5XMM J000251.5-295449
5XMM-DR15 stacked source · SRCID 3004175010100064
Position:
00h02m51.50s -29d54m49.4s
(0.71457°, -29.91373°)
EP flux
8.64e-15
± 2.0e-15
erg cm-2 s-1
CLASSX
Star
(0.997)
Detections
1
| SRCID | 3004175010100064 |
|---|---|
| IAUNAME | 5XMM J000251.5-295449 |
| SC_RA | 00h02m51.50s (0.71457°) |
| SC_DEC | -29d54m49.4s (-29.91373°) |
| RADEC_ERR | 0.75 arcsec |
| LII / BII | 15.4475° / -78.9778° |
| 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): 8.64e-15 ± 2.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.50
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.74
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-1.00
± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
1.00
± 0.49
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 2.55
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
- 8628
- Match probability
- 0.991
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 20.762 | 0.092 |
| B | — | — |
| V | 16.991 | 0.016 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.78e-15 (+8.3e-15 / −5.4e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.19e+20 (+5.9e+20 / −2.4e+19) cm−2 |
| Photon index (Γ) | 2.78 (+2.94 / −2.52) |
| DoF | 42 |
| p-value | 0.462 |
| 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.