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It also had the brightest UVOT afterglow ever recorded once corrected for extinction. [46] It had the largest amount of energy ever recorded in the TeV range, [47] and had the most energetic photons ever recorded for a GRB, peaking at 18 TeV. [25] [20] The burst was ten times brighter than any previous GRB detected by the Swift mission. [48]
The brightest known quasars devour 1000 solar masses of material every year (equivalent to 10 Earths per second). Quasar luminosities can vary considerably over time, depending on their surroundings. Since it is difficult to fuel quasars for many billions of years, after a quasar finishes accreting the surrounding gas and dust, it becomes an ...
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No, a 1040 is not the same as a W-2, but you use the information included on a W-2 to complete the 1040 form. A W-2 is the form employers use to report the wages paid to an employee during the year.
R.I.P. Tho: Guest Book pp. 56-60 This chapter offers postings on the Elsie Blitz obituary page that originate all over the United States and Internationally, including India, Hong Kong and Sweden. The comment from her son, Moses, is among the posts, including the declaration that “ELSIE WAS A #SHITTYMOTHER.”
C/2014 UN 271 (Bernardinelli–Bernstein), simply known as C/2014 UN 271 or Comet Bernardinelli–Bernstein (nicknamed BB), [3] is a large Oort cloud comet discovered by astronomers Pedro Bernardinelli and Gary Bernstein in archival images from the Dark Energy Survey.
First discovered with giant planet(s) Gliese 876: 1998 Gliese 876 b: The giant planet was the first planet discovered around a red dwarf. [2] [3] First discovered with terrestrial planet(s) Kepler-42 : 2012 KOI-961 b KOI-961 c KOI-961 d: 3 terrestrial planets were discovered around KOI-961 in 2012, the first terrestrial planets found to orbit a ...
The object itself was detected in ESO images dating back to 1980, but its identification as a quasar occurred only several decades later. [2]An automated analysis of 2022 data from the European Space Agency's Gaia satellite did not confirm J0529-4351 as too bright to be a quasar, and suggested it was a 16th magnitude star with a 99.98% probability.