Kirsten Knudsen
Kirsten Kraiberg Knudsen's research concerns galaxy formation and evolution and Kirsten focuses in particularly on star forming galaxies at cosmological distances. For the research, she uses large, modern telescopes such as ALMA, VLT, IRAM PdBI, and VLA to study the properties of redshift z=2-7 (lensed) submillimeter galaxies and quasar host galaxies. She receives funding from the VR and KAW as a Wallenberg Academy Fellow and Scholar. She is a former member of the Swedish Young Academy. Kirsten is also vice-head of department for utilization and deputy head of department.
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Showing 83 publications
Gas conditions of a star-formation selected sample in the first billion years
A variable active galactic nucleus at z = 2.06 triply-imaged by the galaxy cluster MACS J0035.4−2015
Big Three Dragons: Molecular Gas in a Bright Lyman-break Galaxy at z = 7.15
The Gas and Stellar Content of a Metal-poor Galaxy at z = 8.496 as Revealed by JWST and ALMA
VLA detects CO(1 0) emission in the z = 3.65 quasar SDSS J160705+533558
Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913
ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z=7.13
Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies
Accurate dust temperature determination in a z = 7.13 galaxy
ALMA Lensing Cluster Survey: A strongly lensed multiply imaged dusty system at z ≥ 6
Measurements of the Dust Properties in z similar or equal to 1-3 Submillimeter Galaxies with ALMA
Detection of H
ALMA detects molecular gas in the halo of the powerful radio galaxy TXS 0828+193
LINESTACKER: A spectral line stacking tool for interferometric data
SMM J04135+10277: a distant QSO-starburst system caught by ALMA
The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): overview and survey description
A spectral stacking analysis to search for faint outflow signatures in z ∼6 quasars
Physical Characterization of an Unlensed, Dusty Star-forming Galaxy at z = 5.85
Panchromatic modeling of the extremely luminous dust-obscured quasars at the cosmic noon
ALMA Detections of CO Emission in the Most Luminous, Heavily Dust-obscured Quasars at z > 3
The Spectral Energy Distribution of the Hyperluminous, Hot Dust-obscured Galaxy W2246-0526
A direct calibration of thtae IRX-β relation in Lyman-break Galaxies at z = 3-5
Measuring size evolution of distant, faint galaxies in the radio regime
The SCUBA-2 850 mu m Follow-up of WISE-selected, Luminous Dust-obscured Quasars
A merger in the dusty, z=7.5 galaxy A1689-zD1?
Evolution of cosmic star formation in the SCUBA-2 Cosmology Legacy Survey
The SCUBA-2 Cosmology Legacy Survey: 850 μm maps, catalogues and number counts
Estimating sizes of faint, distant galaxies in the submillimetre regime
Kiloparsec-Scale Dust Disks in High-Redshift Luminous Submillimeter Galaxies
A resolved map of the infrared excess in a Lyman Break Galaxy at z= 3
C II emission in z similar to 6 strongly lensed, star-forming galaxies
Stacking of Interferometric Data: New Tools for Stacking of ALMA Data
Stacking of SKA data: comparing uv-plane and and image-plane stacking
A dusty, normal galaxy in the epoch of reionization
The SCUBA-2 Cosmology Legacy Survey: the submillimetre properties of Lyman-break galaxies at z=3-5
Shaping ESO2020+ Together: Feedback from the Community Poll
Stacking of large interferometric data sets in the image- and uv-domain - a comparative study
Physical conditions of the gas in an ALMA C II -identified submillimetre galaxy at z=4.44
STAR FORMATION AND GAS KINEMATICS OF QUASAR HOST GALAXIES AT z similar to 6: NEW INSIGHTS FROM ALMA
Herschel-PACS observations of [O I]63 μm towards submillimetre galaxies at z~1
Stacking of interferometric data
Observations of molecules in high redshift galaxies
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Showing 3 research projects
The Origin and Fate of Dust in Our Universe
Galaxy evolution: Tracing the gas fraction of star-forming galaxies
Galaxy evolution: Tracing the cosmic star formation history