5XMM J001507.6-391324

5XMM-DR15 stacked source · SRCID 3002874010100235
Position: 00h15m07.62s -39d13m24.6s (3.78173°, -39.22350°)
EP flux
1.25e-15 ± 5.8e-16 erg cm-2 s-1
CLASSX
Star (0.606)
Detections
10

SRCID 3002874010100235
IAUNAME 5XMM J001507.6-391324
SC_RA 00h15m07.62s (3.78173°)
SC_DEC -39d13m24.6s (-39.22350°)
RADEC_ERR 1.26 arcsec
LII / BII 332.6691° / -75.7347°
N_CONTRIB 10 (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): 1.25e-15 ± 5.8e-16 erg cm-2 s-1

Hardness ratios
HR1
0.69 ± 2.22
0.2-0.5 / 0.5-1.0 keV
HR2
0.82 ± 0.48
0.5-1.0 / 1.0-2.0 keV
HR3
-0.23 ± 0.34
1.0-2.0 / 2.0-4.5 keV
HR4
0.34 ± 0.33
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.8) SUM_FLAG: 1
Long-term lightcurve

Star

CLASSX outlier: 4.67

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
23237
Match probability
0.71
FilterMag (AB)Err
UVW2
UVM2
UVW1 20.594 0.091
U
B
V
Gaia DR3
Source ID
4997972598186504320
Match probability
0.967
Parallax
-1.398 ± 1.366 mas
Proper motion
(0.20, 0.59) mas/yr
Magnitudes
G=20.49, BP=20.76, RP=20.22
AllWISE
Name
J001507.73-391321.8
Match probability
0.993
BandMagErr
W1 14.549 0.035
W2 16.121 0.226
W3 12.344
W4 8.474
CLASSOPT
Class
QSO
Star
0.03
AGN
0.85
Galaxy
0.12

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.