5XMM J144951.1+085243

5XMM-DR15 stacked source · SRCID 3005756030100022
Position: 14h49m51.13s +08d52m43.6s (222.46306°, 8.87879°)
EP flux
4.11e-14 ± 5.8e-15 erg cm-2 s-1
CLASSX
AGN (0.876)
Detections
3

SRCID 3005756030100022
IAUNAME 5XMM J144951.1+085243
SC_RA 14h49m51.13s (222.46306°)
SC_DEC +08d52m43.6s (8.87879°)
RADEC_ERR 0.39 arcsec
LII / BII 5.4071° / 56.6074°
N_CONTRIB 3 (detections)
N_OBS 3 (observations covering the position)
MJD_FIRST 52130.132 (2001-08-09 03:10:43.000 UTC)
MJD_LAST 52868.447 (2003-08-17 10:44:11.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.11e-14 ± 5.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.15 ± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
0.02 ± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.44 ± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.04 ± 0.15
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.9) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.0892

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
3783012
Match probability
0.996
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 21.650 0.088
B 21.671 0.166
V — —

Photometric (TPZ) 2.0254 (conf 0.78)
Photometric (Le Phare) 2.0020 (conf 0.74)

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

Stacked power-law fit
Unabsorbed flux 3.18e-14 (+3.8e-14 / −2.7e-14) erg cm−2 s−1
NH 6.61e+19 (+2.6e+20 / −1.9e+19) cm−2
Photon index (Γ) 1.66 (+1.82 / −1.52)
DoF 241
p-value 0.558
Inter-instrument norm. 1.22 (0.97–1.49)
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.