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91 papers
New methods for ALMA angular-scale based observation scheduling, quality assessment, and beam shaping II: refinements
Dirk Petry, María Díaz Trigo, Rüdiger Kneissl +5
The Atacama Large Millimeter/submillimeter Array remains the largest mm radio interferometer observatory world-wide. It is now conducting its 11th observing cycle. In our previous…
JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noon
M. Polletta, B. L. Frye, N. Garuda +35
Dusty star-forming galaxies (DSFGs) contribute significantly to the stellar buildup at cosmic noon. Major mergers and gas accretion are often invoked to explain DSFGs' prodigious s…
Molecular gas properties of Planck-selected protocluster candidates at z~1.3-3
M. Polletta, H. Dole, C. Martinache +3
We report on IRAM-30m/EMIR observations of 38 red Herschel sources in 18 Planck-selected protocluster candidates (PHz). We detect 40 CO lines on a total of 24 bright Herschel sourc…
An ACA 1mm survey of HzRGs in the ELAIS-S1: survey description and first results
Hugo Messias, Evanthia Hatziminaoglou, Pascale Hibon +16
Radio-emitting jets might be one of the main ingredients shaping the evolution of massive galaxies in the Universe since early cosmic times. However, identifying early radio active…
Confirming ALMA Calibration using Planck and ACT Observations
Gerrit S. Farren, Bruce Partridge, Rüdiger Kneissl +4
We test the accuracy of ALMA flux density calibration by comparing ALMA flux density measurements of extragalactic sources to measurements made by the Planck mission; Planck is abs…
New methods for ALMA angular-scale based observation scheduling, quality assessment, and beam shaping
Dirk Petry, María Díaz Trigo, Rüdiger Kneissl +2
Up to now, the completion of an ALMA interferometric observation is determined based on the achievement of a given shape and size of the synthesized beam and the noise RMS in the r…