5XMM J000235.4-300702
5XMM-DR15 stacked source · SRCID 3004175010100026
Position:
00h02m35.49s -30d07m02.4s
(0.64788°, -30.11732°)
EP flux
2.89e-14
± 2.7e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
1
| SRCID | 3004175010100026 |
|---|---|
| IAUNAME | 5XMM J000235.4-300702 |
| SC_RA | 00h02m35.49s (0.64788°) |
| SC_DEC | -30d07m02.4s (-30.11732°) |
| RADEC_ERR | 0.63 arcsec |
| LII / BII | 14.4741° / -78.8785° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52440.823 (2002-06-15 19:44:59.000 UTC) |
| MJD_LAST | 52441.421 (2002-06-16 10:06:17.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.89e-14 ± 2.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.48
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.60
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.95
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
0.43
± 0.58
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.9)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 1.58
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
- 8109
- Match probability
- 0.984
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 14.413 | 0.002 |
| B | — | — |
| V | 12.439 | 0.001 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.90e-14 (+3.2e-14 / −2.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 8.93e+20 (+1.2e+21 / −6.1e+20) cm−2 |
| Photon index (Γ) | 2.91 (+2.97 / −2.78) |
| DoF | 391 |
| p-value | 0.01 |
| Inter-instrument norm. | 1.34 (1.12–1.60) |
| 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.