5XMM J051705.2-542328
5XMM-DR15 stacked source · SRCID 3004234070100024
Position:
05h17m05.21s -54d23m28.9s
(79.27171°, -54.39135°)
EP flux
2.06e-14
± 5.8e-15
erg cm-2 s-1
CLASSX
AGN
(0.959)
Detections
3
| SRCID | 3004234070100024 |
|---|---|
| IAUNAME | 5XMM J051705.2-542328 |
| SC_RA | 05h17m05.21s (79.27171°) |
| SC_DEC | -54d23m28.9s (-54.39135°) |
| RADEC_ERR | 0.62 arcsec |
| LII / BII | 262.0931° / -35.3154° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52199.200 (2001-10-17 04:47:25.000 UTC) |
| MJD_LAST | 56297.130 (2013-01-05 03:07:32.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.06e-14 ± 5.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.08
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.20
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.55
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.27
± 0.34
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.4)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.304
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
- 1451436
- Match probability
- 0.894
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.541 | 0.137 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.86e-14 (+3.8e-14 / −2.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.42e+20 (+6.8e+20 / −2.4e+19) cm−2 |
| Photon index (Γ) | 1.32 (+1.62 / −1.12) |
| DoF | 143 |
| p-value | 0.957 |
| 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.