PATT Linked Grant for the Durham Astrophysics Group 2014-16
Lead Research Organisation:
Durham University
Department Name: Physics
Abstract
The Durham observational astronomers are among the most successful at obtaining telescope time at observatories around the world. This grant for travel funds is to ensure that the observers have an administratively simple source of funds to be present at the telescope to execute their observations.
Publications
Rawle T
(2014)
[C II] AND 12 CO(1-0) EMISSION MAPS IN HLSJ091828.6+514223: A STRONGLY LENSED INTERACTING SYSTEM AT z = 5.24
in The Astrophysical Journal
McNamara B
(2014)
A 10 10 SOLAR MASS FLOW OF MOLECULAR GAS IN THE A1835 BRIGHTEST CLUSTER GALAXY
in The Astrophysical Journal
Hogan M
(2015)
A comprehensive study of the radio properties of brightest cluster galaxies
in Monthly Notices of the Royal Astronomical Society
An F
(2018)
A Machine-learning Method for Identifying Multiwavelength Counterparts of Submillimeter Galaxies: Training and Testing Using AS2UDS and ALESS
in The Astrophysical Journal
McNamara B
(2016)
A MECHANISM FOR STIMULATING AGN FEEDBACK BY LIFTING GAS IN MASSIVE GALAXIES
in The Astrophysical Journal
Stott J
(2014)
A relationship between specific star formation rate and metallicity gradient within z ~ 1 galaxies from KMOS-HiZELS
in Monthly Notices of the Royal Astronomical Society
Stanley F
(2015)
A remarkably flat relationship between the average star formation rate and AGN luminosity for distant X-ray AGN
in Monthly Notices of the Royal Astronomical Society
Geach J
(2014)
A SUBMILLIMETER GALAXY ILLUMINATING ITS CIRCUMGALACTIC MEDIUM: Lya SCATTERING IN A COLD, CLUMPY OUTFLOW
in The Astrophysical Journal
Alexander D
(2016)
ALMA observations of a z ˜ 3.1 protocluster: star formation from active galactic nuclei and Lyman-alpha blobs in an overdense environment
in Monthly Notices of the Royal Astronomical Society
Geach J
(2016)
ALMA OBSERVATIONS OF Ly a BLOB 1: HALO SUBSTRUCTURE ILLUMINATED FROM WITHIN
in The Astrophysical Journal
Stach S
(2017)
ALMA Pinpoints a Strong Overdensity of U/LIRGs in the Massive Cluster XCS J2215 at z = 1.46
in The Astrophysical Journal
Danielson A
(2017)
An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Spectroscopic Redshifts
in The Astrophysical Journal
Simpson J
(2014)
AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: THE REDSHIFT DISTRIBUTION AND EVOLUTION OF SUBMILLIMETER GALAXIES
in The Astrophysical Journal
Thomson A
(2014)
An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: radio properties and the far-infrared/radio correlation
in Monthly Notices of the Royal Astronomical Society
Simpson J
(2020)
An ALMA survey of the brightest sub-millimetre sources in the SCUBA-2-COSMOS field
in Monthly Notices of the Royal Astronomical Society
Smail I
(2021)
An ALMA survey of the S2CLS UDS field: optically invisible submillimetre galaxies
in Monthly Notices of the Royal Astronomical Society
Van der Werf P
(2020)
An ALMA survey of the SCUBA-2 CLS UDS field: physical properties of 707 sub-millimetre galaxies
in Monthly Notices of the Royal Astronomical Society
Dudzevi
(2019)
An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 Sub-millimetre Galaxies
in arXiv e-prints
Koprowski M
(2020)
An ALMA survey of the SCUBA-2 cosmology legacy survey UKIDSS/UDS field: Dust attenuation in high-redshift Lyman-break galaxies
in Monthly Notices of the Royal Astronomical Society
Gullberg B
(2019)
An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: high-resolution dust continuum morphologies and the link between sub-millimetre galaxies and spheroid formation
in Monthly Notices of the Royal Astronomical Society
Cooke E
(2018)
An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: Identifying Candidate z ~ 4.5 [C II] Emitters
in The Astrophysical Journal
Stach S
(2018)
An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: Number Counts of Submillimeter Galaxies
in The Astrophysical Journal
Stach S
(2019)
An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: source catalogue and properties
in Monthly Notices of the Royal Astronomical Society
Algera H
(2020)
An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: The Far-infrared/Radio Correlation for High-redshift Dusty Star-forming Galaxies
in The Astrophysical Journal
Stach S. M.
