5XMM J152545.8+515007

5XMM-DR15 stacked source · SRCID 3001183020100023
Position: 15h25m45.84s +51d50m07.3s (231.44101°, 51.83537°)
EP flux
4.10e-14 ± 1.3e-14 erg cm-2 s-1
CLASSX
AGN (0.924)
Detections
3

SRCID 3001183020100023
IAUNAME 5XMM J152545.8+515007
SC_RA 15h25m45.84s (231.44101°)
SC_DEC +51d50m07.3s (51.83537°)
RADEC_ERR 0.75 arcsec
LII / BII 84.1435° / 52.0377°
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): 4.10e-14 ± 1.3e-14 erg cm-2 s-1

Hardness ratios
HR1
-0.03 ± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.13 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.45 ± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.37 ± 0.38
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.3) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.516

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.

No multi-wavelength counterpart data available for this source.

Spectroscopic (zsp) 1.72400
Photometric (TPZ) 1.7755 (conf 0.78)
Photometric (Le Phare) 1.6180 (conf 0.85)

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

Stacked power-law fit
Unabsorbed flux 6.52e-14 (+8.5e-14 / −4.8e-14) erg cm−2 s−1
NH 8.53e+19 (+4.1e+20 / −2.0e+19) cm−2
Photon index (Γ) 1.42 (+1.66 / −1.22)
DoF 370
p-value 0.9
Inter-instrument norm. 0.76 (0.59–1.01)
Quality flag 0

APPROX_SOURCE_VAR 5.800 (approximate flux variability amplitude)

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.