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| Query : 2018MNRAS.476.1445G |
2018MNRAS.476.1445G - Mon. Not. R. Astron. Soc., 476, 1445-1469 (2018/May-2)
A dust spectral energy distribution model with hierarchical Bayesian inference - I. Formalism and benchmarking.
GALLIANO F.
Abstract (from CDS):
Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): methods: data analysis - methods: numerical - methods: statistical - dust, extinction - infrared: galaxies - infrared: ISM
Simbad objects: 3
| Number of rows : 3 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | IC 10 | rG | 00 20 17.33520 | +59 18 13.6480 | 13.6 | 9.5 | ~ | 1185 | 1 | |||
| 2 | NAME Magellanic Clouds | GrG | 03 00 | -71.0 | ~ | 7988 | 0 | |||||
| 3 | NGC 3372 | HII | 10 45 02.23 | -59 41 59.8 | ~ | 1071 | 2 |
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