5XMM J001959.5+220603

5XMM-DR15 stacked source · SRCID 3004794010100020
Position: 00h19m59.55s +22d06m03.0s (4.99812°, 22.10084°)
EP flux
1.55e-14 ± 6.8e-15 erg cm-2 s-1
CLASSX
AGN (0.768)
Detections
1

SRCID 3004794010100020
IAUNAME 5XMM J001959.5+220603
SC_RA 00h19m59.55s (4.99812°)
SC_DEC +22d06m03.0s (22.10084°)
RADEC_ERR 1.11 arcsec
LII / BII 113.3832° / -40.1872°
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): 1.55e-14 ± 6.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.00 ± 0.16
0.2-0.5 / 0.5-1.0 keV
HR2
-0.21 ± 0.19
0.5-1.0 / 1.0-2.0 keV
HR3
-0.37 ± 0.26
1.0-2.0 / 2.0-4.5 keV
HR4
-0.69 ± 0.68
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.7) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 1.07

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
29378
Match probability
0.998
FilterMag (AB)Err
UVW2 20.622 0.227
UVM2 — —
UVW1 — —
U — —
B — —
V — —

Spectroscopic (zsp) 1.19400
Photometric (TPZ) 1.0757 (conf 0.58)
Photometric (Le Phare) 0.9622 (conf 0.73)

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

Stacked power-law fit
Unabsorbed flux 1.32e-14 (+1.8e-14 / −1.0e-14) erg cm−2 s−1
NH 9.43e+19 (+4.3e+20 / −2.0e+19) cm−2
Photon index (Γ) 2.53 (+2.85 / −2.22)
DoF 64
p-value 0.88
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.