Evidence for X-ray emission from the type Ia SN PTF11kly (Erratum)

Details Evidence for X-ray emission from the type Ia SN PTF11kly (Erratum) Evidence for X-ray emission from the type Ia SN PTF11kly (Erratum)

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3593....1f&link_type=abstract

The Astronomer's Telegram, #3593

Astronomy and Astrophysics

Astronomy

1

Radio, Optical, Ultra-Violet, X-Ray, Supernovae, Transient

Scientific paper

Due to an error in transcription, the X-ray count rate, flux, and luminosity estimates quoted in ATEL #3592 were in error by a factor of ten. The second paragraph should correctly read: The inferred count rate of ~0.22 cts ksec^-1 falls below the quoted upper limit of 4 cts ksec^-1 from ATEL #3584 and is not in conflict with that report. Assuming a photon index alpha=2 spectrum, the source X-ray flux would be ~7e-15 erg cm-2 s-1 (0.3-10 keV), and the X-ray luminosity at M101 would be ~4e+37 erg s-1 (0.3-10 keV).

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