Result for 25878FD3DB25136E0225EEF51C94BA57BD421ACC

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_step_apply_dist.so
FileSize14488
MD5904065B2DD58F4E393A76A65E7E15C59
SHA-125878FD3DB25136E0225EEF51C94BA57BD421ACC
SHA-2569BFDBC1F0E2AA953F6B5CE1B20903A7B3D811F3A21FC8A01D87000B72007B2B2
SSDEEP192:niXgds8+ooXzv0GnGxX3Qgc2EwjHtltlH/BcQffltUWucKBdIfHX7IJ+xAn30piM:nmgdKooXzj6ggTjNltlfBD3lt3iBRnp
TLSHT18752864BBB51C971C3C225B05047072DA2714835E67FDB827D8D2288EF65AECD9233AE
hashlookup:parent-total1
hashlookup:trust55

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Parents (Total: 1)

The searched file hash is included in 1 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize524536
MD53FC8B3C34A65DF11F4044DD0DED779E6
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.4.9+dfsg-1
SHA-170C4037CF07C67D800F6A6916A4412B35AFD6356
SHA-256A4615C80DE8B1365075BBBC5B4DEDF45435016BCDC59F1DE203D83F86568C5FA