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The Mikulski Archive for Space Telescopes (MAST) is an astronomical data archive. The archive brings together data from the visible, ultraviolet, and near-infrared wavelength regimes. The NASA funded project is located at the Space Telescope Science Institute (STScI) in Baltimore, Maryland and is one of the largest astronomical databases in the ...
The image, along with the individual exposures that make up the new view, is available to the worldwide astronomical community through the Mikulski Archive for Space Telescopes (MAST). MAST, an online database of astronomical data from Hubble and other NASA missions, is located at the Space Telescope Science Institute in Baltimore, Maryland.
NASA Astrophysics Data Archive/Service Centers: these include HEASARC (High Energy Astrophysics Science Archive Research Center), IRSA (Infrared Science Archives), LAMBDA (Legacy Archive for Microwave Background Data Analysis), MAST (Mikulski Archive for Space Telescopes).
In addition to performing continuing science operations of HST and preparing for scientific exploration with JWST and Roman, STScI manages and operates the Mikulski Archive for Space Telescopes (MAST), which holds data from numerous active and legacy missions, including HST, JWST, Kepler, TESS, Gaia, and Pan-STARRS. [4]
This ultimately results in spectra ranging from 80 Å to 825 Å (EUV) and from 1280 Å to 1650 Å (FUV) with 1 Å resolution. Once downlinked and processed, these measurements will be accessible on Mikulski Archive for Space Telescopes (MAST).
The second data release, Pan-STARRS DR2, announced in January 2019, is the largest volume of astronomical data ever released. At over 1.6 petabytes of images, it is equivalent to 30,000 times the text content of Wikipedia. The data reside in the Mikulski Archive for Space Telescopes (MAST). [14]
The project also has a database that is available through the Mikulski Archive for Space Telescopes (MAST). It contains the "goodFraction", describing how often a source was voted as a good source on the website, as well as other information about the source, such as comments from the science team, machine learned classification, cross-matched ...
Only the space telescope XMM-Newton was able to identify the source. It is a white dwarf with about 1.3 solar masses, in orbit about HD 49798 and rotating once every 13 seconds; [ 13 ] this rotation is speeding up by 72.0 ± 0.6 ns per year. [ 6 ]