5XMM J161115.8+540927

5XMM-DR15 stacked source · SRCID 3005975230100029
Position: 16h11m15.82s +54d09m27.8s (242.81593°, 54.15773°)
EP flux
6.39e-14 ± 8.1e-15 erg cm-2 s-1
CLASSX
AGN (0.934)
Detections
5

SRCID 3005975230100029
IAUNAME 5XMM J161115.8+540927
SC_RA 16h11m15.82s (242.81593°)
SC_DEC +54d09m27.8s (54.15773°)
RADEC_ERR 0.39 arcsec
LII / BII 83.7335° / 44.8230°
N_CONTRIB 5 (detections)
N_OBS 12 (observations covering the position)
MJD_FIRST 52529.479 (2002-09-12 11:30:08.000 UTC)
MJD_LAST 52575.391 (2002-10-28 09:22:54.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 6.39e-14 ± 8.1e-15 erg cm-2 s-1

Hardness ratios
HR1
0.12 ± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.03 ± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.34 ± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.40 ± 0.13
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.8) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.0213

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
4083742
Match probability
0.994
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.822 0.314
U 21.674 0.126
B 21.246 0.118
V — —

Spectroscopic (zsp) 1.92900
Photometric (TPZ) 1.8755 (conf 0.65)
Photometric (Le Phare) 1.8870 (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 7.04e-14 (+8.8e-14 / −5.6e-14) erg cm−2 s−1
NH 5.16e+19 (+2.2e+20 / −1.7e+19) cm−2
Photon index (Γ) 1.69 (+1.86 / −1.50)
DoF 560
p-value 0.41
Inter-instrument norm. 1.03 (0.85–1.24)
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.