5XMM J000239.3-300804
5XMM-DR15 stacked source · SRCID 3004175010100007
Position:
00h02m39.36s -30d08m04.2s
(0.66400°, -30.13449°)
EP flux
5.45e-14
± 5.5e-15
erg cm-2 s-1
CLASSX
CV
(0.533)
Detections
1
| SRCID | 3004175010100007 |
|---|---|
| IAUNAME | 5XMM J000239.3-300804 |
| SC_RA | 00h02m39.36s (0.66400°) |
| SC_DEC | -30d08m04.2s (-30.13449°) |
| RADEC_ERR | 0.29 arcsec |
| LII / BII | 14.3714° / -78.8884° |
| 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): 5.45e-14 ± 5.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.48
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.22
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.62
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.89
± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.5)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
CV
CLASSX outlier: 3.86
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
- 8231
- Match probability
- 0.993
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.109 | 0.117 |
| B | — | — |
| V | 18.788 | 0.049 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 4.98e-14 (+5.3e-14 / −4.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.83e+21 (+2.0e+21 / −1.6e+21) cm−2 |
| Photon index (Γ) | 2.93 (+2.98 / −2.84) |
| DoF | 320 |
| p-value | 0.002 |
| Quality flag | 5 |
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.