Result for 02BE0D561F956B99571C6625E7062659B2AF4251

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-1.8.21/hawki_step_photom_2mass.so
FileSize22736
MD57BD45CD4C0AB513606CD8DDEEA410762
SHA-102BE0D561F956B99571C6625E7062659B2AF4251
SHA-256C3DF3F0C540EA2BC1A1C1F5588C2642EE34D97B158EA447F397C095FE65DFAB4
SSDEEP384:A1Ol84Aw9GPp+J2hlDxEzRx8ipjbiKsZ5U9JeF70kwyo/w57Um/Ls6sdrhPAr9:uOl84Aw0kJ2Dmb/DSa/e91wyoOYBt
TLSHT1F3A2F8DFE5027B67C9C02F38549F8B4A621347F0929C7713482D8D346A15ABF8E66E4E
hashlookup:parent-total1
hashlookup:trust55

Network graph view

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
FileSize228074
MD5CE29F2691A6DA88FF83D73C679596827
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
PackageVersion1.8.21+dfsg-1
SHA-1FFAB13A4EB060F369871AD9885635F1D6BDEAB73
SHA-2568D0D52E213F4C1B1787D5035FF57338A5A51EE8C5F408362A01B3492A2590DA5