5XMM J174804.7-281618

5XMM-DR15 stacked source · SRCID 3003054010116185
Position: 17h48m04.77s -28d16m18.7s (267.01990°, -28.27186°)
EP flux
7.13e-15 ± 1.6e-15 erg cm-2 s-1
CLASSX
Extragal_XRB (0.325)
Detections
15

SRCID 3003054010116185
IAUNAME 5XMM J174804.7-281618
SC_RA 17h48m04.77s (267.01990°)
SC_DEC -28d16m18.7s (-28.27186°)
RADEC_ERR 1.85 arcsec
LII / BII 0.8480° / -0.1168°
N_CONTRIB 15 (detections)
N_OBS 308 (observations covering the position)
MJD_FIRST 51802.795 (2000-09-15 19:04:46.000 UTC)
MJD_LAST 59127.048 (2020-10-05 01:09:24.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 7.13e-15 ± 1.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.27 ± 4.65
0.2-0.5 / 0.5-1.0 keV
HR2
0.91 ± 0.41
0.5-1.0 / 1.0-2.0 keV
HR3
0.57 ± 0.22
1.0-2.0 / 2.0-4.5 keV
HR4
0.28 ± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.8) SUM_FLAG: 1
Long-term lightcurve

Extragal_XRB

CLASSX outlier: 6.25

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
4893888
Match probability
0.92
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.343 0.125
U
B
V
Gaia DR3
Source ID
4057626750388748288
Match probability
0.681
Parallax
0.845 ± 0.205 mas
Proper motion
(1.07, 0.03) mas/yr
Magnitudes
G=18.30, BP=19.86, RP=17.13
Distance
502 pc
CLASSOPT
Class
Star
Star
1.00
AGN
0.00
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.