“Guernica” artist

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Possible Answers: PICASSO.

Last seen on: NY Times Crossword 10 Jul 2018, Tuesday

Random information on the term ““Guernica” artist”:

E (named e /iː/, plural ees)[1] is the fifth letter and the second vowel in the modern English alphabet and the ISO basic Latin alphabet. It is the most commonly used letter in many languages, including Czech, Danish, Dutch, English, French, German, Hungarian, Latin, Latvian, Norwegian, Spanish, and Swedish.[2][3][4][5][6]

The Latin letter ‘E’ differs little from its source, the Greek letter epsilon, ‘Ε’. This in turn comes from the Semitic letter hê, which has been suggested to have started as a praying or calling human figure (hillul ‘jubilation’), and was probably based on a similar Egyptian hieroglyph that indicated a different pronunciation. In Semitic, the letter represented /h/ (and /e/ in foreign words); in Greek, hê became the letter epsilon, used to represent /e/. The various forms of the Old Italic script and the Latin alphabet followed this usage.

Although Middle English spelling used ⟨e⟩ to represent long and short /e/, the Great Vowel Shift changed long /eː/ (as in ‘me’ or ‘bee’) to /iː/ while short /ɛ/ (as in ‘met’ or ‘bed’) remained a mid vowel. In other cases, the letter is silent, generally at the end of words.

“Guernica” artist on Wikipedia

Random information on the term “PICASSO”:

In astronomy and cosmology, baryonic dark matter is dark matter composed of baryons. Only a small proportion of the dark matter in the universe is likely to be baryonic.

As “dark matter”, baryonic dark matter is undetectable by its emitted radiation, but its presence can be inferred from gravitational effects on visible matter. This form of dark matter is composed of “baryons”, heavy subatomic particles such as protons and neutrons and combinations of these, including non-emitting ordinary atoms.

Baryonic dark matter may occur in non-luminous gas or in Massive Astrophysical Compact Halo Objects (MACHOs) – condensed objects such as black holes, neutron stars, white dwarfs, very faint stars, or non-luminous objects like planets and brown dwarfs.

The total amount of baryonic dark matter can be inferred from models of Big Bang nucleosynthesis, and observations of the cosmic microwave background. Both indicate that the amount of baryonic dark matter is much smaller than the total amount of dark matter.

PICASSO on Wikipedia