5XMM J144941.0+090212

5XMM-DR15 stacked source · SRCID 3005756030100027
Position: 14h49m41.05s +09d02m12.5s (222.42106°, 9.03680°)
EP flux
1.17e-14 ± 2.4e-15 erg cm-2 s-1
CLASSX
AGN (0.892)
Detections
3

SRCID 3005756030100027
IAUNAME 5XMM J144941.0+090212
SC_RA 14h49m41.05s (222.42106°)
SC_DEC +09d02m12.5s (9.03680°)
RADEC_ERR 0.55 arcsec
LII / BII 5.5917° / 56.7354°
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): 1.17e-14 ± 2.4e-15 erg cm-2 s-1

Hardness ratios
HR1
0.44 ± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.19 ± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.58 ± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.26 ± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.2) SUM_FLAG: 2
Long-term lightcurve

AGN

CLASSX outlier: 0.258

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
3782731
Match probability
0.991
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 21.740 0.184
B 20.849 0.078
V 20.725 0.156

Spectroscopic (zsp) 2.52200
Photometric (TPZ) 2.4253 (conf 0.88)
Photometric (Le Phare) 2.3640 (conf 0.99)

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

Stacked power-law fit
Unabsorbed flux 4.85e-14 (+5.9e-14 / −4.0e-14) erg cm−2 s−1
NH 1.89e+20 (+9.1e+20 / −2.4e+19) cm−2
Photon index (Γ) 1.56 (+1.85 / −1.36)
DoF 138
p-value 0.134
Inter-instrument norm. 0.53 (0.51–0.56)
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.