5XMM J152636.4+513456

5XMM-DR15 stacked source · SRCID 3001183020100029
Position: 15h26m36.40s +51d34m56.3s (231.65166°, 51.58230°)
EP flux
2.00e-14 ± 6.4e-15 erg cm-2 s-1
CLASSX
AGN (0.915)
Detections
3

SRCID 3001183020100029
IAUNAME 5XMM J152636.4+513456
SC_RA 15h26m36.40s (231.65166°)
SC_DEC +51d34m56.3s (51.58230°)
RADEC_ERR 0.65 arcsec
LII / BII 83.6810° / 52.0277°
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): 2.00e-14 ± 6.4e-15 erg cm-2 s-1

Hardness ratios
HR1
0.14 ± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
-0.15 ± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.28 ± 0.17
1.0-2.0 / 2.0-4.5 keV
HR4
-0.27 ± 0.36
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.2) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.323

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
3927267
Match probability
0.998
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.053 0.080
U
B
V

Spectroscopic (zsp) 1.95400
Photometric (TPZ) 1.5256 (conf 0.66)
Photometric (Le Phare) 1.6550 (conf 0.58)

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

Stacked power-law fit
Unabsorbed flux 1.46e-14 (+2.3e-14 / −9.0e-15) erg cm−2 s−1
NH 8.42e+20 (+2.3e+21 / −5.8e+19) cm−2
Photon index (Γ) 2.07 (+2.65 / −1.51)
DoF 169
p-value 0.12
Inter-instrument norm. 1.23 (0.81–1.69)
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.