[HN Gopher] LSST Camera: largest camera for astronomy
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       LSST Camera: largest camera for astronomy
        
       Author : defrost
       Score  : 59 points
       Date   : 2024-04-04 07:57 UTC (2 days ago)
        
 (HTM) web link (www6.slac.stanford.edu)
 (TXT) w3m dump (www6.slac.stanford.edu)
        
       | porphyra wrote:
       | 3200 megapixels custom CCD array cooled to about -100 degC sounds
       | amazing.
       | 
       | The 3.5 degree FoV is around 700 mm focal length equivalent on a
       | full frame camera which makes this relatively wide field by
       | telescope standards, allowing it to capture more of the sky per
       | shot. But the array is 64 cm wide so the actual focal length is
       | around 10 meters.
        
         | perihelions wrote:
         | It has the greatest light-gathering ability (product of field
         | of view * aperture) of any telescope yet. That's the key figure
         | of merit for a surveying telescope! (As I understand--I'm not a
         | domain expert).
         | 
         | - _" Combined with its large aperture (and thus light-
         | collecting ability), this will give it a spectacularly large
         | etendue of 319 m2[?]degree2.[6] This is more than three times
         | the etendue of the largest-view existing telescopes, the Subaru
         | Telescope with its Hyper Suprime Camera[36] and Pan-STARRS, and
         | more than an order of magnitude better than most large
         | telescopes.[37]"_
         | 
         | https://en.wikipedia.org/wiki/Vera_C._Rubin_Observatory
        
           | porphyra wrote:
           | Wow yes, 10.31 m (f/1.23) overall (optical diameter of 8.360
           | m). That's insane.
        
             | mnw21cam wrote:
             | Thanks. It boggles my mind that an article like this about
             | a scientific camera can fail to list the focal length and
             | aperture, which are basically the two most important
             | numbers for any camera.
        
               | ouptppr wrote:
               | Maybe before you get too boggled, consider that the
               | original article is about a scientific instrument
               | designed to be attached to a telescope. The aperture and
               | focal length given in the other source are properties of
               | the telescope, not the instrument.
               | 
               | It's not uncommon to discuss CCD cameras for large
               | telescopes without making any mention of the focal length
               | or aperture of the telescope. See, for example:
               | https://www.eso.org/public/teles-instr/lasilla/ntt/susi2/
               | 
               | Here's a page for another imaging device which lists the
               | aperture and f-number of the telescope--and then gives a
               | separate f-number for the instrument, without stating the
               | instrument's aperture: https://www.eso.org/sci/facilities
               | /lasilla/instruments/wfi/o...
               | 
               | So I don't think the LSST media department dropped the
               | ball on this one. The numbers (focal length and
               | aperture), which you understandably think of as being
               | essential info for any camera, just aren't as relevant
               | here, partly because comparison with other options isn't
               | in the forefront of the scientists minds (the camera is
               | totally bespoke and there are many ways in which it is
               | tailored to the telescope, which constrain its design,
               | including in those two respects).
               | 
               | Focal length and aperture of the LSST camera aren't
               | mentioned here, either https://www.lsst.org/about/camera
        
               | porphyra wrote:
               | Yeah haha I mean even when you buy a consumer camera
               | like, say, a Sony a7 or whatever, it doesn't come with
               | the lens.
        
               | Randalthorro wrote:
               | Focal length and aperture literally mean nothing for this
               | instrument (camera). Telescopes are multi instrument and
               | it's the telescope plus instrument specific mounting
               | configs that determine these. (Focal length is actually
               | pointless except to make sure you design the light path
               | correctly).
               | 
               | Aperture is talked about in the light collecting area of
               | the mirror, and often summarized to its diameter. 8m
               | class telescope, is a telescope with an approximately 8m
               | diameter mirror.
               | 
               | Hubble is a little over 1m.
               | 
               | Other things matter way more for a telescope and are much
               | more interesting.
        
       | ck2 wrote:
       | It is fortunate that storing 15TB per night is now only $300,
       | well before supporting hardware and mirroring.
       | 
       | Imagine having to store that much every day a decade ago.
        
         | imbusy111 wrote:
         | So $600 a decade ago?
         | 
         | [1] https://ourworldindata.org/grapher/historical-cost-of-
         | comput...
        
         | OldGuyInTheClub wrote:
         | They've got fast fiber to get the data off the mountain and
         | into multiple data processing centers in near real-time
         | including alerts when something interesting happens.
         | 
         | "The nightly pipelines are based on image subtraction, a
         | process that highlights differences between two exposures of
         | the same field, and are designed to rapidly detect interesting
         | transient events in the image stream and send out alerts to the
         | community within 60 seconds of completing the image readout. "
         | 
         | https://www.lsst.org/about/dm
        
         | Randalthorro wrote:
         | well we don't have to imagine, there are meeting notes!
        
