Swift observations of SN2011ei (PSN J20342262-3158236)
ATel #3528; R. Margutti (Harvard Univ.), P. Brown (U. of Utah), A. M. Soderberg (Harvard Univ.) P. Roming (SwRI)
on 3 Aug 2011; 15:54 UT
Credential Certification: Raffaella Margutti (email@example.com)
Subjects: Optical, Ultra-Violet, X-ray, Supernovae
The spectral properties of 2011ei (PSN J20342262-3158236) have been recently
demonstrated to show a good match to the energetic type-IIb 'hypernova' 2003bg
approximately 7 days before maximum light (Milisavljevic, ATel #3526).
A Swift-ToO was executed to observe the field of 2011ei
starting from 2011-08-03T04:47:14 UT. No X-ray source
is detected at the optical position of the transient
(RA=20:34:22.62 dec=-31:58:23.6) with a 3 sigma upper limit of 4.6d-3 c/s
in the 0.3-10 keV energy band (total exposure= 9.6 ks). The Galactic neutral
hydrogen column density in the direction of the event is 4.76d20 1/cm2
(Kalberla et al., 2005).
Assuming a spectral photon index ~2, this translates
into an absorbed flux of ~2.3d-13 erg/s/cm2. This implies that 2011ei is
intrinsically fainter than the recently detected type IIb SN2011dh
at comparable epoch (Soderberg et al., ArXiv:1107.1876 ).
Contemporary Swift-UVOT observations have been obtained in the 6 optical/UV
filters. A source is clearly detected at the transient position in the
U, B and V band.
Including possible contamination from the host galaxy, we measure the following
preliminary magnitudes (UVOT photometric system Breeveld et al. 2011, arXiv:1102.4717):
filter MJD Mag err
U 5776.81 16.66 0.10
B 5776.81 17.54 0.10
V 5776.82 17.27 0.10
The source is seen faintly in the uvw1 filter but not clearly in the
uvm2 or uvw2 filters. Reliable magnitudes/limits in the UV would require
subtraction of the underlying galaxy.
The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) =0.059 in the direction of the transient.
(Schlegel et al. 1998).
We thank the Swift team for scheduling these ToO observations.