5XMM J033830.7-354220

5XMM-DR15 stacked source · SRCID 3001283010100507
Position: 03h38m30.71s -35d42m20.3s (54.62796°, -35.70563°)
EP flux
2.14e-15 ± 1.7e-15 erg cm-2 s-1
CLASSX
AGN (0.774)
Detections
4

SRCID 3001283010100507
IAUNAME 5XMM J033830.7-354220
SC_RA 03h38m30.71s (54.62796°)
SC_DEC -35d42m20.3s (-35.70563°)
RADEC_ERR 0.87 arcsec
LII / BII 237.1458° / -53.6235°
N_CONTRIB 4 (detections)
N_OBS 17 (observations covering the position)
MJD_FIRST 52087.772 (2001-06-27 18:31:08.000 UTC)
MJD_LAST 57752.928 (2016-12-30 22:15:48.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.14e-15 ± 1.7e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.73 ± 0.20
0.2-0.5 / 0.5-1.0 keV
HR2
0.12 ± 0.52
0.5-1.0 / 1.0-2.0 keV
HR3
-0.90 ± 0.85
1.0-2.0 / 2.0-4.5 keV
HR4
0.96 ± 1.15
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.8) SUM_FLAG: 2
Long-term lightcurve

AGN

CLASSX outlier: 0.692

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
989778
Match probability
0.886
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.767 0.127
U
B
V 21.294 0.274
AllWISE
Name
J033830.69-354222.6
Match probability
0.995
BandMagErr
W1 17.199 0.087
W2 16.960 0.259
W3 12.710
W4 9.527
CLASSOPT
Class
Galaxy
Star
0.19
AGN
0.00
Galaxy
0.81

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 1.52e-15 (+2.5e-15 / −1.1e-15) erg cm−2 s−1
NH 9.68e+19 (+7.6e+20 / −2.0e+19) cm−2
Photon index (Γ) 2.20 (+2.62 / −1.62)
DoF 248
p-value 0.87
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.