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• W3112464939 endingPage "2676" @default.
• W3112464939 startingPage "2659" @default.
• W3112464939 abstract "We study structural properties of spectroscopically confirmed massive quiescent galaxies at $zapprox 3$ with one of the first sizeable samples of such sources, made of ten $10.8<log(M_{star}/M_{odot})<11.3$ galaxies at $2.4 < z < 3.2$ in the COSMOS field whose redshifts and quiescence are confirmed by HST grism spectroscopy. Although affected by a weak bias toward younger stellar populations, this sample is deemed to be largely representative of the majority of the most massive and thus intrinsically rarest quiescent sources at this cosmic time. We rely on targeted HST/WFC3 observations and fit S'ersic profiles to the galaxy surface brightness distributions at $approx 4000$ angstrom restframe. We find typically high S'ersic indices and axis ratios (medians $approx 4.5$ and $0.73$, respectively) suggesting that, at odds with some previous results, the first massive quiescent galaxies may largely be already bulge-dominated systems. We measure compact galaxy sizes with an average of $approx 1.4$kpc at $log(M_{star}/M_{odot})approx 11.2$, in good agreement with the extrapolation at the highest masses of previous determinations of the stellar mass - size relation of quiescent galaxies, and of its redshift evolution, from photometrically selected samples at lower and similar redshifts. This work confirms the existence of a population of compact, bulge dominated, massive, quiescent sources at $zapprox 3$, providing one of the first statistical estimates of their structural properties, and further constraining the early formation and evolution of the first quiescent galaxies." @default.
• W3112464939 created "2020-12-21" @default.
• W3112464939 creator A5000847197 @default.
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• W3112464939 date "2020-12-05" @default.
• W3112464939 modified "2023-10-16" @default.
• W3112464939 title "Compact, bulge-dominated structures of spectroscopically confirmed quiescent galaxies at <i>z</i> ≈ 3" @default.
• W3112464939 cites W1874935544 @default.
• W3112464939 cites W1913812026 @default.
• W3112464939 cites W1917783267 @default.
• W3112464939 cites W1929330687 @default.
• W3112464939 cites W1963611021 @default.
• W3112464939 cites W1964280853 @default.
• W3112464939 cites W1965907382 @default.
• W3112464939 cites W1970196846 @default.
• W3112464939 cites W1971031790 @default.
• W3112464939 cites W1971770935 @default.
• W3112464939 cites W1972763344 @default.
• W3112464939 cites W1973637537 @default.
• W3112464939 cites W1977361870 @default.
• W3112464939 cites W1978007991 @default.
• W3112464939 cites W1979789803 @default.
• W3112464939 cites W1980247466 @default.
• W3112464939 cites W1982330764 @default.
• W3112464939 cites W1986834411 @default.
• W3112464939 cites W1992635601 @default.
• W3112464939 cites W1992923622 @default.
• W3112464939 cites W1994671833 @default.
• W3112464939 cites W1995667613 @default.
• W3112464939 cites W1996537612 @default.
• W3112464939 cites W2000187183 @default.
• W3112464939 cites W2001085255 @default.
• W3112464939 cites W2001429078 @default.
• W3112464939 cites W2001717952 @default.
• W3112464939 cites W2004084407 @default.
• W3112464939 cites W2012886609 @default.
• W3112464939 cites W2014220424 @default.
• W3112464939 cites W2017719673 @default.
• W3112464939 cites W2018388366 @default.
• W3112464939 cites W2019293240 @default.
• W3112464939 cites W2020747414 @default.
• W3112464939 cites W2025020969 @default.
• W3112464939 cites W2025819094 @default.
• W3112464939 cites W2026067461 @default.
• W3112464939 cites W2031617522 @default.
• W3112464939 cites W2031942083 @default.
• W3112464939 cites W2032317739 @default.
• W3112464939 cites W2033300749 @default.
• W3112464939 cites W2033803356 @default.
• W3112464939 cites W2042022217 @default.
• W3112464939 cites W2042181581 @default.
• W3112464939 cites W2042262980 @default.
• W3112464939 cites W2042369320 @default.
• W3112464939 cites W2043298374 @default.
• W3112464939 cites W2051805380 @default.
• W3112464939 cites W2051907193 @default.
• W3112464939 cites W2053827460 @default.
• W3112464939 cites W2060753691 @default.
• W3112464939 cites W2063375039 @default.
• W3112464939 cites W2069396164 @default.
• W3112464939 cites W2070887798 @default.
• W3112464939 cites W2074106980 @default.
• W3112464939 cites W2075056822 @default.
• W3112464939 cites W2075414028 @default.
• W3112464939 cites W2079227246 @default.
• W3112464939 cites W2079304679 @default.
• W3112464939 cites W2083761364 @default.
• W3112464939 cites W2084091264 @default.
• W3112464939 cites W2085395258 @default.
• W3112464939 cites W2089191176 @default.
• W3112464939 cites W2090046995 @default.
• W3112464939 cites W2092121483 @default.
• W3112464939 cites W2092458937 @default.
• W3112464939 cites W2093697839 @default.
• W3112464939 cites W2094305767 @default.
• W3112464939 cites W2100677756 @default.
• W3112464939 cites W2103734248 @default.
• W3112464939 cites W2107308864 @default.
• W3112464939 cites W2109329782 @default.
• W3112464939 cites W2110974947 @default.
• W3112464939 cites W2112633422 @default.
• W3112464939 cites W2118277889 @default.
• W3112464939 cites W2118921616 @default.
• W3112464939 cites W2120241018 @default.
• W3112464939 cites W2128904482 @default.
• W3112464939 cites W2135052708 @default.
• W3112464939 cites W2136644880 @default.
• W3112464939 cites W2142238829 @default.
• W3112464939 cites W2145086822 @default.

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