5XMM J033920.2-352921
5XMM-DR15 stacked source · SRCID 3001283010100008
Position:
03h39m20.24s -35d29m21.2s
(54.83434°, -35.48923°)
EP flux
1.60e-13
± 4.0e-15
erg cm-2 s-1
CLASSX
AGN
(0.795)
Detections
5
| SRCID | 3001283010100008 |
|---|---|
| IAUNAME | 5XMM J033920.2-352921 |
| SC_RA | 03h39m20.24s (54.83434°) |
| SC_DEC | -35d29m21.2s (-35.48923°) |
| RADEC_ERR | 0.08 arcsec |
| LII / BII | 236.7747° / -53.4612° |
| N_CONTRIB | 5 (detections) |
| N_OBS | 17 (observations covering the position) |
| MJD_FIRST | 51916.608 (2001-01-07 14:34:55.000 UTC) |
| MJD_LAST | 57752.928 (2016-12-30 22:15:48.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.60e-13 ± 4.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.05
± 0.01
0.2-0.5 / 0.5-1.0 keV
HR2
-0.03
± 0.01
0.5-1.0 / 1.0-2.0 keV
HR3
-0.39
± 0.01
1.0-2.0 / 2.0-4.5 keV
HR4
-0.35
± 0.03
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -4.5)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 1.3
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
- 993271
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 20.527 | 0.128 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.36e-13 (+1.4e-13 / −1.3e-13) erg cm−2 s−1 |
|---|---|
| NH | 2.03e+19 (+4.0e+19 / −1.2e+19) cm−2 |
| Photon index (Γ) | 1.99 (+2.03 / −1.96) |
| DoF | 1559 |
| p-value | 0.141 |
| Inter-instrument norm. | 1.01 (0.96–1.05) |
| 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.