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 | 260978 |
MD5 | 5F77ED0FB77CB9283D78B6CC956FBAC7 |
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 | 1.8.21+dfsg-1 |
SHA-1 | 3D00E429E99C1B8D428D87C587056182BBA9003D |
SHA-256 | C39FAE0786F62BF2CDED8B18E826ADF7C549FC82B84F7602C5DC53034AF832DA |
Key |
Value |
FileSize | 224692 |
MD5 | D1343C262A1A7E0BD8BD4569E23F068D |
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 | 1.8.21+dfsg-1 |
SHA-1 | 5671A6932A008A7BDE978A313EC947BFE2999B20 |
SHA-256 | 136A0A4E926B114E41A51F5D4B1915255A9E2B8943770353493F216FBD564D4E |
Key |
Value |
FileSize | 223236 |
MD5 | 250B250B503BC1BE132F283F2DE01047 |
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 | 1.8.21+dfsg-1 |
SHA-1 | 745F2CE42DE269179A9D006DAA409DDB5E4373D2 |
SHA-256 | 97E966AABBC439DB1190D4805629759BA2314151762DE45E9E685D8179ACF04A |
Key |
Value |
FileSize | 203830 |
MD5 | 0217B24BC288D83D67B33CC086B6DC72 |
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 | 1.8.21+dfsg-1 |
SHA-1 | A3D2F47DDC44170E6E18F65F24ECF6BC5365A200 |
SHA-256 | 8BAD397247F133240BFF3538BA243E921F9D81B6F302F0F295AE0F28FE15DF22 |
Key |
Value |
FileSize | 41456 |
MD5 | 9BBB1D4018E3CFA80372BBA15CEE51C9 |
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 | 1.8.21+dfsg-1 |
SHA-1 | 8C8B3ADC165D3B788C9EBBC523DFD1A41E8175D4 |
SHA-256 | 892077FCF1F09E0C1D507FB7D37E2698206802FCD6CE34C6DA528745A718862E |
Key |
Value |
FileSize | 238384 |
MD5 | BD0858144B9991FC7E5BAE6A82F03021 |
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 | 1.8.21+dfsg-1 |
SHA-1 | 8DF945A85ED8F9B9ED454AE4BF385B1504291ADF |
SHA-256 | A63DB43EAB793C6B3E0BF690F6285C633FB2628F6470D923308272C4B5966746 |
Key |
Value |
FileSize | 106990 |
MD5 | 8144AF0B24DEACA4A80D5C83D3CCAC1B |
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 | 1.8.21+dfsg-1 |
SHA-1 | A73452F1285561655061BD422D85750AF77B889D |
SHA-256 | 21844FF71341A5C6BF55356C03F60F981AF2C009576BE235784F026F7B709BD3 |
Key |
Value |
FileSize | 227748 |
MD5 | B2ACC305E3A6F4603A32574AC2FA46EC |
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 | 1.8.21+dfsg-1 |
SHA-1 | FAFAFF50844AC69EF126AC054E01E64C67733705 |
SHA-256 | 129BF7506968CEB0DAF1299EEF863D41B29E5AA4EBA5505D0C3DBD8CAD911A64 |
Key |
Value |
FileSize | 220720 |
MD5 | E4E92A0B8190448093C1085FB0D1AB85 |
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 | 1.8.21+dfsg-1 |
SHA-1 | 5F53BAE9EC1154ED30C70C9E236D9A12E80D8EED |
SHA-256 | 7104AFD5FC486C6AD3216BF94DBBF5645F48AF5AA637F090A9BBBDD4D0A7C17C |
Key |
Value |
FileSize | 226012 |
MD5 | 4C289725D3042772C3CC4229546F32DC |
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 | 1.8.21+dfsg-1 |
SHA-1 | 889A99B4EFD1D9875279122129BC03E6D652C846 |
SHA-256 | 3E3320066BBF6E79776FAB1ECD889581BBED37D5A340ABF0247820338B9C6E8C |
Key |
Value |
FileSize | 228074 |
MD5 | CE29F2691A6DA88FF83D73C679596827 |
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 | 1.8.21+dfsg-1 |
SHA-1 | FFAB13A4EB060F369871AD9885635F1D6BDEAB73 |
SHA-256 | 8D0D52E213F4C1B1787D5035FF57338A5A51EE8C5F408362A01B3492A2590DA5 |
Key |
Value |
FileSize | 216900 |
MD5 | 58F4C14FBDAB174013AEF2ADD25C1325 |
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 | 1.8.21+dfsg-1 |
SHA-1 | FB0E3DEC94087E5EABFE6031DC01EEAB89A68165 |
SHA-256 | EBFA621F4DF309A4CFE2A32612DD9B29AB3DC5A9CA11F9F427CB74E87E4711C7 |