5XMM J030120.9-775844
5XMM-DR15 stacked source · SRCID 3004234040100048
Position:
03h01m20.98s -77d58m44.3s
(45.33743°, -77.97898°)
EP flux
2.58e-14
± 7.0e-15
erg cm-2 s-1
CLASSX
AGN
(0.929)
Detections
5
| SRCID | 3004234040100048 |
|---|---|
| IAUNAME | 5XMM J030120.9-775844 |
| SC_RA | 03h01m20.98s (45.33743°) |
| SC_DEC | -77d58m44.3s (-77.97898°) |
| RADEC_ERR | 0.54 arcsec |
| LII / BII | 294.8780° / -37.0386° |
| 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): 2.58e-14 ± 7.0e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.02
± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.51
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.41
± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.55
± 0.26
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.5)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.467
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
- 905501
- Match probability
- 0.973
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 19.893 | 0.103 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.70e-14 (+4.7e-14 / −3.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 8.19e+19 (+3.4e+20 / −2.0e+19) cm−2 |
| Photon index (Γ) | 1.78 (+2.00 / −1.59) |
| DoF | 224 |
| p-value | 0.58 |
| Inter-instrument norm. | 0.64 (0.54–0.79) |
| 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.