837 citations · 12.2k across the 126 of their papers we have counts for
23 papers · 2 filters
Revealing environmental dependence of molecular gas content in a distant X-ray cluster at z=2.51
Tao Wang, David Elbaz, Emanuele Daddi +13
We present a census of the molecular gas properties of galaxies in the most distant known X-ray cluster, CLJ1001, at z=2.51, using deep observations of CO(1-0) with JVLA. In total…
The Effect of Galaxy Interactions on Molecular Gas Properties
Hsi-An Pan, Lihwai Lin, Bau-Ching Hsieh +26
Galaxy interactions are often accompanied by an enhanced star formation rate (SFR). Since molecular gas is essential for star formation, it is vital to establish whether, and by ho…
Science with an ngVLA: New Parameter Space for Deep Field Radio Continuum Surveys
Amy J. Barger, Kotaro Kohno, Eric J. Murphy +2
Deep continuum surveys at radio wavelengths are able to cover large areas, yield high angular resolution, and do not suffer from dust extinction, thus providing a robust way to mea…
Science with an ngVLA. Cold gas in High-z Galaxies: CO as redshift beacon
R. Decarli, C. Carilli, C. Casey +7
The goal of this science case is to address the use of a ngVLA as a CO redshift machine for dust-obscured high-redshift galaxies which lack of clear counterparts at other wavelengt…
Science with an ngVLA: Radio Continuum Emission from Galaxies: An Accounting of Energetic Processes
Eric J. Murphy, James J. Condon, Antxon Alberdi +14
Radio continuum observations have proven to be a workhorse in our understanding of the star formation process (i.e., stellar birth and death) from galaxies both in the nearby unive…
The molecular gas content and fuel efficiency of starbursts at z ~ 1.6 with ALMA
J. Silverman, W. Rujopakarn, E. Daddi +17
We present an analysis of the molecular gas properties, based on CO(2 - 1) emission, of twelve starburst galaxies at z~1.6 selected by having a boost (>~4x) in their star formation…
Concurrent starbursts in molecular gas disks within a pair of colliding galaxies at z = 1.52
J. Silverman, E. Daddi, W. Rujopakarn +20
We report on the discovery of a merger-driven starburst at z = 1.52, PACS-787, based on high signal-to-noise ALMA observations. CO(5-4) and continuum emission (850um) at a spatial…
Morphological evolution and galactic sizes in the L-Galaxies SA model
Dimitrios Irodotou, Peter A. Thomas, Bruno M. Henriques +2
In this work we update the L-Galaxies semi-analytic model (SAM) to better follow the physical processes responsible for the growth of bulges via disc instabilities (leading to pseu…
JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: I. Survey overview and first results
Amelie Saintonge, Christine D. Wilson, Ting Xiao +88
JINGLE is a new JCMT legacy survey designed to systematically study the cold interstellar medium of galaxies in the local Universe. As part of the survey we perform 850um continuum…
Early- and late-stage mergers among main sequence and starburst galaxies at 0.2<z<2
A. Cibinel, E. Daddi, M. T. Sargent +12
We investigate the fraction of close pairs and morphologically identified mergers on and above the star-forming main sequence (MS) at 0.22.0. The novelty of our work li…
The [C II] emission as a molecular gas mass tracer in galaxies at low and high redshift
A. Zanella, E. Daddi, G. Magdis +19
We present ALMA Band 9 observations of the [C II]158um emission for a sample of 10 main-sequence galaxies at redshift z ~ 2, with typical stellar masses (log M*/Msun ~ 10.0 - 10.9)…
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
Riccardo Pavesi, Chelsea E. Sharon, Dominik A. Riechers +16
We describe the CO Luminosity Density at High-z (COLDz) survey, the first spectral line deep field targeting CO(1-0) emission from galaxies at and CO(2-1) at $z=4.91-…
COLDz: Shape of the CO Luminosity Function at High Redshift and the Cold Gas History of the Universe
Dominik A. Riechers, Riccardo Pavesi, Chelsea E. Sharon +14
We report the first detailed measurement of the shape of the CO luminosity function at high redshift, based on 320 hr of the NSF's Karl G. Jansky Very Large Array (VLA) observat…
"Super-deblended" Dust Emission in Galaxies: II. Far-IR to (sub)millimeter photometry and high redshift galaxy candidates in the full COSMOS field
Shuowen Jin, Emanuele Daddi, Daizhong Liu +17
We present a "super-deblended" far-infrared to (sub)millimeter photometric catalog in the Cosmic Evolution Survey (COSMOS), prepared with the method recently developed by Liu et al…
The molecular gas content in obscured AGN at z > 1
M. Perna, M. T. Sargent, M. Brusa +11
The standard AGN-galaxy co-evolutionary scenario predicts a phase of deeply buried supermassive black hole growth coexisting with a starburst (SB) before feedback phenomena deplete…
Merger driven star-formation activity in Cl J1449+0856 at z=1.99 as seen by ALMA and JVLA
R. T. Coogan, E. Daddi, M. T. Sargent +13
We use ALMA and JVLA observations of the galaxy cluster Cl J1449+0856 at z=1.99, in order to study how dust-obscured star-formation, ISM content and AGN activity are linked to envi…
Probing star formation and ISM properties using galaxy disk inclination II: Testing typical FUV attenuation corrections out to z0.7
S. K. Leslie, E. Schinnerer, B. Groves +4
We evaluate dust-corrected far ultraviolet (FUV) star formation rates (SFRs) for samples of star-forming galaxies at and and find significant differences betwee…
Revolutionizing Our Understanding of AGN Feedback and its Importance to Galaxy Evolution in the Era of the Next Generation Very Large Array
Kristina Nyland, Jeremy J. Harwood, Dipanjan Mukherjee +19
Energetic feedback by Active Galactic Nuclei (AGNs) plays an important evolutionary role in the regulation of star formation (SF) on galactic scales. However, the effects of this f…
GOODS-ALMA: 1.1 mm galaxy survey - I. Source catalogue and optically dark galaxies
M. Franco, D. Elbaz, M. Béthermin +36
We present a 69 arcmin ALMA survey at 1.1mm, GOODS-ALMA, matching the deepest HST-WFC3 H-band part of the GOODS-South field. We taper the 0"24 original image with a homogeneous…
Galaxy pairs in the SDSS - XIII. The connection between enhanced star formation and molecular gas properties in galaxy mergers
Giulio Violino, Sara L. Ellison, Mark Sargent +4
We investigate the connection between star formation and molecular gas properties in galaxy mergers at low redshift (z0.06). The study we present is based on IRAM 30-m CO(1-0…
Molecular outflow and feedback in the obscured Quasar XID2028 revealed by ALMA
M. Brusa, G. Cresci, E. Daddi +29
We imaged with ALMA and ARGOS/LUCI the molecular gas and the dust and stellar continuum in XID2028, an obscured QSO at z=1.593, where the presence of a massive outflow in the ioniz…
Red, redder, reddest: SCUBA-2 imaging of colour-selected \textit{Herschel} sources
S. Duivenvoorden, S. Oliver, J. M. Scudder +28
High-redshift, luminous, dusty star forming galaxies (DSFGs) constrain the extremity of galaxy formation theories. The most extreme are discovered through follow-up on candidates i…
Probing star formation and ISM properties using galaxy disk inclination I: Evolution in disk opacity since
S. K. Leslie, M. T. Sargent, E. Schinnerer +6
Disk galaxies at intermediate redshift () have been found in previous work to display more optically thick behaviour than their local counterparts in the rest-frame B-ban…