(2021)
An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
in arXiv e-prints
Swinbank A. M.
(2017)
Angular momentum evolution of galaxies over the past 10 Gyr: A MUSE and KMOS dynamical survey of 400 star-forming galaxies from z = 0.3-1.7
in Monthly Notices of the Royal Astronomical Society
Swinbank A
(2017)
Angular momentum evolution of galaxies over the past 10 Gyr: A MUSE and KMOS dynamical survey of 400 star-forming galaxies from $z$ = 0.3-1.7
in Monthly Notices of the Royal Astronomical Society
Lansbury G
(2014)
Barred S0 galaxies in the Coma cluster
in Monthly Notices of the Royal Astronomical Society
Banerji M
(2015)
Cold dust emission from X-ray AGN in the SCUBA-2 Cosmology Legacy Survey: dependence on luminosity, obscuration and AGN activity
in Monthly Notices of the Royal Astronomical Society
Tremblay GR
(2016)
Cold, clumpy accretion onto an active supermassive black hole.
in Nature
Head J
(2014)
Dissecting the red sequence: the bulge and disc colours of early-type galaxies in the Coma cluster
in Monthly Notices of the Royal Astronomical Society
Fabian A
(2015)
Effects of the variability of the nucleus of NGC 1275 on X-ray observations of the surrounding intracluster medium
in Monthly Notices of the Royal Astronomical Society
Mackenzie R
(2017)
Evidence against a supervoid causing the CMB Cold Spot
in Monthly Notices of the Royal Astronomical Society
Chen (???) C
(2016)
FAINT SUBMILLIMETER GALAXIES IDENTIFIED THROUGH THEIR OPTICAL/NEAR-INFRARED COLORS. I. SPATIAL CLUSTERING AND HALO MASSES
in The Astrophysical Journal
Mitsuhashi I
(2021)
FIR-luminous [C ii] Emitters in the ALMA-SCUBA-2 COSMOS Survey (AS2COSMOS): The Nature of Submillimeter Galaxies in a 10 Comoving Megaparsec-scale Structure at z ~ 4.6
in The Astrophysical Journal
Gunawardhana M
(2015)
Galaxy And Mass Assembly (GAMA): bivariate functions of Ha star-forming galaxies
in Monthly Notices of the Royal Astronomical Society
Taylor E
(2015)
Galaxy And Mass Assembly (GAMA): deconstructing bimodality - I. Red ones and blue ones
in Monthly Notices of the Royal Astronomical Society
Robotham A
(2014)
Galaxy And Mass Assembly (GAMA): galaxy close pairs, mergers and the future fate of stellar mass
in Monthly Notices of the Royal Astronomical Society
Lange R
(2015)
Galaxy And Mass Assembly (GAMA): mass-size relations of z < 0.1 galaxies subdivided by Sérsic index, colour and morphology
in Monthly Notices of the Royal Astronomical Society
Casteels K
(2014)
Galaxy And Mass Assembly (GAMA): refining the local galaxy merger rate using morphological information
in Monthly Notices of the Royal Astronomical Society
Kelvin L
(2014)
Galaxy And Mass Assembly (GAMA): stellar mass functions by Hubble type
in Monthly Notices of the Royal Astronomical Society
McNaught-Roberts T
(2014)
Galaxy And Mass Assembly (GAMA): the dependence of the galaxy luminosity function on environment, redshift and colour
in Monthly Notices of the Royal Astronomical Society
Wang L
(2018)
Galaxy and Mass Assembly (GAMA): The environmental dependence of the galaxy main sequence
in Astronomy & Astrophysics
Eardley E
(2015)
Galaxy And Mass Assembly (GAMA): the galaxy luminosity function within the cosmic web
in Monthly Notices of the Royal Astronomical Society
Gunawardhana M
(2018)
Galaxy And Mass Assembly (GAMA): the signatures of galaxy interactions as viewed from small-scale galaxy clustering
in Monthly Notices of the Royal Astronomical Society
Kelvin L
(2014)
Galaxy And Mass Assembly (GAMA): ugrizYJHK Sérsic luminosity functions and the cosmic spectral energy distribution by Hubble type
in Monthly Notices of the Royal Astronomical Society
Hogan M
(2015)
High radio-frequency properties and variability of brightest cluster galaxies
in Monthly Notices of the Royal Astronomical Society
Robson E
(2014)
IMAGING THE ENVIRONMENT OF A z = 6.3 SUBMILLIMETER GALAXY WITH SCUBA-2
in The Astrophysical Journal
Tiley A
(2019)
