wise.ssl.berkeley.eduWISE: Wide-Field Infrared Survey Explorer
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wise.ssl.berkeley.edu
Maindomain:berkeley.edu
Title:WISE: Wide-Field Infrared Survey Explorer
Description：WISE will map the sky in infrared light, searching for the nearest and coolest stars, the origins of stellar and planetary systems, and the most luminous galaxies in the Universe.
Keywords：WISE, wide-field infrared survey explorer, nasa mission, solar system, milky way, universe, asteroids, cool stars, warm stars, stars, galaxies, luminous galaxies, galaxy, satellite, infrared telescope, electromagnetic spectrum, infrared, zodiacal light, brown dwarfs,active galactic nuclei, AGN, ultra-luminous infrared galaxies, ULIRGs, lookback times, Arp 220, spiral galaxies, ULIRG, IRAS, hubble space telescope, interstellar gas, all sky, thermal infrared, mid-infrared, allsky, all sky survey, ...
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| Website / Domain: | wise.ssl.berkeley.edu |
| HomePage size: | 19.58 KB |
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| Website IP Address: | 128.32.13.215 |
| Isp Server: | University of California |
wise.ssl.berkeley.edu Ip Information
| Ip Country: | United States |
| City Name: | Berkeley |
| Latitude: | 37.869201660156 |
| Longitude: | -122.2564239502 |
wise.ssl.berkeley.edu Keywords accounting
| Keyword | Count |
|---|---|
| WISE | 8 |
| wide-field infrared survey explorer | 0 |
| nasa mission | 0 |
| solar system | 0 |
| milky way | 0 |
| universe | 0 |
| asteroids | 0 |
| cool stars | 0 |
| warm stars | 0 |
| stars | 0 |
| galaxies | 0 |
| luminous galaxies | 0 |
| galaxy | 1 |
| satellite | 0 |
| infrared telescope | 0 |
| electromagnetic spectrum | 0 |
| infrared | 1 |
| zodiacal light | 0 |
| brown dwarfs | 0 |
| active galactic nuclei | 0 |
| AGN | 0 |
| ultra-luminous infrared galaxies | 0 |
| ULIRGs | 0 |
| lookback times | 0 |
| Arp 220 | 0 |
| spiral galaxies | 0 |
| ULIRG | 1 |
| IRAS | 0 |
| hubble space telescope | 1 |
| interstellar gas | 0 |
| all sky | 0 |
| thermal infrared | 0 |
| mid-infrared | 0 |
| allsky | 0 |
| all sky survey | 0 |
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| content="WISE, wide-field infrared survey explorer, nasa mission, solar system, milky way, universe, asteroids, cool stars, warm stars, stars, galaxies, luminous galaxies, galaxy, satellite, infrared telescope, electromagnetic spectrum, infrared, zodiacal light, brown dwarfs,active galactic nuclei, AGN, ultra-luminous infrared galaxies, ULIRGs, lookback times, Arp 220, spiral galaxies, ULIRG, IRAS, hubble space telescope, interstellar gas, all sky, thermal infrared, mid-infrared, allsky, all sky survey, all sky surveys, all-sky surveys, allsky surveys, sky survey, sky surveys, nearest star, nearest stars, closest star, closest stars, nearby stars, most luminous galaxy, most luminous galaxies, brightest galaxy, brightest galaxies, spitzer, SIRTF, WIRE, MIDEX, Medium Explorer" name="keywords"/ |
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Sep 30, 2014 – How to Use this Site This site is now a rich archive of WISE's extraordinary work. Its primary science mission is complete,but exciting discoveries will keep coming from the extensive data WISE collected in the years 2005-2014. Click on the tabs above for images, news articles and science essays from that time period. If you are looking for news dated after Sep 30, 2014, you can also vist the WISE pages at NASA or JPL . Sky Coverage – this map shows the density of coverage by WISE Read more. Sep 30, 2014 – A Gallery of WISE Images Please check out the many pages of stunning imagery generated from WISE data, along with accompanying descriptions and astronomical information. You can view or dowload small, medium and large versions of most images. More Light Detectives Students use real NASA data to complete an investigation. In this activity, students use real NASA data to complete an investigation via the same basic methods that astronomers use. Students download data directly from NASA’s WISE mission. They then make measurements of those images with the image processing software SalsaJ, and eventually plot and analyze those measurements to find a brown dwarf. In the Going Further section, they follow the same process to find an Ultra-luminous Infrared Galaxy, or ULIRG, and then verify it by finding relevant images taken by the Hubble Space Telescope. The teacher engages and guides students along with the help of a slide show and discussion points. There are questions at the end of each section that the students can answer and turn in to be graded. Note: The current version is a draft that is in field testing . Light Detectives Teachers Guide (pdf) Light Detectives Student Guide (pdf) Light Detectives Presentation (pptx) Light Detectives Data Sheets (xlsx) -- Mission | Science | News & Events | Education & Outreach Multimedia Gallery | For Astronomers | Contact Us WISE at NASA / JPL Display issues? | Last updated 2/6/15 © UC Regents CSE@SSL...