       | dekhn wrote:
       | A project I worked on donated compute cycles to LSST- it was a
       | full scientific-grade ray tracer that takes star catalogs and
       | uses them to render the image on the camera. It worked well
       | enough, and early enough, that it caught a design error in the
       | physical telescope. That work was done 10 years ago, I think they
       | are wrapping up LSST's assembly now and they will have imaging
       | going next year.
       | 
       | It's very exciting because it's a survey which produces
       | statistical quantities of information about a wide range of
       | objects, and also it's great the US and other governments were
       | willing to fund something at this scope for so long.
        
         | venice_benice wrote:
         | Do you recall the name of the software? I am aware only of
         | PhoSim (https://www.phosim.org/)
        
       | KennyBlanken wrote:
       | ...significantly hampered by low-earth-orbit microsat
       | constellations like Starlink. It boggles the mind that there are
       | half a million microsats planned for launch in the next ten
       | years. Starlink is already causing issues for launches, cutting
       | down launch windows and even blocking ones that had been open
       | because Starlink moves a satellite without clearing it with
       | anyone first.
       | 
       | https://www.lsst.org/content/lsst-statement-regarding-increa...
       | 
       | TLDR: the telescope's field of view means that it will be nearly
       | impossible for them to find a "clear" patch of sky, the
       | brightness off satellites saturates the CCD, which in turn causes
       | crosstalk during readout of the CCDs, and even just masking the
       | primary streak is difficult. I'm sure there are optics issues as
       | well from such bright objects, in the field of view and not.
       | 
       | > During the nominal 30-second visit to a sky patch, satellites
       | in 400-600km LEO orbits typically move about 15 degrees across
       | the sky (about four times the diameter of Rubin Observatory's
       | field of view), and are visible a few hours after sunset and
       | before sunrise. With 400,000 satellites orbiting Earth, tens of
       | thousands of satellites would be visible above the horizon and it
       | would be difficult to find a circle of 9.6 square degrees
       | anywhere on the sky that does not contain satellite streaks.
       | Simulations of the LSST observing cadence and the full SpaceX
       | satellite constellation show that as many as 30% of all LSST
       | images would contain at least one Starlink satellite trail. With
       | the planned constellations of 400,000 satellites at 400-600 km,
       | all images in twilight will contain streaks. The OneWeb
       | constellation at 1200 km will be visible all night long in
       | Chilean summer. Measurements of the brightness of the current LEO
       | satellites in their final orbits indicate that these trails would
       | cause residual artifacts in the reduced data. If these LEO
       | satellites can be darkened to 7th magnitude, then a new
       | instrument signature removal algorithm can remove some of the
       | residual artifacts. This is challenging due to apparent non-
       | linear crosstalk between the 16 channels on each of the 189 CCDs,
       | the cause of which is still under study. The bright main
       | satellite trail would still be present, potentially creating
       | bogus alerts and systematics at low surface brightness. Masking
       | of these trails is not 100% perfect. This is a challenge for
       | science data analysis, adding potentially significant effort.
        
         | lawlessone wrote:
         | >It boggles the mind that there are half a million microsats
         | planned for launch in the next ten years.
         | 
         | Great for Space X, they're creating a need for more space
         | telescopes..
        
         | mrbluecoat wrote:
         | Looks like there was concern about this all the way back in
         | 2016: https://twitter.com/lsstepo/status/804412225926463488
        
         | porphyra wrote:
         | > If these LEO satellites can be darkened to 7th magnitude,
         | then a new instrument signature removal algorithm can remove
         | some of the residual artifacts.
         | 
         | The current generation of Starlink satellites is already above
         | the 7th magnitude, so it no longer saturates the CCD. [1] Of
         | course, darkening them further would always be good.
         | 
         | [1] http://arxiv.org/abs/2306.06657
        
           | perihelions wrote:
           | There's however more considerations than just saturated
           | pixels,
           | 
           | https://www.lsst.org/content/lsst-statement-regarding-
           | increa... ( _" Vera C. Rubin Observatory - Impact of
           | Satellite Constellations"_)
        
             | porphyra wrote:
             | That's true, but this article was also from before the
             | Starlink Generation 2 Mini satellites with magnitude > 7
             | came out.
             | 
             | > Darkening satellites to 7th magnitude would simplify
             | removal of some artifacts in LSST images, but there is no
             | guarantee most of the satellites will be limited in
             | brightness to fainter than 7th magnitude.
             | 
             | I'm curious if they were indeed able to implement the
             | artifact removal or if it remains challenging even then.
        
               | gammarator wrote:
               | "Removal" here means "masking"--the pixels under the
               | bright streaks will always be scientifically unusable
               | because the streaks inflate the noise irrevocably. (You
               | can't see stars in the daytime by "removing" the sun.)
               | 
               | The 7th magnitude limit just minimizes the streak signal
               | cross-talk through the rest of the camera. It also means
               | the satellites are invisible to the naked eye.
        
       | mjsweet wrote:
       | I remember the original Google announcement where it was
       | announced that Google would help with the huge storage
       | requirements for the project, I just dug up the YouTube
       | announcement. Pretty amazed that this video is 17 years old now,
       | a testament to how long these projects are in development for...
       | this 2007 video wasn't even when it began.
       | 
       | https://www.youtube.com/watch?v=thPlpDcaewo
        
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