5XMM J130958.8+322506

5XMM-DR15 stacked source · SRCID 3002054040100038
Position: 13h09m58.80s +32d25m06.0s (197.49502°, 32.41832°)
EP flux
1.54e-14 ± 2.5e-15 erg cm-2 s-1
CLASSX
AGN (0.906)
Detections
1

SRCID 3002054040100038
IAUNAME 5XMM J130958.8+322506
SC_RA 13h09m58.80s (197.49502°)
SC_DEC +32d25m06.0s (32.41832°)
RADEC_ERR 0.66 arcsec
LII / BII 86.8030° / 83.3555°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52618.145 (2002-12-10 03:28:52.000 UTC)
MJD_LAST 52618.715 (2002-12-10 17:09:55.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.54e-14 ± 2.5e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.35 ± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.18 ± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
0.20 ± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.56 ± 0.13
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.2) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: -0.44

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
3420842
Match probability
0.998
FilterMag (AB)Err
UVW2 21.772 0.215
UVM2
UVW1 21.348 0.064
U
B
V

Spectroscopic (zsp) 0.81500
Photometric (TPZ) 0.7758 (conf 0.58)
Photometric (Le Phare) 2.0840 (conf 0.64)

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

Stacked power-law fit
Unabsorbed flux 1.12e-14 (+1.4e-14 / −8.8e-15) erg cm−2 s−1
NH 4.54e+19 (+1.8e+20 / −1.6e+19) cm−2
Photon index (Γ) 1.49 (+1.72 / −1.31)
DoF 116
p-value 0.348
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.