5XMM J033809.2-353507

5XMM-DR15 stacked source · SRCID 3001283010100670
Position: 03h38m09.29s -35d35m07.4s (54.53872°, -35.58539°)
EP flux
9.19e-15 ± 3.0e-15 erg cm-2 s-1
CLASSX
AGN (0.913)
Detections
5

SRCID 3001283010100670
IAUNAME 5XMM J033809.2-353507
SC_RA 03h38m09.29s (54.53872°)
SC_DEC -35d35m07.4s (-35.58539°)
RADEC_ERR 0.99 arcsec
LII / BII 236.9464° / -53.6994°
N_CONTRIB 5 (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): 9.19e-15 ± 3.0e-15 erg cm-2 s-1

Hardness ratios
HR1
0.03 ± 0.24
0.2-0.5 / 0.5-1.0 keV
HR2
0.55 ± 0.16
0.5-1.0 / 1.0-2.0 keV
HR3
-0.75 ± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
0.28 ± 0.26
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.4) SUM_FLAG: 2
Long-term lightcurve

AGN

CLASSX outlier: 0.824

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
988404
Match probability
0.987
FilterMag (AB)Err
UVW2
UVM2
UVW1
U
B
V 20.522 0.078
Gaia DR3
Source ID
4860290957587302528
Match probability
0.993
Parallax
0.365 ± 1.362 mas
Proper motion
(0.14, 0.26) mas/yr
Magnitudes
G=20.88, BP=20.91, RP=19.62
AllWISE
Name
J033809.22-353506.6
Match probability
0.995
BandMagErr
W1 17.339 0.092
W2 17.847
W3 13.269
W4 9.416
CLASSOPT
Class
Star
Star
0.98
AGN
0.02
Galaxy
0.00

No redshift estimate available for this source.

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.