5XMM J152636.7+513307

5XMM-DR15 stacked source · SRCID 3001183020100006
Position: 15h26m36.70s +51d33m07.0s (231.65294°, 51.55194°)
EP flux
3.22e-14 ± 5.0e-15 erg cm-2 s-1
CLASSX
AGN (0.87)
Detections
3

SRCID 3001183020100006
IAUNAME 5XMM J152636.7+513307
SC_RA 15h26m36.70s (231.65294°)
SC_DEC +51d33m07.0s (51.55194°)
RADEC_ERR 0.47 arcsec
LII / BII 83.6357° / 52.0398°
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): 3.22e-14 ± 5.0e-15 erg cm-2 s-1

Hardness ratios
HR1
0.00 ± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
0.07 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.27 ± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.78 ± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.8) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.338

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
3927276
Match probability
0.999
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.169 0.146
U
B
V

Spectroscopic (zsp) 0.15600
Photometric (TPZ) 0.1260 (conf 0.52)
Photometric (Le Phare) 0.1950 (conf 1.00)

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

Stacked power-law fit
Unabsorbed flux 3.43e-14 (+4.0e-14 / −2.9e-14) erg cm−2 s−1
NH 4.87e+19 (+1.5e+20 / −1.7e+19) cm−2
Photon index (Γ) 1.74 (+1.88 / −1.61)
DoF 475
p-value 0.456
Inter-instrument norm. 1.07 (0.91–1.29)
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.