Parents (Total: 12)
The searched file hash is included in 12 parent files which include package known and seen by metalookup. A sample is included below:
Key |
Value |
FileSize | 477396 |
MD5 | 36D3852665BA37B7D3A54BDF92495CD3 |
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 | 2.4.3+dfsg-1 |
SHA-1 | FB4CFFDCD3D3AC67745E1A84542709CE1909378B |
SHA-256 | BD03FA5F24D6267A89ED763C03A764AAAFADAFC91D2D1AE4BA51802A7659DA82 |
Key |
Value |
FileSize | 459464 |
MD5 | BF5AA2AF1FD8B5940C7561CD404DCF95 |
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 | 2.4.3+dfsg-1 |
SHA-1 | FBE7872286CE89B53E0544E3D1E8C86BB09581AB |
SHA-256 | A6ECB0026D06870834397818D25A9044D0089E2CC575310F24458F40D0F1B52E |
Key |
Value |
FileSize | 548756 |
MD5 | 7B774D5D5C690C1AD50BAFC43FDDB0C4 |
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 | 2.4.3+dfsg-1 |
SHA-1 | B6C87AC7CEF51846AD1962434E51181D948F75F9 |
SHA-256 | 4BB11E9B6BA556172558877F98E9B23702C96254E0C6CD3DF42D3C2B65C795F7 |
Key |
Value |
FileSize | 76400 |
MD5 | F5D8459ED455DBB253ACDC570E9DD1C9 |
PackageDescription | ESO data reduction pipeline calibration data downloader for HAWK-I
This package downloads calibration data of the data reduction pipeline for
the HAWK-I instrument of the Very Large Telescope (VLT) from the European
Southern Observatory (ESO). |
PackageMaintainer | Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org> |
PackageName | cpl-plugin-hawki-calib |
PackageSection | science |
PackageVersion | 2.4.3+dfsg-1 |
SHA-1 | 542F387722688F7F2843AA373EFD0D1FEDC30FEC |
SHA-256 | FE73C6B44EA51D10AC846009BFDE5EBDE563721A6C4A4B534892F41882B49B1E |
Key |
Value |
FileSize | 468408 |
MD5 | AFB8672F4237B6E084ADD1D7965FEC77 |
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 | 2.4.3+dfsg-1 |
SHA-1 | 5F5A26B6ED1A94FCCDB5418A6EA9D38509C7832D |
SHA-256 | A8BF33C01629FEB6CE296AB321AF3C889D6452D6BE48DD6507E7D949D35B2061 |
Key |
Value |
FileSize | 477952 |
MD5 | 3CAA106DD6246DCF218DE138AE022F77 |
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 | 2.4.3+dfsg-1 |
SHA-1 | 07D5C627FC555F637353012D04FEE7C6F1E6113C |
SHA-256 | 4B04179EDF606ECC3AE590EC5EB34589B088566F820C6F00530B40016D5D6193 |
Key |
Value |
FileSize | 471088 |
MD5 | B8FD83D2BD28D19D4560F9F25976C8F4 |
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 | 2.4.3+dfsg-1 |
SHA-1 | 1C8FE32120734D45F159CF07A89DF8F4AE4700E1 |
SHA-256 | 33B192C73AF4F5B97638210C15508D770F5731F4969E5D34D0864DB81751A269 |
Key |
Value |
FileSize | 547580 |
MD5 | B18CA767A1199AA5AF489CE17CD7BB65 |
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 | 2.4.3+dfsg-1 |
SHA-1 | F236FEA9C8FD567B3682BBF6658FCD7300D6B0E0 |
SHA-256 | F686E8D97B34E3D32A5A43F84F58708D1760617E24A4B37F15023F1F5FB5E51F |
Key |
Value |
FileSize | 515728 |
MD5 | 178BC39B67CCFAC7374837B6783DEFDE |
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 | 2.4.3+dfsg-1 |
SHA-1 | 1B3779DC0D999F9AA02A89F5F799490440FB4A47 |
SHA-256 | 88F0D4E52748D0A396F071C0EAF70FDD8F9BB0D1A987F7729A2B4E284A95C891 |
Key |
Value |
FileSize | 471024 |
MD5 | 948CB92838A4404E1AA12023641CDAB5 |
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 | 2.4.3+dfsg-1 |
SHA-1 | 2E3B1A4071995F103CF47F407CA4EF4591C36C9F |
SHA-256 | 382F8A1605747E26EE33758BD402E6C71DCB38950105E0EEF9E246951EF5205A |
Key |
Value |
FileSize | 470896 |
MD5 | 04E6CDD5BC92409B9B8ACCDBDA45598D |
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 | 2.4.3+dfsg-1 |
SHA-1 | 1AB820B4CF5A53A38486A13C3E51A928A2FE694D |
SHA-256 | F4E93FD2283238717114016AB9CA5CDBD1B98D37FDA6784152CB5222AD3B3867 |
Key |
Value |
FileSize | 167796 |
MD5 | 40574540DEC596DCC1B170F3330307A4 |
PackageDescription | ESO data reduction pipeline documentation for HAWK-I
This package contains the HTML documentation and manpages for the data
reduction pipeline for the HAWK-I instrument of the Very Large Telescope
(VLT) from the European Southern Observatory (ESO). |
PackageMaintainer | Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org> |
PackageName | cpl-plugin-hawki-doc |
PackageSection | doc |
PackageVersion | 2.4.3+dfsg-1 |
SHA-1 | BEDDE3D6B0FF5F753CE66BDE6F4EF46E69436760 |
SHA-256 | 2148D1A28D132F54A965FF405938AF1E317E2C0F940E037724E6472A73966E99 |