MAST
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Follow us on BlueSky: https://t.co/jYAkjn95or MAST archives UV/optical/IR data from NASA missions, contributed science products, and analysis tools.
Baltimore, MD, USA
Joined March 2013
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Mission Update: The first survey from the SDSS Legacy Archive at MAST is now available! MAST+SDSS-V partnership to host a copy of all science-ready SDSS data side-by-side with our space missions. Read more: https://t.co/AVV1Bso3UF
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HLSP Update: TICA = quick-look, calibrated #TESS full frame images from Sector 85, Orbit 1, Part A are now available at MAST. https://t.co/6OeuoAWGw4
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HLSP Update: GLASS-JWST augmented with NIRSpec spectra of 245 unique sources, a spectral template, and a detection catalog of >60 emission lines. These enable an exploration of cosmic evolution from cosmic noon (z~2) to the era of reionization (z> 5). https://t.co/pwssE2jAyM
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HLSP Update: TICA = quick-look, calibrated #TESS full frame images from Sector 84, Orbit 2, Part B are now available at MAST. https://t.co/6OeuoAW8Gw
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HLSP Update: TESS-SPOC calibrated light curves and target pixel files from #TESS full frame images for Sector 72 are now available at MAST. This Sector adds 159999 targets derived from 200 second cadence FFIs. https://t.co/SLPBpu2WBE
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HLSP Update: TICA = quick-look, calibrated #TESS full frame images from Sector 84, Orbit 2, Part A are now available at MAST. https://t.co/6OeuoAWGw4
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HLSP Update: OPAL HST observations of Saturn from Cycle 31 are now available at MAST. OPAL is a multi-year HST survey of the outer planets to observe how their atmospheres change over time. https://t.co/yYvQTVJluT
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HLSP Update: QLP calibrated light curves from #TESS full frame images for Sector 80 are now available at MAST. This Sector adds 1750792 targets derived from 200 second cadence FFIs. https://t.co/qEEOVhaNoF
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HLSP Update: REFERENCE-ATLASES, 19 new white dwarf (WD) stars were added that are fainter than most of the other CALSPEC stars. Therefore, 19 stellar spectra files (stis) and 19 model files (mod) are being delivered for the first time. https://t.co/L5z8VR44qm
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HLSP Update: TESS-SPOC calibrated light curves and target pixel files from #TESS full frame images for Sector 71 are now available at MAST. This Sector adds 159,999 targets derived from 200 second cadence FFIs. https://t.co/SLPBpu2oM6
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New HLSP: Scylla is a pure-parallel HST-WFC3 imaging survey that operated alongside the ULLYSES survey. Scylla surveyed LMC and SMC fields from the near UV to the IR. The first data release consists of 96 fields imaged over 342 orbits. https://t.co/HoWoeB9psj
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HLSP Update: TICA = quick-look, calibrated #TESS full frame images from Sectors 84, Orbit 1, Parts A and B are now available at MAST. https://t.co/6OeuoAW8Gw
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HLSP Update: TICA = quick-look, calibrated #TESS full frame images from Sector 83, Orbit 2, Part B is now available at MAST. https://t.co/6OeuoAW8Gw
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HLSP Update: TICA = quick-look, calibrated #TESS full frame images from Sector 83, Orbit 2, Part A is now available at MAST. https://t.co/6OeuoAWGw4
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HLSP Update: TICA = quick-look, calibrated #TESS full frame images from Sector 83, Orbit 1, Parts A and B are BOTH now available at MAST. https://t.co/6OeuoAW8Gw
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New HLSP: SMILES is a 34 sq arcmin multi-band JWST/MIRI imaging survey of the GOODS-S/HUDF region with NIRSpec follow-up, aimed at cosmic noon science. Its first data release presents custom-reduced mosaics in 8 MIRI bands & a photometric catalog: https://t.co/ObN4yZ0GyW
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New HLSP: The WIDE Survey releases reduced JWST/NIRSpec spectra from the first 5 (of 31) pointings from the CANDELS/AEGIS fields, each with an average of 135 galaxies. 2D and 1D extracted spectra from low-resolution PRISM and high-resolution gratings! https://t.co/D2KeENR1Ll
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HLSP Update: TICA = quick-look, calibrated #TESS full frame images from Sector 82, Orbit 2, Part B is now available at MAST. https://t.co/6OeuoAW8Gw Note that due to a downlink issue, ~5% of images are missing and will be added next week.
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HLSP Update: MSTARPANSPEC adds data for LTT 1445A and GJ 486, the two closest M-dwarfs with transiting exoplanets. Panchromatic spectra are constructed from UV and X-ray observations, Ly-a reconstructions, DEM estimates, and BT-settl models. https://t.co/QUXNkr9Cmj
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