5XMM J001619.3-391645

5XMM-DR15 stacked source · SRCID 3002874020100202
Position: 00h16m19.38s -39d16m45.0s (4.08074°, -39.27917°)
EP flux
5.36e-15 ± 1.7e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.776)
Detections
8

SRCID 3002874020100202
IAUNAME 5XMM J001619.3-391645
SC_RA 00h16m19.38s (4.08074°)
SC_DEC -39d16m45.0s (-39.27917°)
RADEC_ERR 0.70 arcsec
LII / BII 331.7623° / -75.8188°
N_CONTRIB 8 (detections)
N_OBS 10 (observations covering the position)
MJD_FIRST 52227.605 (2001-11-14 14:31:49.000 UTC)
MJD_LAST 59561.812 (2021-12-13 19:29:06.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 5.36e-15 ± 1.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.80 ± 0.15
0.2-0.5 / 0.5-1.0 keV
HR2
0.40 ± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.29 ± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.43 ± 0.26
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.0) SUM_FLAG: 0
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 2.89

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
26127
Match probability
0.98
FilterMag (AB)Err
UVW2 18.836 0.056
UVM2 18.673 0.033
UVW1 18.130 0.008
U 17.735 0.013
B 16.523 0.008
V 16.757 0.041
Gaia DR3
Source ID
4997980810165341440
Match probability
0.984
Magnitudes
G=22.01, BP=18.48, RP=17.78
AllWISE
Name
J001619.49-391645.6
Match probability
0.993
BandMagErr
W1 14.273 0.028
W2 14.072 0.040
W3 10.515 0.077
W4 8.126 0.239
CLASSOPT
Class
Galaxy
Star
0.10
AGN
0.15
Galaxy
0.76

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 4.66e-15 (+9.8e-15 / −1.8e-15) erg cm−2 s−1
NH 4.50e+22 (+4.4e+23 / −3.4e+21) cm−2
Photon index (Γ) 1.70 (+2.54 / −1.19)
DoF 292
p-value 0.999
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.