5XMM J093900.9+355003
5XMM-DR15 stacked source · SRCID 3002174010100067
Position:
09h39m00.94s +35d50m03.3s
(144.75392°, 35.83426°)
EP flux
1.07e-14
± 1.1e-14
erg cm-2 s-1
CLASSX
AGN
(0.866)
Detections
2
| SRCID | 3002174010100067 |
|---|---|
| IAUNAME | 5XMM J093900.9+355003 |
| SC_RA | 09h39m00.94s (144.75392°) |
| SC_DEC | +35d50m03.3s (35.83426°) |
| RADEC_ERR | 1.62 arcsec |
| LII / BII | 188.4976° / 48.4830° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52209.321 (2001-10-27 07:42:42.000 UTC) |
| MJD_LAST | 58796.982 (2019-11-09 23:33:27.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.07e-14 ± 1.1e-14 erg cm-2 s-1
Hardness ratios
HR1
0.09
± 0.24
0.2-0.5 / 0.5-1.0 keV
HR2
-0.06
± 0.27
0.5-1.0 / 1.0-2.0 keV
HR3
-0.86
± 0.31
1.0-2.0 / 2.0-4.5 keV
HR4
0.81
± 0.56
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.2)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.0122
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
- 2756977
- Match probability
- 0.501
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.604 | 0.097 |
| U | — | — |
| B | — | — |
| V | 16.673 | 0.024 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 5.96e-15 (+8.7e-15 / −4.3e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.11e+20 (+5.3e+20 / −2.3e+19) cm−2 |
| Photon index (Γ) | 2.61 (+2.87 / −2.25) |
| DoF | 69 |
| p-value | 0.728 |
| 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.