5XMM J152510.7+513959

5XMM-DR15 stacked source · SRCID 3001183020100015
Position: 15h25m10.76s +51d39m59.0s (231.29484°, 51.66640°)
EP flux
4.28e-14 ± 9.9e-15 erg cm-2 s-1
CLASSX
AGN (0.915)
Detections
3

SRCID 3001183020100015
IAUNAME 5XMM J152510.7+513959
SC_RA 15h25m10.76s (231.29484°)
SC_DEC +51d39m59.0s (51.66640°)
RADEC_ERR 0.66 arcsec
LII / BII 83.9587° / 52.1921°
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): 4.28e-14 ± 9.9e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.17 ± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
0.16 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.37 ± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.26 ± 0.25
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: -0.611

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
3925723
Match probability
0.997
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.007 0.170
U
B
V

Spectroscopic (zsp) 1.13800
Photometric (TPZ) 1.1257 (conf 0.73)
Photometric (Le Phare) 1.1100 (conf 0.81)

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

Stacked power-law fit
Unabsorbed flux 2.89e-14 (+3.7e-14 / −2.2e-14) erg cm−2 s−1
NH 8.65e+19 (+3.8e+20 / −2.1e+19) cm−2
Photon index (Γ) 1.86 (+2.11 / −1.63)
DoF 197
p-value 0.95
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.