5XMM J004219.2-091653
| SRCID | 3006514010100035 |
|---|---|
| IAUNAME | 5XMM J004219.2-091653 |
| SC_RA | 00h42m19.20s (10.58000°) |
| SC_DEC | -09d16m53.1s (-9.28143°) |
| RADEC_ERR | 0.22 arcsec |
| LII / BII | 115.6248° / -72.0237° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 8 (observations covering the position) |
| MJD_FIRST | 52281.557 (2002-01-07 13:21:35.000 UTC) |
| MJD_LAST | 56462.381 (2013-06-19 09:08:46.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.29e-14 ± 2.5e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.421
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.
- OM Source ID
- 130608
- Match probability
- 0.988
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 20.951 | 0.087 |
| UVW1 | 20.967 | 0.072 |
| U | 20.654 | 0.081 |
| B | 20.680 | 0.079 |
| V | 20.440 | 0.148 |
- Source ID
- 2426012414585316224
- Match probability
- 0.996
- Parallax
- -0.653 ± 1.049 mas
- Proper motion
- (-0.01, -0.02) mas/yr
- Magnitudes
- G=20.45, BP=20.55, RP=20.03
- Class
- QSO
| Photometric (TPZ) | 0.3259 (conf 0.50) |
|---|---|
| Photometric (Le Phare) | 0.7941 (conf 0.36) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 4.27e-14 (+4.6e-14 / −3.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.04e+19 (+1.7e+20 / −1.7e+19) cm−2 |
| Photon index (Γ) | 2.27 (+2.38 / −2.17) |
| DoF | 310 |
| p-value | 0.868 |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 7.100 (approximate flux variability amplitude) |
|---|
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.