5XMM J005559.8-011737
5XMM-DR15 stacked source · SRCID 3001244010100145
Position:
00h55m59.89s -01d17m37.1s
(13.99955°, -1.29365°)
EP flux
5.79e-15
± 3.0e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.532)
Detections
4
| SRCID | 3001244010100145 |
|---|---|
| IAUNAME | 5XMM J005559.8-011737 |
| SC_RA | 00h55m59.89s (13.99955°) |
| SC_DEC | -01d17m37.1s (-1.29365°) |
| RADEC_ERR | 1.36 arcsec |
| LII / BII | 125.5460° / -64.1423° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 4 (observations covering the position) |
| MJD_FIRST | 51923.975 (2001-01-14 23:23:18.000 UTC) |
| MJD_LAST | 57210.407 (2015-07-07 09:46:43.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 5.79e-15 ± 3.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.53
± 0.20
0.2-0.5 / 0.5-1.0 keV
HR2
-0.51
± 0.23
0.5-1.0 / 1.0-2.0 keV
HR3
-0.54
± 0.42
1.0-2.0 / 2.0-4.5 keV
HR4
0.63
± 0.43
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 2.55
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
- 336850
- Match probability
- 0.989
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.077 | 0.211 |
| U | — | — |
| B | 19.341 | 0.085 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.73e-14 (+4.4e-14 / −3.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.15e+20 (+5.0e+20 / −2.5e+19) cm−2 |
| Photon index (Γ) | 1.63 (+1.87 / −1.48) |
| DoF | 239 |
| p-value | 0.976 |
| 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.