5XMM J001551.4-390642
5XMM-DR15 stacked source · SRCID 3002874010100139
Position:
00h15m51.46s -39d06m42.0s
(3.96441°, -39.11165°)
EP flux
1.67e-14
± 4.9e-15
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
10
| SRCID | 3002874010100139 |
|---|---|
| IAUNAME | 5XMM J001551.4-390642 |
| SC_RA | 00h15m51.46s (3.96441°) |
| SC_DEC | -39d06m42.0s (-39.11165°) |
| RADEC_ERR | 1.75 arcsec |
| LII / BII | 332.4521° / -75.9072° |
| N_CONTRIB | 10 (detections) |
| N_OBS | 10 (observations covering the position) |
| MJD_FIRST | 52227.605 (2001-11-14 14:31:49.000 UTC) |
| MJD_LAST | 59561.812 (2021-12-13 19:29:06.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.67e-14 ± 4.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.50
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.54
± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.87
± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
0.81
± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent:
16.65
± 0.88
arcsec
(ML 244.8)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 2.33
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
- 25282
- Match probability
- 0.958
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 19.045 | 0.096 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.53e-15 (+6.0e-15 / −2.2e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.22e+20 (+6.8e+20 / −2.1e+19) cm−2 |
| Photon index (Γ) | 2.18 (+2.69 / −1.61) |
| DoF | 133 |
| p-value | 0.493 |
| 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.