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The [[space observatory|spacecraft's]] mission was to observe hundreds of thousands of galaxies, with the goal of determining the distance of each galaxy from [[Earth]] and the rate of [[star formation]] in each galaxy. Near-UV (NUV) and Far-UV (FUV) emissions as measured by GALEX can indicate the presence of young stars, but may also originate from old stellar populations (e.g. [[sdB stars]]). |
The [[space observatory|spacecraft's]] mission was to observe hundreds of thousands of galaxies, with the goal of determining the distance of each galaxy from [[Earth]] and the rate of [[star formation]] in each galaxy. Near-UV (NUV) and Far-UV (FUV) emissions as measured by GALEX can indicate the presence of young stars, but may also originate from old stellar populations (e.g. [[sdB stars]]). |
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Partnering with the NASA [[Jet Propulsion Laboratory]] (JPL) on the mission were the [[California Institute of Technology]], [[Orbital Sciences Corporation]], [[University of California, Berkeley]], [[Yonsei University]], [[Johns Hopkins University]], [[Columbia University]], and [[ |
Partnering with the NASA [[Jet Propulsion Laboratory]] (JPL) on the mission were the [[California Institute of Technology]], [[Orbital Sciences Corporation]], [[University of California, Berkeley]], [[Yonsei University]], [[Johns Hopkins University]], [[Columbia University]], and [[Laboratoire d'Astrophysique de Marseille, France]]. |
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The observatory participated in GOALS with [[Spitzer Space Telescope]], [[Chandra X-ray Observatory]], and [[Hubble Space Telescope]].<ref name=goals>[https://arxiv.org/abs/0904.4498 GOALS: The Great Observatories All-Sky LIRG Survey]</ref> GOALS stands for ''Great Observatories All-sky LIRG Survey'', and [[Luminous Infrared Galaxies]] were studied at the multiple wavelengths allowed by the telescopes.<ref name=goals/> |
The observatory participated in GOALS with [[Spitzer Space Telescope]], [[Chandra X-ray Observatory]], and [[Hubble Space Telescope]].<ref name=goals>[https://arxiv.org/abs/0904.4498 GOALS: The Great Observatories All-Sky LIRG Survey]</ref> GOALS stands for ''Great Observatories All-sky LIRG Survey'', and [[Luminous Infrared Galaxies]] were studied at the multiple wavelengths allowed by the telescopes.<ref name=goals/> |
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Latin: A a Á á À à  â Ä ä Ǎ ǎ Ă ă Ā ā à ã Å å Ą ą Æ æ Ǣ ǣ B b C c Ć ć Ċ ċ Ĉ ĉ Č č Ç ç D d Ď ď Đ đ Ḍ ḍ Ð ð E e É é È è Ė ė Ê ê Ë ë Ě ě Ĕ ĕ Ē ē Ẽ ẽ Ę ę Ẹ ẹ Ɛ ɛ Ǝ ǝ Ə ə F f G g Ġ ġ Ĝ ĝ Ğ ğ Ģ ģ H h Ĥ ĥ Ħ ħ Ḥ ḥ I i İ ı Í í Ì ì Î î Ï ï Ǐ ǐ Ĭ ĭ Ī ī Ĩ ĩ Į į Ị ị J j Ĵ ĵ K k Ķ ķ L l Ĺ ĺ Ŀ ŀ Ľ ľ Ļ ļ Ł ł Ḷ ḷ Ḹ ḹ M m Ṃ ṃ N n Ń ń Ň ň Ñ ñ Ņ ņ Ṇ ṇ Ŋ ŋ O o Ó ó Ò ò Ô ô Ö ö Ǒ ǒ Ŏ ŏ Ō ō Õ õ Ǫ ǫ Ọ ọ Ő ő Ø ø Œ œ Ɔ ɔ P p Q q R r Ŕ ŕ Ř ř Ŗ ŗ Ṛ ṛ Ṝ ṝ S s Ś ś Ŝ ŝ Š š Ş ş Ș ș Ṣ ṣ ß T t Ť ť Ţ ţ Ț ț Ṭ ṭ Þ þ U u Ú ú Ù ù Û û Ü ü Ǔ ǔ Ŭ ŭ Ū ū Ũ ũ Ů ů Ų ų Ụ ụ Ű ű Ǘ ǘ Ǜ ǜ Ǚ ǚ Ǖ ǖ V v W w Ŵ ŵ X x Y y Ý ý Ŷ ŷ Ÿ ÿ Ỹ ỹ Ȳ ȳ Z z Ź ź Ż ż Ž ž ß Ð ð Þ þ Ŋ ŋ Ə ə
Greek: Ά ά Έ έ Ή ή Ί ί Ό ό Ύ ύ Ώ ώ Α α Β β Γ γ Δ δ Ε ε Ζ ζ Η η Θ θ Ι ι Κ κ Λ λ Μ μ Ν ν Ξ ξ Ο ο Π π Ρ ρ Σ σ ς Τ τ Υ υ Φ φ Χ χ Ψ ψ Ω ω {{Polytonic|}}
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