5XMM J104921.7+325721

5XMM-DR15 stacked source · SRCID 3005599020100030
Position: 10h49m21.79s +32d57m21.1s (162.34079°, 32.95585°)
EP flux
8.08e-14 ± 1.4e-14 erg cm-2 s-1
CLASSX
AGN (0.968)
Detections
1

SRCID 3005599020100030
IAUNAME 5XMM J104921.7+325721
SC_RA 10h49m21.79s (162.34079°)
SC_DEC +32d57m21.1s (32.95585°)
RADEC_ERR 0.59 arcsec
LII / BII 192.9971° / 63.0466°
N_CONTRIB 1 (detections)
N_OBS 3 (observations covering the position)
MJD_FIRST 52226.012 (2001-11-13 00:17:04.000 UTC)
MJD_LAST 52226.450 (2001-11-13 10:48:00.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 8.08e-14 ± 1.4e-14 erg cm-2 s-1

Hardness ratios
HR1
0.14 ± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.04 ± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.16 ± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.44 ± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.6) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.366

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
2940525
Match probability
0.995
FilterMag (AB)Err
UVW2 20.560 0.164
UVM2 — —
UVW1 20.030 0.066
U 19.995 0.074
B — —
V 19.217 0.086

Spectroscopic (zsp) 1.04700
Photometric (TPZ) 1.4756 (conf 0.76)
Photometric (Le Phare) 1.7150 (conf 0.83)

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

Stacked power-law fit
Unabsorbed flux 6.79e-14 (+8.2e-14 / −5.4e-14) erg cm−2 s−1
NH 3.28e+19 (+9.5e+19 / −1.5e+19) cm−2
Photon index (Γ) 1.57 (+1.72 / −1.43)
DoF 1039
p-value 0.665
Inter-instrument norm. 1.02 (0.86–1.21)
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.