preview
loading

'Wfcam' web sites

Wfcam home page
2013-02-16
wfcam Home Page wfcam Home Wide Field Infrared Camera For UKIRT wfcam is an IR widefield camera for the UK Infrared Telescope on Mauna Kea UKIRT , and is currently the most capable IR imaging survey instrument in the world. The camera has been designed to maximize survey speed at J, H and K while retaining excellent image quality. With large allocations of UKIRT time, unprecedented surveys in depth area will be possible. Both
Wfcam science archive
wfcam SCIENCE ARCHIVE WSA Home Start Here Data Overview Known Issues the Surveys Coverage Maps Schema browser Data access Login Archive Listing GetImage ColourImage MultiGetImage Region Menu query Freeform SQL CrossID Analysis services SQL Cookbook Q A Glossary Release History non.Survey Gallery Publications Monitor Downtime Links IFA ROE Home. Overview. Browser. Access. Login. Cookbook. nonSurvey WSA. wfcam Science Archive UKIDSS
Wfcam data processing mdash; cambridge astronomy survey unit
2016-01-07
wfcam data processing mdash; Cambridge Astronomy Survey Unit Skip to content. Skip to navigation Personal tools Log in Search Site only in current section Advanced Search hellip; Navigation HomeSurveys ProjectsDocumentsPublications You are here Home Surveys Projects wfcam Data Processing Info wfcam data processing wfcam reduction progress per semester see also the information for the illumination correction and the overall version
Cambridge astronomy survey unit
wfcam Technical Documentation Data Processing Status Survey Progress and Data Access more.. VST Technical Documentation Data Processing Status Survey Progress and Data Access more.. Spectroscopic Surveys GAIA.ESO Survey WEAVE 4MOST NEW CASUTools Software Release more information The Cambridge Astronomical Survey Unit CASU is part of the Institute of Astronomy, Cambridge University. The main projects that we are currently working
Ukidss archive
2013-02-16
wfcam Science Archive WSA. DR8 is proprietary to ESO astronomers for 18 months. The current World Release is DR4. Before World Release, access to the data requires a username and password, as explained here and first announced in the ESO Messenger, No. 119, Mar 2005. You can get your username and password from your community contact someone at your institution. To see if you have a community contact, check the list of registered
Ukidss home page
wfcam on the UK Infrared Telescope UKIRT in Hawaii. wfcam has four 2048x2048 Rockwell devices, at 94 spacing, as illustrated at the top. The pixel scale of 0.4 arcsec gives an exposed solid angle of 0.21 sq. degs. Four of the principal quarry of UKIDSS are the coolest and nearest brown dwarfs, high.redshift dusty starburst galaxies, elliptical galaxies and galaxy clusters at redshifts 1 139;z 139;2, and the highest.redshift
Ukirt discovers impossible binary stars
2015-05-08 ⚑news ⚑r&d
wfcam Transit Survey, and appear in the journal Monthly Notices of the Royal Astronomical Society. This artist impression shows the tightest of the new record breaking binary systems. Two active M4 type red dwarfs orbit each other every 2.5 hours, as they continue to spiral inwards. Eventually they will coalesce into a single star. Credit J. Pinfield, for the RoPACS network. Click on the image for a high resolution version.About
Eso archive query form
2012-11-27 ⚑shop
wfcam LGSF MASCOT MAD Category SCIENCE CALIB ACQUISITION Data Product Info Type Any OBJECT STD ASTROMETRY BIAS DARK FLAT User defined input Mode Any IMAGE SPECTRUM ECHELLE MOS MXU IFU POLARIMETRY CORONOGRAPHY INTERFEROMETRY User defined input Dataset ID Orig Name Release Date OB Name OB ID Instrumental Setup Exptime Filter Grism Grating Slit Instrument Mode Additional Tools and Parameters Airmass FITS Header Display Distance
The most distant quasar both headache and opportunity. gemini observatory [..]
