5XMM J152549.7+513703

5XMM-DR15 stacked source · SRCID 3001183020100024
Position: 15h25m49.75s +51d37m03.5s (231.45729°, 51.61764°)
EP flux
1.33e-14 ± 3.1e-15 erg cm-2 s-1
CLASSX
AGN (0.921)
Detections
3

SRCID 3001183020100024
IAUNAME 5XMM J152549.7+513703
SC_RA 15h25m49.75s (231.45729°)
SC_DEC +51d37m03.5s (51.61764°)
RADEC_ERR 0.77 arcsec
LII / BII 83.8165° / 52.1220°
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): 1.33e-14 ± 3.1e-15 erg cm-2 s-1

Hardness ratios
HR1
0.21 ± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
-0.22 ± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.34 ± 0.16
1.0-2.0 / 2.0-4.5 keV
HR4
-0.28 ± 0.26
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.0) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.673

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
3926089
Match probability
0.506
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.686 0.228
U
B
V

Photometric (TPZ) 3.0751 (conf 0.94)
Photometric (Le Phare) 3.0020 (conf 0.89)

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

Stacked power-law fit
Unabsorbed flux 1.27e-14 (+1.8e-14 / −9.1e-15) erg cm−2 s−1
NH 4.45e+20 (+1.6e+21 / −4.7e+19) cm−2
Photon index (Γ) 1.84 (+2.50 / −1.51)
DoF 274
p-value 0.36
Inter-instrument norm. 1.04 (0.79–1.38)
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.