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- W3174746124 endingPage "4483" @default.
- W3174746124 startingPage "4459" @default.
- W3174746124 abstract "ABSTRACT Improving our knowledge of global Milky Way (MW) properties is critical for connecting the detailed measurements only possible from within our Galaxy to our understanding of the broader galaxy population. We here train Gaussian process regression (GPR) models on SDSS (Sloan Digital Sky Survey) galaxies to map from galaxy properties (stellar mass, apparent axial ratio, star formation rate, bulge-to-total ratio, disc scale length, and bar vote fraction) to ultraviolet (UV; GALEX FUV/NUV), optical (SDSS ugriz), and infrared (IR; 2MASS JHKs and WISE W1/W2/W3/W4) fluxes and uncertainties. With these models, we estimate the photometric properties of the MW, resulting in a full UV-to-IR spectral energy distribution (SED) as it would be measured externally, viewed face-on. We confirm that the MW lies in the green valley in optical diagnostic diagrams, but show for the first time that the MW is in the star-forming region in standard UV and IR diagnostics – characteristic of the population of red spiral galaxies. Although our GPR method predicts one band at a time, the resulting MW UV–IR SED is consistent with SEDs of local spirals with characteristics broadly similar to the MW, suggesting that these independent predictions can be combined reliably. Our UV–IR SED will be invaluable for reconstructing the MW’s star formation history using the same tools employed for external galaxies, allowing comparisons of results from in situ measurements to those from the methods used for extragalactic objects." @default.
- W3174746124 created "2021-07-05" @default.
- W3174746124 creator A5008859611 @default.
- W3174746124 creator A5026494828 @default.
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- W3174746124 creator A5066271293 @default.
- W3174746124 creator A5075874259 @default.
- W3174746124 creator A5083519136 @default.
- W3174746124 date "2021-09-15" @default.
- W3174746124 modified "2023-10-16" @default.
- W3174746124 title "Constraining the Milky Way’s ultraviolet-to-infrared SED with Gaussian process regression" @default.
- W3174746124 cites W1506021077 @default.
- W3174746124 cites W1586340492 @default.
- W3174746124 cites W1842880767 @default.
- W3174746124 cites W1869753654 @default.
- W3174746124 cites W1924655545 @default.
- W3174746124 cites W1934387688 @default.
- W3174746124 cites W1939543898 @default.
- W3174746124 cites W1961031417 @default.
- W3174746124 cites W1969141849 @default.
- W3174746124 cites W1970683243 @default.
- W3174746124 cites W1970932181 @default.
- W3174746124 cites W1977486943 @default.
- W3174746124 cites W1978107999 @default.
- W3174746124 cites W1984455337 @default.
- W3174746124 cites W1987134687 @default.
- W3174746124 cites W1998961346 @default.
- W3174746124 cites W2004037589 @default.
- W3174746124 cites W2011301426 @default.
- W3174746124 cites W2013527347 @default.
- W3174746124 cites W2018075550 @default.
- W3174746124 cites W2018460805 @default.
- W3174746124 cites W2023037133 @default.
- W3174746124 cites W2024370579 @default.
- W3174746124 cites W2026619221 @default.
- W3174746124 cites W2028715663 @default.
- W3174746124 cites W2031521127 @default.
- W3174746124 cites W2033223429 @default.
- W3174746124 cites W2034276863 @default.
- W3174746124 cites W2034532013 @default.
- W3174746124 cites W2034569796 @default.
- W3174746124 cites W2035541286 @default.
- W3174746124 cites W2036491734 @default.
- W3174746124 cites W2038434077 @default.
- W3174746124 cites W2039414721 @default.
- W3174746124 cites W2049062775 @default.
- W3174746124 cites W2052937506 @default.
- W3174746124 cites W2055864709 @default.
- W3174746124 cites W2060864745 @default.
- W3174746124 cites W2061939373 @default.
- W3174746124 cites W2073751390 @default.
- W3174746124 cites W2074571006 @default.
- W3174746124 cites W2074747635 @default.
- W3174746124 cites W2075074183 @default.
- W3174746124 cites W2080927107 @default.
- W3174746124 cites W2081173787 @default.
- W3174746124 cites W2081810596 @default.
- W3174746124 cites W2082266584 @default.
- W3174746124 cites W2093052816 @default.
- W3174746124 cites W2095917766 @default.
- W3174746124 cites W2103082206 @default.
- W3174746124 cites W2104067061 @default.
- W3174746124 cites W2104403548 @default.
- W3174746124 cites W2110284565 @default.
- W3174746124 cites W2110562740 @default.
- W3174746124 cites W2111817932 @default.
- W3174746124 cites W2124324031 @default.
- W3174746124 cites W2130164698 @default.
- W3174746124 cites W2130527528 @default.
- W3174746124 cites W2142918001 @default.
- W3174746124 cites W2146292423 @default.
- W3174746124 cites W2148347826 @default.
- W3174746124 cites W2153048564 @default.
- W3174746124 cites W2155544987 @default.
- W3174746124 cites W2155670397 @default.
- W3174746124 cites W2156905179 @default.
- W3174746124 cites W2157604520 @default.
- W3174746124 cites W2157917411 @default.
- W3174746124 cites W2157952614 @default.
- W3174746124 cites W2159461184 @default.
- W3174746124 cites W2166365370 @default.
- W3174746124 cites W2167635287 @default.
- W3174746124 cites W2216753448 @default.
- W3174746124 cites W2467225246 @default.
- W3174746124 cites W2470237704 @default.
- W3174746124 cites W2480931374 @default.
- W3174746124 cites W2518715366 @default.
- W3174746124 cites W2520926510 @default.
- W3174746124 cites W2528255028 @default.
- W3174746124 cites W2594159061 @default.
- W3174746124 cites W2752616583 @default.
- W3174746124 cites W2756294295 @default.
- W3174746124 cites W2761541545 @default.
- W3174746124 cites W2794043445 @default.
- W3174746124 cites W2798336535 @default.
- W3174746124 cites W2799242196 @default.