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D. Ceverino

Identifiers

  • name variant D. Ceverino 0.60 · backfill

Papers (11)

  1. High-ionization coronal lines trace quasar-like activity in recently quenched galaxies at high redshift astro-ph.GA · 2026 · author #18
  2. Extremely UV-bright starbursts at the end of cosmic reionization astro-ph.GA · 2025 · author #13
  3. CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism: dependence on redshift, halo mass and radius astro-ph.GA · 2018 · author #6
  4. Deep Learning Identifies High-z Galaxies in a Central Blue Nugget Phase in a Characteristic Mass Range astro-ph.GA · 2018 · author #6
  5. A universal structural and star-forming relation since $z\sim3$: connecting compact star-forming and quiescent galaxies astro-ph.GA · 2015 · author #14
  6. Caught in the act: gas and stellar velocity dispersions in a fast quenching compact star-forming galaxy at z~1.7 astro-ph.GA · 2015 · author #17
  7. Geometry of Star-Forming Galaxies from SDSS, 3D-HST and CANDELS astro-ph.GA · 2014 · author #15
  8. Keck-I MOSFIRE spectroscopy of compact star-forming galaxies at z$\gtrsim$2: High velocity dispersions in progenitors of compact quiescent galaxies astro-ph.GA · 2014 · author #16
  9. CANDELS+3D-HST: compact SFGs at z~2-3, the progenitors of the first quiescent galaxies astro-ph.CO · 2013 · author #16
  10. Toy Models for Galaxy Formation versus Simulations astro-ph.CO · 2013 · author #5
  11. The SINS survey of z~2 galaxy kinematics: properties of the giant star forming clumps astro-ph.CO · 2010 · author #15

Mentions

  • 1509.00469 #14 · backfill · confidence 0.70 D. Ceverino
  • 1503.07164 #17 · backfill · confidence 0.70 D. Ceverino
  • 2605.30424 #18 · arxiv_oai · confidence 0.70 D. Ceverino
  • 1407.4233 #15 · backfill · confidence 0.70 D. Ceverino
  • 1405.7042 #16 · backfill · confidence 0.70 D. Ceverino
  • 1311.5559 #16 · backfill · confidence 0.70 D. Ceverino
  • 1303.3009 #5 · backfill · confidence 0.70 D. Ceverino
  • 2510.12411 #13 · arxiv_oai · confidence 0.70 D. Ceverino
  • 1011.5360 #15 · backfill · confidence 0.70 D. Ceverino

Frequent Coauthors