5XMM J083749.0+254413

5XMM-DR15 stacked source · SRCID 3002554030100022
Position: 08h37m49.01s +25d44m13.4s (129.45420°, 25.73705°)
EP flux
6.32e-14 ± 2.7e-14 erg cm-2 s-1
CLASSX
AGN (0.952)
Detections
1

SRCID 3002554030100022
IAUNAME 5XMM J083749.0+254413
SC_RA 08h37m49.01s (129.45420°)
SC_DEC +25d44m13.4s (25.73705°)
RADEC_ERR 0.81 arcsec
LII / BII 198.8143° / 33.8423°
N_CONTRIB 1 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52026.319 (2001-04-27 07:38:53.000 UTC)
MJD_LAST 52026.458 (2001-04-27 10:59:04.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 6.32e-14 ± 2.7e-14 erg cm-2 s-1

Hardness ratios
HR1
0.09 ± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.11 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.66 ± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
0.52 ± 0.54
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.4) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.304

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
2599442
Match probability
0.999
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 18.575 0.032
B
V

Spectroscopic (zsp) 1.90900
Photometric (TPZ) 1.9255 (conf 0.90)
Photometric (Le Phare) 1.7590 (conf 1.00)

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

Stacked power-law fit
Unabsorbed flux 5.24e-14 (+6.3e-14 / −4.5e-14) erg cm−2 s−1
NH 1.97e+20 (+7.9e+20 / −2.6e+19) cm−2
Photon index (Γ) 2.59 (+2.85 / −2.30)
DoF 57
p-value 0.603
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.