5XMM J001446.1-302710

5XMM-DR15 stacked source · SRCID 3004234010100118
Position: 00h14m46.16s -30d27m10.6s (3.69234°, -30.45293°)
EP flux
1.77e-14 ± 4.5e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.856)
Detections
2

SRCID 3004234010100118
IAUNAME 5XMM J001446.1-302710
SC_RA 00h14m46.16s (3.69234°)
SC_DEC -30d27m10.6s (-30.45293°)
RADEC_ERR 1.26 arcsec
LII / BII 8.2847° / -81.3091°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52059.831 (2001-05-30 19:57:00.000 UTC)
MJD_LAST 57011.090 (2014-12-20 02:09:28.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.77e-14 ± 4.5e-15 erg cm-2 s-1

Hardness ratios
HR1
0.29 ± 0.18
0.2-0.5 / 0.5-1.0 keV
HR2
-0.74 ± 0.19
0.5-1.0 / 1.0-2.0 keV
HR3
0.29 ± 0.57
1.0-2.0 / 2.0-4.5 keV
HR4
0.88 ± 0.10
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.3) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 1.72

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
22270
Match probability
0.976
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U — —
B — —
V 18.248 0.023
Gaia DR3
Source ID
2320207480091628160
Match probability
0.99
Magnitudes
G=20.82, BP=19.40, RP=17.74
AllWISE
Name
J001446.15-302710.2
Match probability
0.994
BandMagErr
W1 14.323 0.029
W2 13.905 0.037
W3 12.541 0.507
W4 8.736 —
CLASSOPT
Class
Galaxy
Star
0.01
AGN
0.00
Galaxy
0.99

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 8.74e-15 (+1.1e-14 / −6.4e-15) erg cm−2 s−1
NH 6.16e+19 (+2.3e+20 / −1.9e+19) cm−2
Photon index (Γ) 1.27 (+1.55 / −1.09)
DoF 182
p-value 0.184
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

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