5XMM J034155.4-445613
5XMM-DR15 stacked source · SRCID 3004594030100028
Position:
03h41m55.44s -44d56m13.9s
(55.48101°, -44.93720°)
EP flux
1.16e-14
± 6.0e-15
erg cm-2 s-1
CLASSX
AGN
(0.954)
Detections
1
| SRCID | 3004594030100028 |
|---|---|
| IAUNAME | 5XMM J034155.4-445613 |
| SC_RA | 03h41m55.44s (55.48101°) |
| SC_DEC | -44d56m13.9s (-44.93720°) |
| RADEC_ERR | 1.01 arcsec |
| LII / BII | 252.1439° / -51.7819° |
| 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): 1.16e-14 ± 6.0e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.44
± 0.16
0.2-0.5 / 0.5-1.0 keV
HR2
0.30
± 0.19
0.5-1.0 / 1.0-2.0 keV
HR3
-0.51
± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
-0.94
± 0.46
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.8)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.0682
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
- 1000275
- Match probability
- 0.993
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.153 | 0.316 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.56e-15 (+1.2e-14 / −6.5e-15) erg cm−2 s−1 |
|---|---|
| NH | 8.35e+19 (+3.9e+20 / −1.9e+19) cm−2 |
| Photon index (Γ) | 2.44 (+2.79 / −2.13) |
| DoF | 162 |
| p-value | 0.949 |
| 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.