361 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR107 papers
- The University of TokyoJP88 papers
- Chulalongkorn UniversityTH85 papers
- University of SheffieldGB71 papers
- Chinese Academy of SciencesCN70 papers
- Instituto de Astrofísica de CanariasES70 papers
- University of WarwickGB64 papers
- Kavli Institute for the Physics and Mathematics of the UniverseJP61 papers
- California Institute of TechnologyUS56 papers
- National Astronomical Observatory of JapanJP55 papers
- University of ManchesterGB55 papers
- Sorbonne UniversitéFR48 papers
9 papers · 2 filters
Evolution of the Stellar Mass-Metallicity Relation. II. Constraints on Galactic Outflows from the Mg Abundances of Quiescent Galaxies
Nicha Leethochawalit, Evan N. Kirby, Richard S. Ellis +2
We present the stellar mass-[Fe/H] and mass-[Mg/H] relation of quiescent galaxies in two galaxy clusters at and . We derive the age, [Fe/H], and [Mg/Fe] for…
Molecular clouds in the Cosmic Snake normal star-forming galaxy 8 billion years ago
Miroslava Dessauges-Zavadsky, Johan Richard, Françoise Combes +12
The cold molecular gas in contemporary galaxies is structured in discrete cloud complexes. These giant molecular clouds (GMCs), with - solar masses and radii of 5-100 p…
MOS spectroscopy of protocluster candidate galaxies at z=6.5
Rosa Calvi, José Miguel Rodríguez Espinosa, José Miguel Mas-Hesse +7
The epoch corresponding to a redshift of z is close to full re-ionisation of the Universe, and early enough to provide an intriguing environment to observe the early sta…
No signs of star formation being regulated in the most luminous quasars at z~2 with ALMA
A. Schulze, J. D. Silverman, E. Daddi +7
We present ALMA Band~7 observations at m of 20 luminous ( [erg s]) unobscured quasars at . We detect continuum emission for 19/20 quas…
AGN in Dusty Starbursts at Z=2: Feedback Still To Kick In
G. Rodighiero, A. Enia, I. Delvecchio +18
We investigate a sample of 152 dusty sources at 1:5 < z < 2:5 to understand the connection of enhanced Star-Formation-Rate (SFR) and Black-Hole-Accretion-Rate (BHAR). The sources a…
Radio spectra and sizes of ALMA-identified submillimetre galaxies: evidence of age-related spectral curvature and cosmic ray diffusion?
A. P. Thomson, Ian Smail, A. M. Swinbank +21
We analyse the multi-frequency radio spectral properties of 6GHz-detected ALMA-identified, submillimetre galaxies (SMGs), observed at 610MHz, 1.4GHz, 6GHz with GMRT and the VL…
ALMA 200-parsec Resolution Imaging of Smooth Cold Dusty Disks in Typical Star-Forming Galaxies
W. Rujopakarn, E. Daddi, G. H. Rieke +14
We present high-fidelity, 30 milliarcsecond (200-pc) resolution ALMA rest-frame 240 m observations of cold dust emission in three typical main-sequence star-forming galaxies (SF…
ALMA twenty-six arcmin survey of GOODS-S at one-millimeter (ASAGAO): Near-infrared-dark faint ALMA sources
Yuki Yamaguchi, Kotaro Kohno, Bunyo Hatsukade +21
We report detections of two 1.2 mm continuum sources ( ~ 0.6 mJy) without any counterparts in the deep - and/or -band image (i.e., -band magnitude $\gtrs…
HI-MaNGA: HI Followup for the MaNGA Survey
Karen L. Masters, David V. Stark, Zachary J. Pace +16
We present the HI-MaNGA programme of HI follow-up for the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey. MaNGA, which is part of the Fourth phase of the Sloan…