5XMM J033810.2+002325

5XMM-DR15 stacked source · SRCID 3003654010100026
Position: 03h38m10.21s +00d23m25.0s (54.54253°, 0.39027°)
EP flux
8.50e-14 ± 8.4e-15 erg cm-2 s-1
CLASSX
AGN (0.852)
Detections
1

SRCID 3003654010100026
IAUNAME 5XMM J033810.2+002325
SC_RA 03h38m10.21s (54.54253°)
SC_DEC +00d23m25.0s (0.39027°)
RADEC_ERR 0.36 arcsec
LII / BII 185.4031° / -41.4184°
N_CONTRIB 1 (detections)
N_OBS 17 (observations covering the position)
MJD_FIRST 52327.346 (2002-02-22 08:18:20.000 UTC)
MJD_LAST 52327.604 (2002-02-22 14:29:38.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 8.50e-14 ± 8.4e-15 erg cm-2 s-1

Hardness ratios
HR1
0.20 ± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
-0.04 ± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.43 ± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.60 ± 0.12
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.2) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.596

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
988464
Match probability
1
FilterMag (AB)Err
UVW2 19.961 0.137
UVM2
UVW1
U
B
V

Spectroscopic (zsp) 1.12400
Photometric (TPZ) 1.1757 (conf 0.88)
Photometric (Le Phare) 1.0510 (conf 0.98)

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

Stacked power-law fit
Unabsorbed flux 7.38e-14 (+8.1e-14 / −6.8e-14) erg cm−2 s−1
NH 1.14e+20 (+4.3e+20 / −2.2e+19) cm−2
Photon index (Γ) 2.00 (+2.16 / −1.90)
DoF 500
p-value 0.654
Inter-instrument norm. 1.00 (0.90–1.10)
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.