5XMM J001547.1-390519
5XMM-DR15 stacked source · SRCID 3002874010100273
Position:
00h15m47.19s -39d05m19.0s
(3.94663°, -39.08862°)
EP flux
1.04e-14
± 4.0e-15
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
10
| SRCID | 3002874010100273 |
|---|---|
| IAUNAME | 5XMM J001547.1-390519 |
| SC_RA | 00h15m47.19s (3.94663°) |
| SC_DEC | -39d05m19.0s (-39.08862°) |
| RADEC_ERR | 1.99 arcsec |
| LII / BII | 332.5524° / -75.9184° |
| 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): 1.04e-14 ± 4.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.12
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.57
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.42
± 0.29
1.0-2.0 / 2.0-4.5 keV
HR4
0.77
± 0.16
2.0-4.5 / 4.5-12.0 keV
Extent:
13.25
± 1.25
arcsec
(ML 30.9)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 2.28
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
- 25090
- Match probability
- 0.704
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.802 | 0.258 |
| U | — | — |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.00e-15 (+3.7e-15 / −1.3e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.28e+20 (+7.6e+20 / −2.3e+19) cm−2 |
| Photon index (Γ) | 2.35 (+2.79 / −1.71) |
| DoF | 300 |
| p-value | 0.187 |
| 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.