5XMM J014154.5-675041
5XMM-DR15 stacked source · SRCID 3003214040100025
Position:
01h41m54.54s -67d50m41.2s
(25.47723°, -67.84478°)
EP flux
1.74e-14
± 4.9e-15
erg cm-2 s-1
CLASSX
Extragal_XRB
(0.636)
Detections
2
| SRCID | 3003214040100025 |
|---|---|
| IAUNAME | 5XMM J014154.5-675041 |
| SC_RA | 01h41m54.54s (25.47723°) |
| SC_DEC | -67d50m41.2s (-67.84478°) |
| RADEC_ERR | 0.96 arcsec |
| LII / BII | 295.7793° / -48.5766° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52032.413 (2001-05-03 09:54:03.000 UTC) |
| MJD_LAST | 52625.252 (2002-12-17 06:03:10.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.74e-14 ± 4.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.59
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.26
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.66
± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
0.35
± 0.30
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 2.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Extragal_XRB
CLASSX outlier: 5.71
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
- 678025
- Match probability
- 0.965
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 19.653 | 0.065 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.16e-14 (+1.5e-14 / −9.4e-15) erg cm−2 s−1 |
|---|---|
| NH | 3.62e+20 (+1.3e+21 / −3.4e+19) cm−2 |
| Photon index (Γ) | 2.33 (+2.77 / −2.02) |
| DoF | 94 |
| p-value | 0.456 |
| 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.