5XMM J152517.0+513440

5XMM-DR15 stacked source · SRCID 3001183020100016
Position: 15h25m17.01s +51d34m40.6s (231.32087°, 51.57793°)
EP flux
2.48e-14 ± 5.8e-15 erg cm-2 s-1
CLASSX
AGN (0.652)
Detections
3

SRCID 3001183020100016
IAUNAME 5XMM J152517.0+513440
SC_RA 15h25m17.01s (231.32087°)
SC_DEC +51d34m40.6s (51.57793°)
RADEC_ERR 0.67 arcsec
LII / BII 83.8171° / 52.2156°
N_CONTRIB 3 (detections)
N_OBS 3 (observations covering the position)
MJD_FIRST 52120.591 (2001-07-30 14:11:33.000 UTC)
MJD_LAST 52256.395 (2001-12-13 09:28:36.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.48e-14 ± 5.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.14 ± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.15 ± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.39 ± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.47 ± 0.31
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML 4.9) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 3.37

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
3925775
Match probability
0.997
FilterMag (AB)Err
UVW2
UVM2
UVW1 20.983 0.093
U
B
V

Spectroscopic (zsp) 1.84000
Photometric (TPZ) 1.7755 (conf 0.79)
Photometric (Le Phare) 1.7620 (conf 0.95)

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

Stacked power-law fit
Unabsorbed flux 2.08e-14 (+2.5e-14 / −1.7e-14) erg cm−2 s−1
NH 1.32e+20 (+6.3e+20 / −2.5e+19) cm−2
Photon index (Γ) 2.15 (+2.46 / −1.95)
DoF 415
p-value 0.863
Inter-instrument norm. 0.82 (0.67–1.05)
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.