5XMM J152516.1+513709

5XMM-DR15 stacked source · SRCID 3001183020100038
Position: 15h25m16.13s +51d37m09.0s (231.31719°, 51.61916°)
EP flux
1.71e-14 ± 7.1e-15 erg cm-2 s-1
CLASSX
AGN (0.961)
Detections
3

SRCID 3001183020100038
IAUNAME 5XMM J152516.1+513709
SC_RA 15h25m16.13s (231.31719°)
SC_DEC +51d37m09.0s (51.61916°)
RADEC_ERR 0.88 arcsec
LII / BII 83.8794° / 52.1999°
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): 1.71e-14 ± 7.1e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.02 ± 0.15
0.2-0.5 / 0.5-1.0 keV
HR2
-0.00 ± 0.16
0.5-1.0 / 1.0-2.0 keV
HR3
-0.43 ± 0.19
1.0-2.0 / 2.0-4.5 keV
HR4
-0.17 ± 0.47
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.9) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.029

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
3925764
Match probability
0.998
FilterMag (AB)Err
UVW2
UVM2
UVW1 20.605 0.075
U
B
V

Spectroscopic (zsp) 1.55300
Photometric (TPZ) 1.5256 (conf 0.88)
Photometric (Le Phare) 1.7170 (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 6.67e-15 (+8.5e-15 / −5.2e-15) erg cm−2 s−1
NH 9.06e+19 (+4.0e+20 / −1.9e+19) cm−2
Photon index (Γ) 2.73 (+2.92 / −2.47)
DoF 74
p-value 0.493
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.