5XMM J005555.4-012127

5XMM-DR15 stacked source · SRCID 3001244010100175
Position: 00h55m55.46s -01d21m27.2s (13.98107°, -1.35756°)
EP flux
6.01e-15 ± 3.2e-15 erg cm-2 s-1
CLASSX
AGN (0.941)
Detections
4

SRCID 3001244010100175
IAUNAME 5XMM J005555.4-012127
SC_RA 00h55m55.46s (13.98107°)
SC_DEC -01d21m27.2s (-1.35756°)
RADEC_ERR 1.01 arcsec
LII / BII 125.5095° / -64.2068°
N_CONTRIB 4 (detections)
N_OBS 4 (observations covering the position)
MJD_FIRST 51923.975 (2001-01-14 23:23:18.000 UTC)
MJD_LAST 57210.407 (2015-07-07 09:46:43.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 6.01e-15 ± 3.2e-15 erg cm-2 s-1

Hardness ratios
HR1
0.15 ± 0.21
0.2-0.5 / 0.5-1.0 keV
HR2
0.19 ± 0.19
0.5-1.0 / 1.0-2.0 keV
HR3
-0.33 ± 0.19
1.0-2.0 / 2.0-4.5 keV
HR4
-0.40 ± 0.46
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.5) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.289

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
335627
Match probability
0.977
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 22.227 0.222
B
V
AllWISE
Name
J005555.37-012126.7
Match probability
0.995
BandMagErr
W1 16.617 0.101
W2 16.771 0.538
W3 12.041
W4 8.640
CLASSOPT
Class
Star
Star
0.97
AGN
0.00
Galaxy
0.03

Photometric (TPZ) 0.6258 (conf 0.71)
Photometric (Le Phare) 0.5274 (conf 0.74)

Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.

Automated spectral fits are not yet available for this source. Interactive fitting on individual observations will be available from the contributing detections table soon.

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

The per-observation light curve is shown in the X-ray properties section above.