'A New Setup for Ground-based Measurements of Solar Activity at 10 pm'(PASP, 118, 1558 [2006])

摘要

The mid-IR (10 μm) temperature scale adopted in the article was inadvertently derived from a calibration made with thecamera nearly saturated. It provided a temperature input versus reading temperature ratio of about 36. New calibrations were repeatedseveral times in the following campaigns, one year later, showing a temperature input versus reading temperature ratio of 2. Thereforethe published mid-IR burst time profile and derived fluxes should be divided by a factor of 18. Center for Radio Astronomy and Astrophysics (CRAAM), Mackenzie Pres-byterian University, Sao Paulo, Brazil; armame@gmail.com. Center for Semiconductor Components, Campinas State University, Campi-nas, Brazil. Physics Institute Gleb Wataghin, Campinas State University, Campinas,Brazil. Bernard Lyot Observatory, Campinas, Brazil. 5E1 Leoncito Astronomical Complex, San Juan, Argentina. 1296