5XMM J092101.4-631653
5XMM-DR15 stacked source · SRCID 3005159010100068
Position:
09h21m01.42s -63d16m53.1s
(140.25590°, -63.28141°)
EP flux
2.25e-14
± 6.1e-15
erg cm-2 s-1
CLASSX
AGN
(0.935)
Detections
2
| SRCID | 3005159010100068 |
|---|---|
| IAUNAME | 5XMM J092101.4-631653 |
| SC_RA | 09h21m01.42s (140.25590°) |
| SC_DEC | -63d16m53.1s (-63.28141°) |
| RADEC_ERR | 0.85 arcsec |
| LII / BII | 281.7019° / -9.4552° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 51898.315 (2000-12-20 07:32:54.000 UTC) |
| MJD_LAST | 51899.141 (2000-12-21 03:23:20.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.25e-14 ± 6.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.66
± 1.29
0.2-0.5 / 0.5-1.0 keV
HR2
0.98
± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.07
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.58
± 0.20
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.1)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.158
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
- 2734569
- Match probability
- 0.612
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 21.846 | 0.275 |
| UVW1 | 20.247 | 0.055 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.36e-14 (+2.9e-14 / −1.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.62e+22 (+2.1e+22 / −1.2e+22) cm−2 |
| Photon index (Γ) | 2.51 (+2.83 / −2.02) |
| DoF | 91 |
| p-value | 0.479 |
| 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.