5XMM J152608.9+514433

5XMM-DR15 stacked source · SRCID 3001183020100012
Position: 15h26m08.98s +51d44m33.9s (231.53741°, 51.74275°)
EP flux
3.96e-14 ± 1.0e-14 erg cm-2 s-1
CLASSX
AGN (0.888)
Detections
3

SRCID 3001183020100012
IAUNAME 5XMM J152608.9+514433
SC_RA 15h26m08.98s (231.53741°)
SC_DEC +51d44m33.9s (51.74275°)
RADEC_ERR 0.64 arcsec
LII / BII 83.9660° / 52.0236°
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): 3.96e-14 ± 1.0e-14 erg cm-2 s-1

Hardness ratios
HR1
0.04 ± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.07 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.46 ± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
0.19 ± 0.23
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: 0.778

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
3926410
Match probability
0.999
FilterMag (AB)Err
UVW2
UVM2 20.742 0.295
UVW1 20.294 0.043
U
B
V

Spectroscopic (zsp) 1.39700
Photometric (TPZ) 1.3256 (conf 0.84)
Photometric (Le Phare) 1.3360 (conf 0.90)

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

Stacked power-law fit
Unabsorbed flux 3.78e-14 (+4.7e-14 / −3.0e-14) erg cm−2 s−1
NH 2.07e+20 (+8.5e+20 / −2.4e+19) cm−2
Photon index (Γ) 2.20 (+2.59 / −1.91)
DoF 205
p-value 0.56
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.