5XMM J003401.6-053752
5XMM-DR15 stacked source · SRCID 3003174010100020
Position:
00h34m01.64s -05d37m52.6s
(8.50682°, -5.63128°)
EP flux
1.77e-14
± 8.9e-15
erg cm-2 s-1
CLASSX
Star
(0.994)
Detections
1
| SRCID | 3003174010100020 |
|---|---|
| IAUNAME | 5XMM J003401.6-053752 |
| SC_RA | 00h34m01.64s (8.50682°) |
| SC_DEC | -05d37m52.6s (-5.63128°) |
| RADEC_ERR | 1.18 arcsec |
| LII / BII | 111.2453° / -68.1071° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52444.358 (2002-06-19 08:35:54.000 UTC) |
| MJD_LAST | 52444.769 (2002-06-19 18:27:04.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.77e-14 ± 8.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.55
± 0.15
0.2-0.5 / 0.5-1.0 keV
HR2
-0.54
± 0.16
0.5-1.0 / 1.0-2.0 keV
HR3
-0.93
± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
0.58
± 0.39
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.06
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
- 70313
- Match probability
- 0.993
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.403 | 0.198 |
| U | 20.447 | 0.111 |
| B | 18.178 | 0.049 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.42e-14 (+1.7e-14 / −1.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.14e+19 (+2.0e+20 / −1.7e+19) cm−2 |
| Photon index (Γ) | 2.85 (+2.96 / −2.63) |
| DoF | 62 |
| p-value | 0.132 |
| 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.