Result for 347F5F797198174D9ADB937A86A87751F9847C0D

Query result

Key Value
FileName./usr/share/cpl-plugins/hawki-2.4.9/gasgano/config/HAWKI.prefs
FileSize3952
MD5E6C12E4443C2335BB3BBA9A7153906F4
SHA-1347F5F797198174D9ADB937A86A87751F9847C0D
SHA-256FEC415E6766F8DA1AC433A875886C01427AD67085759BB628FDD0F97A147F2E9
SSDEEP48:gYe25Zl3dZIoIH5s1QZKqDiNqx6b9JMi8XPJ1DrEoZu+PhfPhTAfmEVJalLRUPXv:n75VZZI8QZmsw7R8XcOTkK3Y7
TLSHT14C81FF2D631F0D6497765AC9171E146E4DC8C8F96265AB853499A8FCC80F3AEC033FE2
hashlookup:parent-total9
hashlookup:trust95

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Parents (Total: 9)

The searched file hash is included in 9 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize451748
MD5071B9F4695EF80D6D86B48ECB848BDB1
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-12EFAE4DCB62A49CB19F7510008CFF9C14342BE11
SHA-256ABAE21EFC2A432D5D37BD2D33604B5CE713A35277F7F34E80A7E278641E8009B
Key Value
FileSize525508
MD502A40EB100388240DB4D5D6169497C90
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-11DF42B5AAC2B9A9BD2D43985F3D8ABB2D7B93FBB
SHA-25654DC6921752833B0AD602101C2BD1ADE309304A73249C9EFE3E22121EB856F01
Key Value
FileSize489816
MD50DC386B9AA2A31F951B2CAB6994240A4
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-1174D5C4F5AF18807F53EFF58FA4460491B0A01A0
SHA-2561A2BE31E56411C85A56DFA78B4D7E21032BB44C3A3A3C03F2A8F1F1DD66465F1
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
Key Value
FileSize453352
MD55CFC0CB5C37652E14DA39B16073327E6
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-109AD28C108CC2A32C4F9E9E6E17CB27DA90FFD5E
SHA-2567A78D83C1E6E73EB9D53CA7D68B3C5EB49076AFE08652C402C0E2888B970DE64
Key Value
FileSize448916
MD515510D708B30FD3447AB413D215ADBF9
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-1617C0F0EC2D7EA25558AFB56BCCB07552925D079
SHA-2569202A8FDCCDB13C2F3ACC2DC6A1BDFA123AD464F752FF6FE14DB8FC365CA9AE6
Key Value
FileSize446980
MD516EFB69819EAF8E09B64CBD57CC67A9B
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-1BAF855C0E5F8829D60769AF9482EFE8ED23EFB36
SHA-2560E43A15CEC1735CDE3AE4C7FF1A00C540392D2A763450F033F2AB8EAEB957702
Key Value
FileSize432820
MD5C12CBBEF48D8105D146F3F56E4FC6A80
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-1E41BD0569D8F9C390A871D226FEBCF087EAA5725
SHA-2561645C1BA99874DEA41DB29C0692F68499585F6E8E7C1FA36686DA058B91EFAFC
Key Value
FileSize447560
MD5313F0A8BE77EE12C7AF31C26CE90DC22
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-13807DF06BE1E959160FCB49D785AAEE6751E71BE
SHA-25636FAFBF666EB029A87DADFC2A4503881FB8C4DF4DA5FAE8B9768C2EE810AC74C