5XMM J144924.4+085937

5XMM-DR15 stacked source · SRCID 3005756030100004
Position: 14h49m24.45s +08d59m37.6s (222.35187°, 8.99377°)
EP flux
5.87e-14 ± 2.5e-15 erg cm-2 s-1
CLASSX
AGN (0.824)
Detections
3

SRCID 3005756030100004
IAUNAME 5XMM J144924.4+085937
SC_RA 14h49m24.45s (222.35187°)
SC_DEC +08d59m37.6s (8.99377°)
RADEC_ERR 0.18 arcsec
LII / BII 5.4541° / 56.7643°
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): 5.87e-14 ± 2.5e-15 erg cm-2 s-1

Hardness ratios
HR1
0.04 ± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.03 ± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38 ± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.50 ± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.8) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.415

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
3782149
Match probability
0.997
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 22.194 0.280
B 21.919 0.220
V 21.150 0.268

Photometric (TPZ) 0.3259 (conf 0.61)
Photometric (Le Phare) 0.5159 (conf 0.48)

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

Stacked power-law fit
Unabsorbed flux 4.15e-14 (+4.5e-14 / −3.8e-14) erg cm−2 s−1
NH 3.69e+19 (+1.1e+20 / −1.5e+19) cm−2
Photon index (Γ) 1.86 (+1.94 / −1.79)
DoF 537
p-value 0.758
Inter-instrument norm. 1.17 (1.06–1.29)
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.