5XMM J003415.1-211749

5XMM-DR15 stacked source · SRCID 3004435010100002
Position: 00h34m15.18s -21d17m49.1s (8.56324°, -21.29697°)
EP flux
1.77e-13 ± 1.7e-14 erg cm-2 s-1
CLASSX
AGN (0.849)
Detections
1

SRCID 3004435010100002
IAUNAME 5XMM J003415.1-211749
SC_RA 00h34m15.18s (8.56324°)
SC_DEC -21d17m49.1s (-21.29697°)
RADEC_ERR 0.35 arcsec
LII / BII 88.1267° / -82.9762°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52423.209 (2002-05-29 05:01:16.000 UTC)
MJD_LAST 52423.467 (2002-05-29 11:12:36.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.77e-13 ± 1.7e-14 erg cm-2 s-1

Hardness ratios
HR1
0.13 ± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.05 ± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.32 ± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.56 ± 0.11
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.1) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.511

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
71307
Match probability
0.998
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 19.804 0.094
U 19.679 0.096
B 19.401 0.076
V — —

Photometric (TPZ) 0.4259 (conf 0.74)
Photometric (Le Phare) 0.4812 (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 1.48e-13 (+1.6e-13 / −1.3e-13) erg cm−2 s−1
NH 4.64e+19 (+1.5e+20 / −1.7e+19) cm−2
Photon index (Γ) 1.90 (+2.02 / −1.80)
DoF 606
p-value 0.049
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.