E
E. F. Jiménez-Andrade
Researcher at University of Bonn
Publications - 9
Citations - 332
E. F. Jiménez-Andrade is an academic researcher from University of Bonn. The author has contributed to research in topics: Galaxy & Stellar mass. The author has an hindex of 7, co-authored 9 publications receiving 260 citations. Previous affiliations of E. F. Jiménez-Andrade include University of Cologne & University of Copenhagen.
Papers
More filters
Journal ArticleDOI
Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS). II. Cold Molecular Gas Evolution out to Redshift 6
Daizhong Liu,Eva Schinnerer,Brent Groves,Brent Groves,Benjamin Magnelli,Philipp Lang,Sarah K. Leslie,E. F. Jiménez-Andrade,E. F. Jiménez-Andrade,Dominik A. Riechers,Dominik A. Riechers,Gergö Popping,Gergö Popping,Georgios E. Magdis,Georgios E. Magdis,E. Daddi,Mark Sargent,Yu Gao,Y. Fudamoto,Pascal Oesch,Frank Bertoldi +20 more
TL;DR: In this article, the authors present new measurements of the cosmic cold molecular gas evolution out to redshift 6 based on systematic mining of the ALMA public archive in the COSMOS deep field (A3COSMOSS).
Journal ArticleDOI
Starburst to Quiescent from HST/ALMA: Stars and Dust Unveil Minor Mergers in Submillimeter Galaxies at z ∼ 4.5
Carlos Gómez-Guijarro,Sune Toft,Alexander Karim,Benjamin Magnelli,Georgios E. Magdis,Georgios E. Magdis,E. F. Jiménez-Andrade,E. F. Jiménez-Andrade,E. F. Jiménez-Andrade,Peter Capak,Filippo Fraternali,S. Fujimoto,Dominik A. Riechers,Eva Schinnerer,Vernesa Smolčić,Manuel Aravena,Frank Bertoldi,Isabella Cortzen,Günther Hasinger,E. M. Hu,G. C. Jones,Anton M. Koekemoer,N. Lee,H. J. McCracken,Michał J. Michałowski,F. P. Navarrete,Mirjana Pović,Mirjana Pović,A. Puglisi,Emilio Romano-Diaz,K. Sheth,John D. Silverman,Johannes Staguhn,Johannes Staguhn,Charles L. Steinhardt,Mikkel Stockmann,Masaomi Tanaka,Francesco Valentino,E. van Kampen,Andrew Zirm +39 more
TL;DR: In this article, a detailed spatially resolved study of the stars, dust, and stellar mass in a sample of six submillimeter-bright starburst galaxies at z ≥ 4.5 is presented.
Journal ArticleDOI
Revealing the stellar mass and dust distributions of submillimeter galaxies at Redshift 2.
Philipp Lang,Eva Schinnerer,Ian Smail,U. Dudzevičiūtė,A. M. Swinbank,Daizhong Liu,Sarah K. Leslie,Omar Almaini,Fang Xia An,Fang Xia An,Frank Bertoldi,Andrew Blain,Scott Chapman,Chian-Chou Chen,C. J. Conselice,E. A. Cooke,Kristen Coppin,James Dunlop,Duncan Farrah,Y. Fudamoto,James E. Geach,Bitten Gullberg,K. Harrington,Jacqueline Hodge,Rob Ivison,Rob Ivison,E. F. Jiménez-Andrade,Benjamin Magnelli,Michał J. Michałowski,Pascal Oesch,Douglas Scott,J. M. Simpson,Vernesa Smolčić,S. M. Stach,Alasdair Thomson,Sune Toft,Eleni Vardoulaki,Julie Wardlow,Achim Weiss,P. van der Werf +39 more
TL;DR: In this paper, high-resolution ALMA and HST/CANDELS observations of 20 submillimeter galaxies (SMGs) were combined from the AS2UDS survey at z ≃ 2.
Journal ArticleDOI
Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS): II. Cold Molecular Gas Evolution out to Redshift 6
Daizhong Liu,Eva Schinnerer,Brent Groves,Brent Groves,Benjamin Magnelli,Philipp Lang,Sarah K. Leslie,E. F. Jiménez-Andrade,E. F. Jiménez-Andrade,Dominik A. Riechers,Dominik A. Riechers,Gergö Popping,Gergö Popping,Georgios E. Magdis,Georgios E. Magdis,E. Daddi,Mark Sargent,Yu Gao,Y. Fudamoto,Pascal Oesch,Frank Bertoldi +20 more
TL;DR: In this article, the authors present new measurements of the cosmic cold molecular gas evolution out to redshift 6 based on systematic mining of the ALMA public archive in the COSMOS deep field (A3COSMOSS).
Journal ArticleDOI
Radio continuum size evolution of star-forming galaxies over 0.35 < z < 2.25
E. F. Jiménez-Andrade,Benjamin Magnelli,Alexander Karim,G. Zamorani,M. Bondi,Eva Schinnerer,Mark Sargent,Emilio Romano-Diaz,Mladen Novak,Mladen Novak,Philipp Lang,Frank Bertoldi,Eleni Vardoulaki,Sune Toft,Vernesa Smolčić,K. Harrington,Sarah K. Leslie,J. Delhaize,J. Delhaize,Daizhong Liu,C. Karoumpis,Jeyhan S. Kartaltepe,Anton M. Koekemoer +22 more
TL;DR: In this paper, the authors present the first systematic study of the radio continuum size evolution of star formation in a star formation model and propose a method to better constrain the physical mechanisms driving star formation.