Discovery of a fast X-ray transient in the Chandra Deep Field-South survey
ATel #6541; Bin Luo (Penn State), Niel Brandt (Penn State), Franz Bauer (Pontificia Universidad CatÃ³lica de Chile)
on 5 Oct 2014; 02:10 UT
Distributed as an Instant Email Notice Transients
Credential Certification: Bin Luo (firstname.lastname@example.org)
Subjects: X-ray, Transient
We discovered a fast X-ray transient in one of the new Chandra Deep
Field-South (CDF-S) observations (obsid 16454, ~50 ks exposure). The
J2000 source position is RA=53.161661 and DEC=-27.859467, with a
positional uncertainty ~0.5". It appears as a new X-ray source with
~110 counts in the 0.5-8 keV band, and it was not present in the
previous ~4.5 Ms of exposure with Chandra. Fitting the X-ray spectrum
with a simple power law yields Gamma=1.43+/-0.28.
Inspection of the Chandra light curve indicates that the bulk of
detected photons arrived over a time span of ~1 ks. The rise
time is ~70-160 s, and the decay time appears exponential with net rate
going as (t/100.)^(-1.6) (e-folding time ~100 s). No further detection
of the source is found. The transient occurred on 2014 Oct 01
07:04:37 UT. It is unlikely due to any previously known Chandra
instrumental effect based on several tests performed.
The source is ~4' away from the CDF-S aim point, and it is within the
3D-HST coverage. The closest 3D-HST counterpart is ~0.4" away, with AB
magnitudes R~30, z~28, and Ks~26, and a low-quality photometric
redshift of ~0.53 (Skelton et al. 2014). There is another possible
counterpart ~0.6" away, which is even fainter. The next closet 3D-HST
source is 1.9" away. At a redshift of 0.53, the peak X-ray luminosity
is ~1.3E45 erg/s (count rate ~0.1 cts/s).
We searched through the ESO archive for additional optical constraints.
A VIMOS pre-image (PI Pentericci, program ID 194.A-2003A) overlaps
with the position of the X-ray flare. The 550s R-band image was
obtained at 2014 Oct 01 08:20:09.6 UT with 0.66" seeing and at 1.03
airmass. After aligning the X-ray and R-band images to 0.1", no object
is detected at the location of the X-ray flare, with an approximate
limit of R>~25.5 (3sigma, 0.5" radius aperture).
The nature of this transient remains unclear. Observations of any
supernova or afterglow emission in optical, radio, etc. would be