2013-03-21
wfcam which was built at the Astronomy Technology Center ATC at the Royal Observatory Edinburgh. The observations are made at the United Kingdom Infrared Telescope UKIRT on the summit area of Mauna Kea in Hawai i. Both the ATC and UKIRT are establishments of the UK Science and Technology Facilities Council STFC. 4 Light from distant parts of the universe is stretched out or redshifted by the expansion of the universe. This means
Topcat leader of the catalogue manipulation gang
2013-03-21 ⚑blog ⚑r&d
wfcam photometry tables. Couple of times I 8217;ve managed to work with whole Astrogrid suite connecting TOPCAT and ALADIN 8211; nice idea but since everything is on java it 8217;s gradually slows down the whole system. Using TOPCAT separately I found that by increasing the Java 8217;s heap memory things are manageable. The command for the quick reference would be 8220;topcat.Xmx256M 8221; or 8220;java.Xmx256M.jar topcat.full.jar
Libraweb
2016-01-09 ⚑books
wfcam near.infrared survey of M31 dwarf elliptical satellites; C.B. Pereira, E.G. Jilinski, N.A. Drake, D.B. de Castro, V.G. Ortega, C. Chavero, F. Roig, Abundance and kinematic analysis of the CH star CD.62 1346. The first hypervelocity red giant.; P. Drazinos, E. Kontizas, A. Karampelas, M. Kontizas, A. Dapergolas, I. Bellas.Velidis, Star forming regions with indication of hierarchical structure in a sample of spiral galaxies;
Ukirt discovers impossible binary stars
2015-05-08 news ⚑r&d
wfcam Transit Survey, and appear in the journal Monthly Notices of the Royal Astronomical Society. This artist impression shows the tightest of the new record breaking binary systems. Two active M4 type red dwarfs orbit each other every 2.5 hours, as they continue to spiral inwards. Eventually they will coalesce into a single star. Credit J. Pinfield, for the RoPACS network. Click on the image for a high resolution version.About
Eso archive query form
2012-11-27 shop
wfcam LGSF MASCOT MAD Category SCIENCE CALIB ACQUISITION Data Product Info Type Any OBJECT STD ASTROMETRY BIAS DARK FLAT User defined input Mode Any IMAGE SPECTRUM ECHELLE MOS MXU IFU POLARIMETRY CORONOGRAPHY INTERFEROMETRY User defined input Dataset ID Orig Name Release Date OB Name OB ID Instrumental Setup Exptime Filter Grism Grating Slit Instrument Mode Additional Tools and Parameters Airmass FITS Header Display Distance
Topcat leader of the catalogue manipulation gang
2013-03-21 blog ⚑r&d
wfcam photometry tables. Couple of times I 8217;ve managed to work with whole Astrogrid suite connecting TOPCAT and ALADIN 8211; nice idea but since everything is on java it 8217;s gradually slows down the whole system. Using TOPCAT separately I found that by increasing the Java 8217;s heap memory things are manageable. The command for the quick reference would be 8220;topcat.Xmx256M 8221; or 8220;java.Xmx256M.jar topcat.full.jar
Libraweb
2016-01-09 books
wfcam near.infrared survey of M31 dwarf elliptical satellites; C.B. Pereira, E.G. Jilinski, N.A. Drake, D.B. de Castro, V.G. Ortega, C. Chavero, F. Roig, Abundance and kinematic analysis of the CH star CD.62 1346. The first hypervelocity red giant.; P. Drazinos, E. Kontizas, A. Karampelas, M. Kontizas, A. Dapergolas, I. Bellas.Velidis, Star forming regions with indication of hierarchical structure in a sample of spiral galaxies;

'Wfcam' white pages

  • ndelmottei-tieso.org
  • mortlockei-tiimperial.ac

Sound like 'wfcam'


visitors counter and page-rank checker and web-site statistics UNCENSORED  SEARCH  ENGINE  HOME-PAGE

No cookies are saved on your client
We are completely no-profit and volunteers

Use robots.txt to block indexing
Contact us via email for other removals

Read DMCA Policy

CopyLeft by GiPOCO 2006-2023
Contact us to contribute
info (at) gipoco.com


All trade marks, contents, etc
belong to their respective owners