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Mar Mezcua

Researcher at Spanish National Research Council

Publications -  51
Citations -  1288

Mar Mezcua is an academic researcher from Spanish National Research Council. The author has contributed to research in topics: Galaxy & Supermassive black hole. The author has an hindex of 15, co-authored 40 publications receiving 1003 citations. Previous affiliations of Mar Mezcua include Harvard University & University of Barcelona.

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Observational evidence for intermediate-mass black holes

TL;DR: Intermediate-mass black holes (IMBHs), with masses in the range 100-106M⊙, are the link between stellar-mass BHs and supermassive BHS (SMBHs) as mentioned in this paper.
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A Candidate Massive Black Hole in the Low-metallicity Dwarf Galaxy Pair Mrk 709

TL;DR: In this paper, high-resolution X-ray and radio observations of the low-metallicity, star-forming, dwarf-galaxy system Mrk 709 with the Chandra Xray Observatory and the Karl G. Jansky Very Large Array are presented.
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A population of intermediate-mass black holes in dwarf starburst galaxies up to redshift = 1.5

TL;DR: In this paper, a sample of 50,000 dwarf starburst and late-type galaxies drawn from the COSMOS survey with the aim of investigating the presence of nuclear accreting black holes (BHs) as those seed BHs from which supermassive BHOs could grow in the early Universe was studied.
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Titans of the early Universe: The Prato statement on the origin of the first supermassive black holes

TL;DR: In this article, the authors present their present understanding of this remarkable formation scenario, based on the discussions held at the Monash Prato Centre from November 20 to 24, 2017, during the workshop "Titans of the Early Universe: The Origin of the First Supermassive Black Holes".
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A population of intermediate-mass black holes in dwarf starburst galaxies up to redshift=1.5

TL;DR: In this paper, a sample of 50,000 dwarf starburst and late-type galaxies drawn from the COSMOS survey with the aim of investigating the presence of nuclear accreting black holes (BHs) as those seed BHs from which supermassive BHOs could grow in the early Universe was studied.