5XMM J034125.2-450045
5XMM-DR15 stacked source · SRCID 3004594030100027
Position:
03h41m25.29s -45d00m45.7s
(55.35539°, -45.01270°)
EP flux
1.10e-14
± 8.1e-15
erg cm-2 s-1
CLASSX
AGN
(0.949)
Detections
1
| SRCID | 3004594030100027 |
|---|---|
| IAUNAME | 5XMM J034125.2-450045 |
| SC_RA | 03h41m25.29s (55.35539°) |
| SC_DEC | -45d00m45.7s (-45.01270°) |
| RADEC_ERR | 1.07 arcsec |
| LII / BII | 252.2955° / -51.8512° |
| 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): 1.10e-14 ± 8.1e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.21
± 0.15
0.2-0.5 / 0.5-1.0 keV
HR2
0.09
± 0.16
0.5-1.0 / 1.0-2.0 keV
HR3
-0.60
± 0.21
1.0-2.0 / 2.0-4.5 keV
HR4
-1.00
± 1.71
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.
AGN
CLASSX outlier: 0.742
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
- 999387
- Match probability
- 0.994
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 20.374 | 0.093 |
| B | 19.492 | 0.108 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.32e-15 (+1.1e-14 / −6.4e-15) erg cm−2 s−1 |
|---|---|
| NH | 5.63e+19 (+2.8e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 2.59 (+2.85 / −2.26) |
| DoF | 159 |
| p-value | 0.944 |
| 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.