5XMM J005602.7-012003
5XMM-DR15 stacked source · SRCID 3001244010100038
Position:
00h56m02.75s -01d20m03.6s
(14.01144°, -1.33433°)
EP flux
1.32e-14
± 2.7e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.965)
Detections
4
| SRCID | 3001244010100038 |
|---|---|
| IAUNAME | 5XMM J005602.7-012003 |
| SC_RA | 00h56m02.75s (14.01144°) |
| SC_DEC | -01d20m03.6s (-1.33433°) |
| RADEC_ERR | 0.60 arcsec |
| LII / BII | 125.5771° / -64.1824° |
| 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): 1.32e-14 ± 2.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.69
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
-0.35
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.83
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
0.25
± 0.38
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 6.3)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 3.92
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
- 337575
- Match probability
- 0.993
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 19.433 | 0.104 |
| U | — | — |
| B | 16.396 | 0.018 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.67e-14 (+2.1e-14 / −1.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 8.96e+20 (+1.6e+21 / −1.2e+20) cm−2 |
| Photon index (Γ) | 2.33 (+2.78 / −1.88) |
| DoF | 351 |
| p-value | 0.433 |
| Inter-instrument norm. | 1.53 (1.26–1.79) |
| 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.