18 ± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
-0.56 ± 0.20
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.1) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.551

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
3472619
Match probability
0.992
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.129 0.182
U 21.752 0.161
B
V

Spectroscopic (zsp) 1.24000
Photometric (TPZ) 1.0757 (conf 0.61)
Photometric (Le Phare) 1.0500 (conf 0.62)

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

Stacked power-law fit
Unabsorbed flux 1.41e-14 (+1.8e-14 / −1.1e-14) erg cm−2 s−1
NH 8.16e+19 (+4.6e+20 / −1.9e+19) cm−2
Photon index (Γ) 1.97 (+2.32 / −1.74)
DoF 118
p-value 0.719
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.