Result for 0534888234C9188898CA5E224D1422776AA3C4D1

Query result

Key Value
FileNamehawki_step_detect_obj.la
FileSize1033
MD52390B5FB1E61EA2542AABFD1F1828A49
RDS:package_id182052
SHA-10534888234C9188898CA5E224D1422776AA3C4D1
SHA-2564DFB6D98D1623759F2444B4FFFAC614927F5A53E4B12A6832032649DB38ACF11
SSDEEP24:PeSGWWJU2icBxIY+Ahmfvi45vD2NGDe5/oxn:lGWWJUzcBxIY1hmfKqLcox
TLSHT1E911C03FD3DE713AAFD41A4596CF303E42C9847907352E5063C795DB224B81921A7E2B
insert-timestamp1679423153.2980564
sourceRDS.db
hashlookup:parent-total2
hashlookup:trust60

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Parents (Total: 2)

The searched file hash is included in 2 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileName13697
FileSize222964
MD5974C59296FB3D0C20D19308DD77F09D1
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.21+dfsg-1build1
RDS:package_id182052
SHA-14E0EAFAA7F8F95F0090AB88C11D17F77A12BCCFE
SHA-256266882D5AE449DE6BE617369A30F14C4281B4D1A395A3C0695B24BA38DAC0ADE
insert-timestamp1679408379.314181
sourceRDS.db
Key Value
FileSize260978
MD55F77ED0FB77CB9283D78B6CC956FBAC7
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-13D00E429E99C1B8D428D87C587056182BBA9003D
SHA-256C39FAE0786F62BF2CDED8B18E826ADF7C549FC82B84F7602C5DC53034AF832DA