5XMM J132424.5+300726

5XMM-DR15 stacked source · SRCID 3002574020100037
Position: 13h24m24.51s +30d07m26.6s (201.10212°, 30.12406°)
EP flux
3.66e-14 ± 1.0e-14 erg cm-2 s-1
CLASSX
AGN (0.789)
Detections
1

SRCID 3002574020100037
IAUNAME 5XMM J132424.5+300726
SC_RA 13h24m24.51s (201.10212°)
SC_DEC +30d07m26.6s (30.12406°)
RADEC_ERR 0.67 arcsec
LII / BII 57.3653° / 82.1720°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52255.718 (2001-12-12 17:14:17.000 UTC)
MJD_LAST 52256.169 (2001-12-13 04:02:51.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.66e-14 ± 1.0e-14 erg cm-2 s-1

Hardness ratios
HR1
0.13 ± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.09 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.10 ± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.43 ± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.3) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.619

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
3471621
Match probability
0.996
FilterMag (AB)Err
UVW2
UVM2
UVW1 20.978 0.084
U 20.956 0.088
B
V

Spectroscopic (zsp) 0.70500
Photometric (TPZ) 0.7258 (conf 0.74)
Photometric (Le Phare) 0.4728 (conf 0.57)

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

Stacked power-law fit
Unabsorbed flux 2.80e-14 (+3.5e-14 / −2.3e-14) erg cm−2 s−1
NH 1.61e+21 (+3.0e+21 / −2.1e+20) cm−2
Photon index (Γ) 2.12 (+2.58 / −1.62)
DoF 66
p-value 0.578
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.