5XMM J210434.3-111619
5XMM-DR15 stacked source · SRCID 3004115010100009
Position:
21h04m34.33s -11d16m19.7s
(316.14303°, -11.27213°)
EP flux
1.60e-14
± 6.0e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
1
| SRCID | 3004115010100009 |
|---|---|
| IAUNAME | 5XMM J210434.3-111619 |
| SC_RA | 21h04m34.33s (316.14303°) |
| SC_DEC | -11d16m19.7s (-11.27213°) |
| RADEC_ERR | 0.68 arcsec |
| LII / BII | 37.9123° / -34.6192° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52029.408 (2001-04-30 09:48:01.000 UTC) |
| MJD_LAST | 52029.869 (2001-04-30 20:51:37.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.60e-14 ± 6.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.63
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.70
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.93
± 0.16
1.0-2.0 / 2.0-4.5 keV
HR4
0.36
± 1.56
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.3)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 0.521
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
- 6275438
- Match probability
- 0.984
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 14.356 | 0.006 |
| UVM2 | — | — |
| UVW1 | 12.486 | 0.001 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.24e-14 (+1.5e-14 / −1.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 6.99e+20 (+1.2e+21 / −1.5e+20) cm−2 |
| Photon index (Γ) | 2.78 (+2.94 / −2.47) |
| DoF | 114 |
| p-value | 0.012 |
| 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
No hardness-ratio pairs available for this source.
The per-observation light curve is shown in the X-ray properties section above.