The missing light of the Hubble Ultra Deep Field

Alejandro Borlaff; Ignacio Trujillo; Javier Román; John E. Beckman; M. Carmen Eliche-Moral; Raúl Infante-Sáinz; Alejandro Lumbreras-Calle; Rodrigo Takuro Sato Martín de Almagro; Carlos Gómez-Guijarro; María Cebrián; Antonio Dorta; Nicolás Cardiel; Mohammad Akhlaghi; Cristina Martínez-Lombilla

doi:10.1051/0004-6361/201834312

Free Access

Fig. 12.

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Comparison of the ABYSS mosaics of the HUDF WFC3 IR and the previous releases. Each plot represents the intensity difference between our version of the mosaics (ABYSS) and the reference versions (left panels: XDF, right panels: HUDF12), for the F105W filter (top panels) and the F125W filter (bottom panels). See the colour bar for reference.

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