5XMM J034058.7-445850
5XMM-DR15 stacked source · SRCID 3004594030100031
Position:
03h40m58.75s -44d58m50.8s
(55.24481°, -44.98078°)
EP flux
1.11e-14
± 6.9e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
1
| SRCID | 3004594030100031 |
|---|---|
| IAUNAME | 5XMM J034058.7-445850 |
| SC_RA | 03h40m58.75s (55.24481°) |
| SC_DEC | -44d58m50.8s (-44.98078°) |
| RADEC_ERR | 1.01 arcsec |
| LII / BII | 252.2743° / -51.9346° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52512.427 (2002-08-26 10:14:56.000 UTC) |
| MJD_LAST | 52512.793 (2002-08-26 19:01:59.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.11e-14 ± 6.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.29
± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
-0.81
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.71
± 0.28
1.0-2.0 / 2.0-4.5 keV
HR4
0.69
± 0.69
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 0.808
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
- 997795
- Match probability
- 0.995
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 16.183 | 0.021 |
| UVM2 | — | — |
| UVW1 | 14.039 | 0.004 |
| U | 13.124 | 0.002 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.16e-15 (+1.1e-14 / −6.2e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.30e+20 (+6.0e+20 / −2.1e+19) cm−2 |
| Photon index (Γ) | 2.54 (+2.85 / −2.14) |
| DoF | 161 |
| p-value | 0.354 |
| 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.