5XMM J101752.8+412423

5XMM-DR15 stacked source · SRCID 3002874030100010
Position: 10h17m52.88s +41d24m23.4s (154.47035°, 41.40649°)
EP flux
6.14e-14 ± 1.2e-14 erg cm-2 s-1
CLASSX
AGN (0.759)
Detections
1

SRCID 3002874030100010
IAUNAME 5XMM J101752.8+412423
SC_RA 10h17m52.88s (154.47035°)
SC_DEC +41d24m23.4s (41.40649°)
RADEC_ERR 0.57 arcsec
LII / BII 178.3941° / 55.5681°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52215.969 (2001-11-02 23:15:02.000 UTC)
MJD_LAST 52216.312 (2001-11-03 07:28:39.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 6.14e-14 ± 1.2e-14 erg cm-2 s-1

Hardness ratios
HR1
0.05 ± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.03 ± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.35 ± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.53 ± 0.24
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.6) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 1.53

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
2859423
Match probability
0.928
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.404 0.157
U 22.031 0.368
B
V 20.970 0.381

Photometric (TPZ) 0.6758 (conf 0.67)
Photometric (Le Phare) 0.5468 (conf 0.93)

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

Stacked power-law fit
Unabsorbed flux 6.32e-14 (+7.2e-14 / −5.5e-14) erg cm−2 s−1
NH 4.55e+19 (+1.6e+20 / −1.7e+19) cm−2
Photon index (Γ) 1.72 (+1.85 / −1.61)
DoF 410
p-value 0.461
Inter-instrument norm. 1.05 (0.90–1.23)
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.