![]() |
|
![]() |
|
To expand on this, Webb uses the Deep Space Network (DSN) to communicate with us. It can’t stream data back 24/7. There are generally three contacts per day each lasting a few hours, but I believe this is dependent on the scheduling of contacts with other missions that also use the DSN. Also, the science data that is sent back is a stream of packets from all the data that was taken since the last contact. The packets are arranged for efficient transmission. One of the first steps of the science data processing is to sort the packets into exposures. Often packets for an exposure are split among multiple SSR (which stands for solid-state recorder) files. Sometimes there are duplicate packets between SSRs (data sent at the end of a contact is repeated at the beginning of the next contact). Only when the processing code determines that all expected packets are present—by using clues from other subsystems—can the next step (creating the uncalibrated FITS) begin. If anyone is interested more details, the packet stuff is based on standards from the Consultative Committee for Space Data Standards (https://public.ccsds.org/Publications/BlueBooks.aspx). |
![]() |
|
Are they not doing that? What is the origin of the idea that they sit on the images too long choosing a custom wavelength conversion formula? Is it just that their images look good?
|
![]() |
|
Hmmm, unfortunate timing: "Planned Outage - On Friday, April 12th starting at noon through Sunday, April 14th, Space Telescope Live may be unavailable. We apologize for any inconvenience." |
![]() |
|
The other option is to use Chrome/Firefox headless mode and take a screen shot. You can probably then crop it automagically with some command line image tool to get you an image for your desktop. |
![]() |
|
I presume it's not a live view of what Webb is seeing but existing images / visualisations from other sources pointing in the same direction Webb is right now.
|
You can read interesting details about the current observation at the top, though. Currently:
* A census of high-redshift kpc-scale dual quasars
* A 49 minute, 55 second observation.
There’s a link to the research proposal [2]
Apparently it’s a six-month survey of dual (possibly lensed) quasars. Gravitational lensing can cause magnification, distortion, and duplication of the image of whatever is behind it, so this is a way to learn more about very distant (early) quasars.
A quasar is a supermassive black hole at the center of a galaxy, so this seems like a way to take lensed pictures of a lot of early galaxies?
[1] https://en.m.wikipedia.org/wiki/2MASS [2] https://www.stsci.edu/jwst/science-execution/program-informa...