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• W3105987340 abstract "Our aims are to determine flux densities and their photometric accuracy for a set of seventeen stars that range in flux from intermediately bright (<2.5 Jy) to faint (>5 mJy) in the far-infrared (FIR). We also aim to derive signal-to-noise dependence with flux and time, and compare the results with predictions from the Herschel exposure-time calculation tool. The PACS faint star sample has allowed a comprehensive sensitivity assessment of the PACS photometer. Accurate photometry allows us to establish a set of five FIR primary standard candidates, namely alpha Ari, epsilon Lep, omega,Cap, HD41047 and 42Dra, which are 2 -- 20 times fainter than the faintest PACS fiducial standard (gamma Dra) with absolute accuracy of <6%. For three of these primary standard candidates, essential stellar parameters are known, meaning that a dedicated flux model code may be run." @default.
• W3105987340 created "2020-11-23" @default.
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• W3105987340 date "2018-05-01" @default.
• W3105987340 modified "2023-09-27" @default.
• W3105987340 title "Herschel-PACS photometry of faint stars for sensitivity performance assessment and establishment of faint FIR primary photometric standards" @default.
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• W3105987340 doi "https://doi.org/10.1051/0004-6361/201731812" @default.
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