KROSS-SAMI: a direct IFS comparison of the Tully-Fisher relation across 8 Gyr since z ˜ 1
in Monthly Notices of the Royal Astronomical Society
Magdis G
(2016)
KROSS: mapping the Ha emission across the star formation sequence at z ˜ 1
in Monthly Notices of the Royal Astronomical Society
Description | The award of funds to travel to telescopes that this grant enabled allowed Durham astronomers to make a number of significant new discoveries in the properties of galaxies, clusters of galaxies and AGN over a wide range in distance from the Milky Way. These ranged from sub-mm surveys with the JCMT and the SCUBA-2 instrument on Hawaii, using a new instrument KMOS, on the VLT in Chile. developed in Durham, using the Australia Telescope Compact Array in Australia as well as optical and sub-mm telescopes in Europe and the Canary Islands. In addition we have contributed to the imaging surveys required for the DESI survey using the Kitt Peak 4m telescope. |
Exploitation Route | The sub-mm surveys have a wide impact as the SCUBA-2 instrument is unique and the sources detected are being followed up by Durham astronomers and others with ALMA and many other optical, NIR and radio telescopes. The new DESI survey has now started full operations and the some of the recent runs were to cover the imaging survey required for target selection and have been vital. |
Sectors | Digital/Communication/Information Technologies (including Software),Education |
Description | The observations performed in the 2014-2016 period were heavily weighted to our involvement in the SCUBA-2 Legacy Surveys that have resulted in many direct papers and papers from follow-up observations particularly with ALMA, |
First Year Of Impact | 2016 |
Sector | Digital/Communication/Information Technologies (including Software),Education |
Impact Types | Cultural,Societal |
Description | GAMA and SAMI Surveys using AAT |
Organisation | Anglo Australian Observatory |
Country | Australia |
Sector | Academic/University |
PI Contribution | Involvement in large AAT surveys GAMA and SAMI through collaboration and contribution to observing effort facilitated by our PATT travel grant. |
Collaborator Contribution | Observing effort, data analysis and creation of mock catalogues from N-body simulations. |
Impact | Numerous papers from the GAMA and SAMI consortia. |
Start Year | 2011 |
Description | GAMA and SAMI Surveys using AAT |
Organisation | University of Sydney |
Country | Australia |
Sector | Academic/University |
PI Contribution | Involvement in large AAT surveys GAMA and SAMI through collaboration and contribution to observing effort facilitated by our PATT travel grant. |
Collaborator Contribution | Observing effort, data analysis and creation of mock catalogues from N-body simulations. |
Impact | Numerous papers from the GAMA and SAMI consortia. |
Start Year | 2011 |
Description | Observational cosmology with CalTech |
Organisation | California Institute of Technology |
Department | Caltech Astronomy |
Country | United States |
Sector | Academic/University |
PI Contribution | Preparing, performing and analysing Keck data then writing a number of papers from these obsevations.. |
Collaborator Contribution | Access to Keck 10m telescopes |
Impact | Several papers from the publication list are the result of this collaboration. |
Start Year | 2006 |
Description | Numerous schools visits, science fairs and open days |
Form Of Engagement Activity | Participation in an open day or visit at my research institution |
Part Of Official Scheme? | Yes |
Geographic Reach | National |
Primary Audience | Schools |
Results and Impact | The outreach activity in Durham is too wide and frequent to make filling in boxes like this feasible. If any group can they they are\ n't doing enough of it. The public appreciation of astronomy in the North East is higher than it would be without our work. |
Year(s) Of Engagement Activity | 2011,2012 |