Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Reionization, and Astronomy.
REBELS-IFU: dust attenuation curves of 12 massive galaxies at <i>z</i> ≃ 7
The ALMA REBELS survey: obscured star formation in massive Lyman-break galaxies at <i>z</i> <b>=</b> 4–8 revealed by the IRX–β and <i>M</i>⋆ relations
The ALMA REBELS Survey: discovery of a massive, highly star-forming, and morphologically complex ULIRG at <i>z</i> = 7.31
Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z > 6.5 Universe
The ALMA REBELS Survey: cosmic dust temperature evolution out to <i>z</i> ∼ 7
The ALMA REBELS survey: the dust content of <i>z</i> ∼ 7 Lyman break galaxies
The ALMA REBELS Survey: dust continuum detections at <i>z</i> &gt; 6.5
The ALMA REBELS survey: the dust-obscured cosmic star formation rate density at redshift 7
The ALMA REBELS Survey. Epoch of Reionization giants: Properties of dusty galaxies at <i>z</i> ≈ 7
The ALMA REBELS Survey: Average [C ii] 158 μm Sizes of Star-forming Galaxies from z ∼ 7 to z ∼ 4
The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years
UWA Profiles and Research Repository (UWA) 2021cited by 136position: middle
The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy
COLDz: Shape of the CO Luminosity Function at High Redshift and the Cold Gas History of the Universe
Figshare 2019cited by 50position: middle
Rotation in [C ii]-emitting gas in two galaxies at a redshift of 6.8
The CO Luminosity Density at High-z (COLDz) Survey: A Sensitive, Large-area Blind Search for Low-J CO Emission from Cold Gas in the Early Universe with the Karl G. Jansky Very Large Array
THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: CONTINUUM NUMBER COUNTS, RESOLVED 1.2 mm EXTRAGALACTIC BACKGROUND, AND PROPERTIES OF THE FAINTEST DUSTY STAR-FORMING GALAXIES
THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: MOLECULAR GAS RESERVOIRS IN HIGH-REDSHIFT GALAXIES
ALMA OBSERVATION OF 158 µM [CII] LINE AND DUST CONTINUUM OF A Z = 7 NORMALLY STAR-FORMING GALAXY IN THE EPOCH OF REIONIZATION*
2016cited by 91position: middle
CO excitation of normal star-forming galaxies out to<i>z</i>= 1.5 as regulated by the properties of their interstellar medium
ALMA REVEALS THE MOLECULAR MEDIUM FUELING THE NEAREST NUCLEAR STARBURST
CONSTRAINING THE RADIO-LOUD FRACTION OF QUASARS AT<i>z</i>> 5.5
The kiloparsec-scale star formation law at redshift 4: Widespread, highly efficient star formation in the dust-obscured starburst galaxy GN20
Max Planck Institute for Plasma Physics 2015cited by 75position: first
THE SLOAN DIGITAL SKY SURVEY STRIPE 82 IMAGING DATA: DEPTH-OPTIMIZED CO-ADDS OVER 300 deg <sup>2</sup> IN FIVE FILTERS
ALLSMOG: an APEX Low-redshift Legacy Survey for MOlecular Gas – I. Molecular gas scaling relations, and the effect of the CO/H2 conversion factor
Dust and gas in luminous proto-cluster galaxies at<i>z</i>= 4.05: the case for different cosmic dust evolution in normal and starburst galaxies
AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD-SOUTH: THE AGN FRACTION AND X-RAY PROPERTIES OF SUBMILLIMETER GALAXIES
The intense starburst HDF 850.1 in a galaxy overdensity at z ≈ 5.2 in the Hubble Deep Field
The Spitzer Extragalactic Representative Volume Survey (SERVS): Survey Definition and Goals*