5XMM J021714.3-735947
5XMM-DR15 stacked source · SRCID 3004915010100004
Position:
02h17m14.30s -73d59m47.7s
(34.30957°, -73.99660°)
EP flux
2.03e-13
± 9.5e-15
erg cm-2 s-1
CLASSX
AGN
(0.817)
Detections
7
| SRCID | 3004915010100004 |
|---|---|
| IAUNAME | 5XMM J021714.3-735947 |
| SC_RA | 02h17m14.30s (34.30957°) |
| SC_DEC | -73d59m47.7s (-73.99660°) |
| RADEC_ERR | 0.13 arcsec |
| LII / BII | 295.1580° / -41.8115° |
| N_CONTRIB | 7 (detections) |
| N_OBS | 9 (observations covering the position) |
| MJD_FIRST | 51730.634 (2000-07-05 15:13:30.000 UTC) |
| MJD_LAST | 53386.433 (2005-01-16 10:23:46.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.03e-13 ± 9.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.38
± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.33
± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.33
± 0.02
1.0-2.0 / 2.0-4.5 keV
HR4
-0.37
± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -4.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.549
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
- 763289
- Match probability
- 0.993
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 21.515 | 0.261 |
| UVM2 | — | — |
| UVW1 | 21.197 | 0.068 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.46e-13 (+3.7e-13 / −3.3e-13) erg cm−2 s−1 |
|---|---|
| NH | 6.46e+20 (+8.5e+20 / −4.4e+20) cm−2 |
| Photon index (Γ) | 1.77 (+1.87 / −1.68) |
| DoF | 874 |
| p-value | 0.916 |
| Inter-instrument norm. | 1.07 (1.00–1.14) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 5.900 (approximate flux variability amplitude) |
|---|
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.