Parents (Total: 11)

The searched file hash is included in 11 parent files which include package known and seen by metalookup. A sample is included below:

Key	Value
FileSize	442062
MD5	E779873E6D359675CEDBC17AC57E9320
PackageDescription	ESO 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).
PackageMaintainer	Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.2.0+dfsg-1+b1
SHA-1	3C5CD869CACE89525DD780CA8081A8C6802AEDE3
SHA-256	EB202A58AA0E86581745FF06F55E29A9F37826AF733B571458392DCD61AAD19D

Key	Value
FileSize	438120
MD5	F14E612CDAC168854029D313E0FF1BC8
PackageDescription	ESO 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.2.0+dfsg-1build1
SHA-1	25C318905E702AE7B4F69DF645F83D37B0452B9E
SHA-256	F63148016DA1AE247452781483A4BC1347D39621941BC5D9B51B2F5CE00EB9CD

Key	Value
FileSize	441700
MD5	90A8B68481078A3E72CFC40CE28E0F8A
PackageDescription	ESO 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.2.0+dfsg-1build1
SHA-1	9C4376EABFD6588229052226F6F1AE0C1D40B920
SHA-256	613F99F73A40908D157F4AE391FF2BBCE5911C50EC90D7A17D61089B608EA276

Key	Value
FileSize	510596
MD5	C3A8598255D089A56D7555D54E939763
PackageDescription	ESO 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).
PackageMaintainer	Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.2.0+dfsg-1+b1
SHA-1	26EC7B533367155E98EE1068CED505920F9DD102
SHA-256	AE2F773418C6EAFE9CB8230F334D27A87C21AD03F9D91B92A96859FA35E55D2F

Key	Value
FileSize	339148
MD5	C58D5E032A626182ED9262A1DA69BDEA
PackageDescription	ESO 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.2.0+dfsg-1build1
SHA-1	A3CF036AA00324958F4AD1F5F560ACB7C87F5FAE
SHA-256	06CC17F274E65C368C62414C15C314154E9EE262D76EEC3AA890F81158595536

Key	Value
FileSize	363444
MD5	008665630BEAB04AA3E699DF53464A28
PackageDescription	ESO 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.2.0+dfsg-1build1
SHA-1	016893D9A8DABB8BCACD581CEE5327857904F01D
SHA-256	C671E8C5D435484D7BD2ADE46FC2CAA48D49C8518AE118BED3AB6D604EE5336B

Key	Value
FileSize	412076
MD5	08B3CE36677FB07D89A49E60A807357C
PackageDescription	ESO 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).
PackageMaintainer	Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.2.0+dfsg-1+b1
SHA-1	EDDFA8E4D2940474F63B25AC9BDAB2C9340BD1C7
SHA-256	F5CDE157AB1385847031F916C70B8A0015D5F3794F32164E289FACCEFEA462DA

Key	Value
FileSize	479446
MD5	05163626569370830CB4BA3492E0B092
PackageDescription	ESO 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).
PackageMaintainer	Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.2.0+dfsg-1+b1
SHA-1	CEDE6337214FC45AF5F212D7F8B8F84CD8EDCD55
SHA-256	89D9D055F1AB77CD76E039FA4BC12C013BD5702025C1FA292279C2316B1D1BB8

Key	Value
FileSize	426848
MD5	C8FC8B61CFE578FB387193CC0948C4CE
PackageDescription	ESO 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).
PackageMaintainer	Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.2.0+dfsg-1+b1
SHA-1	0D7A9C3BDB5386D1AD3C03E278B8A26A53117B63
SHA-256	E99CF0D36C035AAC0C944D8858B13809B9E0F719118FEA0D5165C368314DEA9E

Key	Value
FileSize	353598
MD5	A1BD40963DB2A77A0D7730FE85D0AF94
PackageDescription	ESO 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.2.0+dfsg-1build1
SHA-1	EB736B139332F6B26DE6CFF7CB6FC31819963E2A
SHA-256	97C93587330F9AE975DB4E10FD12ADD6E9FA3078083991808F019B208598BCBD

Key	Value
FileSize	407134
MD5	8BB75CFCA14D06B369847DA5AD3C0659
PackageDescription	ESO 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.2.0+dfsg-1build1
SHA-1	57E12B5F92879BB2A2B01FC61AE6BF5307FC2945
SHA-256	0A0320B5C8F5B44A2C6CBD2E98BE1B3BEC71DBF24EF43CE8BC2912388B5663DD