The SDSS 3D Universe MapEducation
for their secret attribute keys {αk}, and then directly calculate the traditional content key κ for final decryption of CT: C/∏k∈IAe(gαk,C′)=κ, where the value C=κ⋅∏k∈IAe(g,g)αks and C′ = gs are components of the CT, and e is a bilinear map...
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This is the largest IFU map made (to date) of the Milky Way, and contains well-known nebulae (the Horsehead Nebula, Flame Nebula, IC 434, and IC 432), as well as ionized interfaces with the neighboring dense Orion B molecular cloud. We resolve the ionization structure of each nebula, ...
It will also create an integral-field spectroscopic map of the gas in the Galaxy and the Local Group that is 1,000x larger than the current state of the art and at high enough spatial resolution to reveal the self-regulation mechanisms of galactic ecosystems. SDSS-V will pioneer systematic...
The distribution of extinction within the EDSGC area was obtained using the Stark {\\\it et al.} HI map and the IRAS $100\\\mum{m}$ flux map. We find that the amplitude of the whole EDSGC correlation function varies by less than ${m \\\delta w}=0.003$ for reddening ratios $m...
* Move get_fibermap_table to tools.py * Move schemas to target.schemas * Add configuration_to_dataframe tool * Also monkeypatch SDSSCORE_DIR * Allow passing additional col-value to configuration_to_dataframe * Remove polars.lit where not needed ...
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We find that (i) the dust reddening map of Schlegel et al. overestimates E(B - V) by about 14 per cent, consistent with the recent work of Schlafly et al. and Schlafly & Finkbeiner; (ii) after accounting for the differences in reddening normalization, the newly deduced reddening ...
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