5XMM J173257.1+434401

5XMM-DR15 stacked source · SRCID 3002114050100014
Position: 17h32m57.14s +43d44m01.9s (263.23808°, 43.73385°)
EP flux
3.11e-14 ± 6.1e-15 erg cm-2 s-1
CLASSX
AGN (0.886)
Detections
10

SRCID 3002114050100014
IAUNAME 5XMM J173257.1+434401
SC_RA 17h32m57.14s (263.23808°)
SC_DEC +43d44m01.9s (43.73385°)
RADEC_ERR 0.63 arcsec
LII / BII 69.4863° / 32.0846°
N_CONTRIB 10 (detections)
N_OBS 11 (observations covering the position)
MJD_FIRST 52579.434 (2002-11-01 10:24:27.000 UTC)
MJD_LAST 58155.531 (2018-02-06 12:44:10.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.11e-14 ± 6.1e-15 erg cm-2 s-1

Hardness ratios
HR1
0.14 ± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
0.07 ± 0.15
0.5-1.0 / 1.0-2.0 keV
HR3
-0.13 ± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
-0.63 ± 0.18
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.0) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.636

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
4709094
Match probability
0.994
FilterMag (AB)Err
UVW2
UVM2
UVW1
U
B 20.369 0.071
V

Spectroscopic (zsp) 3.43000
Photometric (TPZ) 3.4250 (conf 0.36)
Photometric (Le Phare) 3.0280 (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 6.98e-14 (+8.3e-14 / −5.7e-14) erg cm−2 s−1
NH 1.57e+20 (+7.4e+20 / −2.6e+19) cm−2
Photon index (Γ) 2.13 (+2.41 / −1.94)
DoF 359
p-value 0.819
Inter-instrument norm. 0.77 (0.62–0.96)
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.