The Lanczos sampler is a truncated version of the optimal sampling function, sinc(x). The
kernel of this sampler is given as
f(x) = sinc(pi x) sinc(pi x/n) |x| < n
0 |x| >= n
Here x is given in units of pixels and the sinc function is just sin(x)/x. Take a look at Wikipedia for a sense of the function.
Let’s say we want to sample our function at 4.8 when we have measured values, f_n at the integer values of x. If we are using an order 3 Lanczos sampler then the value, m(x) we measure would be
m(4.8) = f_2 f(-2.8) + f_3 f(-1.8) + f_4 f(-0.8) +
f(5) f(0.2) + f(6) f(1.2) + f_7 f(2.2)
This is how we have used the Lanczos sampler since we introduced it into SkyView. A keen-eyed user, Benjamin Winkler, noted that his resampled images using the Lanczos sampler were slightly fainter than the originals on average. It turns out that the Lanczos sampler as given above is not quite normalized. If we integrate f(x) the total integral for n-3 is about 0.997, about 0.3% less than unity.
We have updated the Lanczos sampler to properly normalize the sampler. The correction gets smaller with increasing n.
Since SkyView samples in two directions, the introduced error is actually the square of the value in the table. The renormalized samplers will be installed in the next release of SkyView next week. Fortunately the error of order 1% or less except for the first order Lanczos sampler.
If there are any users who would prefer to use the unnormalized samplers we have added the LanczosNorm setting, but this will only be available to SkyView-in-a-Jar users.
We apologize for this long-standing issue. We greatly appreciate any feedback or concerns you have with SkyView processing.
In the next few days we’ll be updating the Fermi survey datasets. The updates include data through week 379 of the mission (in October). This adds several years of data since we last updated Fermi early in 2012. Unlike the previous edition where the survey was given as count maps, the new data are rendered as intensity maps where we have divided each pixel by the exposure. These new surveys also are based upon the recently reprocessed Pass 8 Fermi archive data.
Many thanks to Dave Davis for providing the updated maps. We’re now planning on updating the Fermi data regularly — likely each quarter — using the Hera facility at the HEASARC. Click on the comparison all-sky images to see the substantial increase in the signal to noise of the Fermi data.
RGB image of Fermi bands 3,4,5: Old data
RGB Image of Fermi Bands 3,4,5: New Data
Update (11/17/2015): SkyView version 3.1.15 has been released with the new Fermi surveys.
Posted in Notices
FIRST image of 3C273 generated in SkyView
SkyView version 3.1.14 has been released with a change that affects FIRST survey images.
It was brought to our attention that some FIRST images generated using SkyView differed from images generated via the FIRST web server. We investigated and found that the files we created to describe FIRST data contained some older FIRST file names. These older files were being retrieved to generate FIRST images instead of newer reprocessed data files. We have updated out FIRST data description files so that only the latest data files will be used to generate FIRST images in SkyView.
We’ve just released new version of SkyView that fixes a couple of bugs associated with using SkyView-in-a-Jar. Users of the web pages should not see any changes.
There is a batch mode option in the jar which allows many requests to be run without restarting Java each time. In some cases batch mode requests after the first would fail. SkyView attempts to optimize the calculation of the resampling geometry when a user requests images from multiple surveys that have exactly the same geometry on the sky, (I.e. they are broken into tiles with the same sky coverage like the four IRAS or IRIS surveys). Unfortunately this ‘optimization’ was sometimes being applied to subsequent batch mode requests even though the requested positions were quite different. Thanks to Kelley Hess for bringing this to our attention. When we fixed this we also updated the parsing of quotes in the batch file to mimic the behavior of the command line more closely.
The other problem did not cause any errors in the output. If a user had set the SaveBySurvey flag to request that data from different surveys be saved in different cache directories, then in a request where there was both multiple surveys requested and a contour image, the cached data for the second and later images was being stored in the directory associated with the survey that contour image was taken from. E.g., if the user had specified
SaveBySurveys Survey=s1,s2,s3 Contour=c1 position=xxx
then the cached files for surveys s2 and s3 were stored in the directory for c1. This is unlikely to be a problem for most users, but it meant that we occasionally had junk in the cache that our SkyView web server maintains.
We have released SkyView v3.1.12 with 2 enhancements! This new version adds social network sharing options to the SkyView Image Gallery and a helpful option to the Overlays section of the main SkyView Query form.
Facebook and Twitter Share buttons are now displayed with all images in the SkyView Image Gallery. So if you have an account on either of these social networks you can share images that you or other users have created. If you are interested but have never added an image to the Gallery check out this post
The new feature in the Overlays section of the SkyView Query form is the option to draw a reticule indicating where the center of your SkyView image is located.
Below are screen shots from a SkyView Image Gallery page, an individual gallery image, and the SkyView Query form showing the location of the new reticule overlay option. Note that the gallery images also demonstrate the new overlay option.
We’re getting ready to release the next version of SkyView. The only significant change is an update to the WISE datasets which will now point to the All-WISE data release. This provides significantly deeper coverage in some areas and bands but is structurally similar to the previous data sets. Since we’ll be building up the All-WISE data available in our caches, WISE retrievals may be a little slower on average for a while since the base images will more frequently need to be downloaded from the IRSA archive. To access the All-WISE data from the SkyView-in-a-Jar you will need to download the latest jar file.
We’ll be making this the default release shortly (within the day), but if you can’t want you can get the the new release as: http://skyview.gsfc.nasa.gov/v3.1.10
For more information on the All-WISE data see this summary at IRSA.
If you have any questions or concerns or suggestions for new surveys please let us know.
A new version of SkyView, v3.1.8, has been installed as the default version. The significant change from the user perspective is that the GALEX DR7 is included. New data is mostly in the NUV. To access these data through SkyView-in-a-Jar you will need to download a new copy of the jar file.
We’re testing out a new version of SkyView where we’ve upgraded the GALEX survey to include more GR7 data. There are a few minor internal changes. Most of the new data is for the NUV. When we release this survey we will probably clean out the cache of GALEX data at the SkyView site and start repopulating it with the latest files from MAST. Some of the tile files may have been updated since we last downloaded them. This may slightly slow down generation of images as we build the cache back up.
If you wish to try the new release, start at the URL
Let us know if you have any problems — or suggestions for additional changes.
Posted in Notices
Tagged GALEX, Release
One of the restrictions on SkyView is that you need to specify a fixed position in the sky to look at. For many years the SkyView machine has hosted a companion service, SkyMorph, that allows you to look for many moving targets: asteroids, comets and some planets. It uses the Horizons service at JPL to get the position of the moving target as a function of time and then uses the epoch of various observations to find which fields of view might include the object. The primary set of observations available in SkyMorph are data from the Near Earth Asteroid Tracking (NEAT) project which has about 700,000 images of the sky. DSS and other datasets are also available. Since the NEAT project looked at some areas of the sky dozens of times, the data can also be used to look for transients or high proper motion objects.
In the next year or so SkyMorph will be leaving the SkyView host and moving to JPL. You can access SkyMorph through its ‘classic’ interface, or try the new service at JPL which is now available as an early beta version.
SkyView‘s disk area for user-generated images filled up on the morning of August 24 (EDT) and the problem was not corrected until about 9 AM on August 25. SkyView and SkyMorph requests during that time failed. We apologize for any inconvenience to our users.