5XMM J001959.4+215435

5XMM-DR15 stacked source · SRCID 3004794010100005
Position: 00h19m59.40s +21d54m35.9s (4.99750°, 21.90998°)
EP flux
4.68e-14 ± 6.6e-15 erg cm-2 s-1
CLASSX
AGN (0.922)
Detections
1

SRCID 3004794010100005
IAUNAME 5XMM J001959.4+215435
SC_RA 00h19m59.40s (4.99750°)
SC_DEC +21d54m35.9s (21.90998°)
RADEC_ERR 0.51 arcsec
LII / BII 113.3426° / -40.3755°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52274.800 (2001-12-31 19:12:31.000 UTC)
MJD_LAST 52275.441 (2002-01-01 10:35:25.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.68e-14 ± 6.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.19 ± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
0.02 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.44 ± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.05 ± 0.16
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: -0.655

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
29362
Match probability
0.999
FilterMag (AB)Err
UVW2 21.457 0.250
UVM2 — —
UVW1 — —
U — —
B — —
V — —

Spectroscopic (zsp) 1.19600
Photometric (TPZ) 1.2756 (conf 0.77)
Photometric (Le Phare) 1.1400 (conf 0.82)

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

Stacked power-law fit
Unabsorbed flux 2.54e-14 (+3.0e-14 / −2.1e-14) erg cm−2 s−1
NH 9.24e+20 (+1.7e+21 / −2.9e+20) cm−2
Photon index (Γ) 2.25 (+2.68 / −1.91)
DoF 323
p-value 0.427
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.