5XMM J033832.2-353343
5XMM-DR15 stacked source · SRCID 3001283010100112
Position:
03h38m32.21s -35d33m43.2s
(54.63423°, -35.56199°)
EP flux
1.02e-14
± 1.4e-15
erg cm-2 s-1
CLASSX
AGN
(0.93)
Detections
4
| SRCID | 3001283010100112 |
|---|---|
| IAUNAME | 5XMM J033832.2-353343 |
| SC_RA | 03h38m32.21s (54.63423°) |
| SC_DEC | -35d33m43.2s (-35.56199°) |
| RADEC_ERR | 0.41 arcsec |
| LII / BII | 236.9035° / -53.6223° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 17 (observations covering the position) |
| MJD_FIRST | 52087.772 (2001-06-27 18:31:08.000 UTC) |
| MJD_LAST | 57752.928 (2016-12-30 22:15:48.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.02e-14 ± 1.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.06
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
0.02
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.62
± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.5)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.726
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
- 989886
- Match probability
- 0.991
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.904 | 0.226 |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.02e-14 (+2.5e-14 / −1.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.09e+20 (+4.9e+20 / −2.2e+19) cm−2 |
| Photon index (Γ) | 1.75 (+1.97 / −1.58) |
| DoF | 574 |
| p-value | 0.938 |
| Inter-instrument norm. | 0.76 (0.61–0.93) |
| 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.