5XMM J163327.5+571027

5XMM-DR15 stacked source · SRCID 3004954010100033
Position: 16h33m27.57s +57d10m27.4s (248.36486°, 57.17428°)
EP flux
2.00e-14 ± 5.3e-15 erg cm-2 s-1
CLASSX
AGN (0.888)
Detections
6

SRCID 3004954010100033
IAUNAME 5XMM J163327.5+571027
SC_RA 16h33m27.57s (248.36486°)
SC_DEC +57d10m27.4s (57.17428°)
RADEC_ERR 0.58 arcsec
LII / BII 86.6175° / 41.0258°
N_CONTRIB 6 (detections)
N_OBS 6 (observations covering the position)
MJD_FIRST 52208.338 (2001-10-26 08:07:10.000 UTC)
MJD_LAST 53674.442 (2005-10-31 10:36:41.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.00e-14 ± 5.3e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.04 ± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.19 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.40 ± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.10 ± 0.24
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.5) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.454

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
4234556
Match probability
0.996
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 20.841 0.035
B — —
V — —

Spectroscopic (zsp) 1.52000
Photometric (TPZ) 0.4259 (conf 0.35)
Photometric (Le Phare) 1.8330 (conf 0.58)

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

Stacked power-law fit
Unabsorbed flux 5.36e-14 (+6.6e-14 / −4.3e-14) erg cm−2 s−1
NH 5.69e+19 (+2.4e+20 / −1.8e+19) cm−2
Photon index (Γ) 1.88 (+2.11 / −1.68)
DoF 185
p-value 0.699
Inter-instrument norm. 0.55 (0.51–0.63)
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.