5XMM J105159.9+572424

5XMM-DR15 stacked source · SRCID 3002274010100114
Position: 10h51m59.91s +57d24m24.1s (162.99963°, 57.40671°)
EP flux
5.79e-15 ± 8.3e-16 erg cm-2 s-1
CLASSX
AGN (0.878)
Detections
16

SRCID 3002274010100114
IAUNAME 5XMM J105159.9+572424
SC_RA 10h51m59.91s (162.99963°)
SC_DEC +57d24m24.1s (57.40671°)
RADEC_ERR 0.36 arcsec
LII / BII 149.4789° / 53.1245°
N_CONTRIB 16 (detections)
N_OBS 21 (observations covering the position)
MJD_FIRST 51661.158 (2000-04-27 03:47:47.000 UTC)
MJD_LAST 52615.196 (2002-12-07 04:41:59.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 5.79e-15 ± 8.3e-16 erg cm-2 s-1

Hardness ratios
HR1
0.34 ± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
0.54 ± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.44 ± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.35 ± 0.14
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: -0.525

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
2953472
Match probability
0.946
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.803 0.305
U 22.834 0.148
B 21.756 0.197
V

Photometric (TPZ) 1.9255 (conf 0.29)
Photometric (Le Phare) 0.9291 (conf 0.29)

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

Stacked power-law fit
Unabsorbed flux 3.48e-14 (+4.2e-14 / −2.7e-14) erg cm−2 s−1
NH 1.64e+20 (+7.5e+20 / −3.1e+19) cm−2
Photon index (Γ) 1.25 (+1.46 / −1.08)
DoF 882
p-value 0.661
Inter-instrument norm. 0.90 (0.73–1.12)
Quality flag 0

APPROX_SOURCE_VAR 8.300 (approximate flux variability amplitude)

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.