5XMM J030537.3-775715
5XMM-DR15 stacked source · SRCID 3004234040100042
Position:
03h05m37.34s -77d57m15.7s
(46.40559°, -77.95437°)
EP flux
2.01e-14
± 2.5e-15
erg cm-2 s-1
CLASSX
AGN
(0.76)
Detections
5
| SRCID | 3004234040100042 |
|---|---|
| IAUNAME | 5XMM J030537.3-775715 |
| SC_RA | 03h05m37.34s (46.40559°) |
| SC_DEC | -77d57m15.7s (-77.95437°) |
| RADEC_ERR | 0.49 arcsec |
| LII / BII | 294.6378° / -36.9230° |
| N_CONTRIB | 5 (detections) |
| N_OBS | 5 (observations covering the position) |
| MJD_FIRST | 52032.765 (2001-05-03 18:21:36.000 UTC) |
| MJD_LAST | 59685.458 (2022-04-16 11:00:04.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.01e-14 ± 2.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.77
± 0.24
0.2-0.5 / 0.5-1.0 keV
HR2
0.69
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.09
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.22
± 0.10
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.3)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.412
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
- 908532
- Match probability
- 0.985
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.949 | 0.194 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.82e-14 (+2.2e-14 / −1.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 9.33e+20 (+1.9e+21 / −1.6e+20) cm−2 |
| Photon index (Γ) | 1.41 (+1.70 / −1.18) |
| DoF | 767 |
| p-value | 0.282 |
| Inter-instrument norm. | 0.72 (0.58–0.90) |
| 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.