All Outputs (29)

ALMACAL I: First Dual-band Number Counts from a Deep and Wide ALMA Submillimeter Survey, Free from Cosmic Variance (2016)
Journal Article
Oteo, I., Zwaan, M., Ivison, R., Smail, I., & Biggs, A. (2016). ALMACAL I: First Dual-band Number Counts from a Deep and Wide ALMA Submillimeter Survey, Free from Cosmic Variance. Astrophysical Journal, 822(1), Article 36. https://doi.org/10.3847/0004-637x/822/1/36

We have exploited ALMA calibration observations to carry out a novel, wide, and deep submillimeter (submm) survey, almacal. These calibration data comprise a large number of observations of calibrator fields in a variety of frequency bands and array... Read More about ALMACAL I: First Dual-band Number Counts from a Deep and Wide ALMA Submillimeter Survey, Free from Cosmic Variance.

The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s (2016)
Journal Article
Johnson, H., Harrison, C., Swinbank, A., Bower, R., Smail, I., Koyama, Y., & Geach, J. (2016). The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s. Monthly Notices of the Royal Astronomical Society, 460(1), 1059-1076. https://doi.org/10.1093/mnras/stw1030

To investigate what drives the reversal of the morphology–density relation at intermediate/high redshift, we present a multiwavelength analysis of 27 dusty starburst galaxies in the massive cluster Cl 0024+17 at z = 0.4. We combine Hα dynamical maps... Read More about The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s.

The KMOS Redshift One Spectroscopic Survey (KROSS): the Tully–Fisher relation at z ∼ 1 (2016)
Journal Article
Tiley, A., Stott, J., Swinbank, A., Bureau, M., Harrison, C., Bower, R., …Best, P. (2016). The KMOS Redshift One Spectroscopic Survey (KROSS): the Tully–Fisher relation at z ∼ 1. Monthly Notices of the Royal Astronomical Society, 460(1), 103-129. https://doi.org/10.1093/mnras/stw936

We present the stellar mass (M*), and K-corrected K-band absolute magnitude (MK) Tully–Fisher relations (TFRs) for subsamples of the 584 galaxies spatially resolved in H α emission by the KMOS Redshift One Spectroscopic Survey (KROSS). We model the v... Read More about The KMOS Redshift One Spectroscopic Survey (KROSS): the Tully–Fisher relation at z ∼ 1.

A complete census of Herschel-detected infrared sources within the HST Frontier Fields (2016)
Journal Article
Rawle, T., Altieri, B., Egami, E., Pérez-González, P., Boone, F., Clement, B., …Smail, I. (2016). A complete census of Herschel-detected infrared sources within the HST Frontier Fields. Monthly Notices of the Royal Astronomical Society, 459(2), 1626-1645. https://doi.org/10.1093/mnras/stw712

We present a complete census of all Herschel-detected sources within the six massive lensing clusters of the HST Frontier Fields (HFF). We provide a robust legacy catalogue of 263 sources with Herschel fluxes, primarily based on imaging from the Hers... Read More about A complete census of Herschel-detected infrared sources within the HST Frontier Fields.

The SCUBA-2 Cosmology Legacy Survey: Multi-wavelengths counterparts to 10^3 submillimeter galaxies in the UKIDSS-UDS field (2016)
Journal Article
Chen, C., Smail, I., Ivison, R., Arumugam, V., Almaini, O., Conselice, C., …Zavala, J. (2016). The SCUBA-2 Cosmology Legacy Survey: Multi-wavelengths counterparts to 10^3 submillimeter galaxies in the UKIDSS-UDS field. Astrophysical Journal, 820(2), Article 82. https://doi.org/10.3847/0004-637x/820/2/82

We present multiwavelength identifications for the counterparts of 1088 submillimeter sources detected at 850 μm in the SCUBA-2 Cosmology Legacy Survey study of the UKIRT Infrared Deep Sky Survey-Ultra-Deep Survey (UDS) field. By utilizing an Atacama... Read More about The SCUBA-2 Cosmology Legacy Survey: Multi-wavelengths counterparts to 10^3 submillimeter galaxies in the UKIDSS-UDS field.

The CALYMHA survey: Lyα escape fraction and its dependence on galaxy properties at z = 2.23 (2016)
Journal Article
Matthee, J., Sobral, D., Oteo, I., Best, P., Smail, I., Röttgering, H., & Paulino-Afonso, A. (2016). The CALYMHA survey: Lyα escape fraction and its dependence on galaxy properties at z = 2.23. Monthly Notices of the Royal Astronomical Society, 458(1), 449-467. https://doi.org/10.1093/mnras/stw322

We present the first results from our CAlibrating LYMan-α with Hα (CALYMHA) pilot survey at the Isaac Newton Telescope. We measure Lyα emission for 488 Hα selected galaxies at z = 2.23 from HiZELS in the COSMOS and UDS fields with a specially designe... Read More about The CALYMHA survey: Lyα escape fraction and its dependence on galaxy properties at z = 2.23.

The KMOS Redshift One Spectroscopic Survey (KROSS): dynamical properties, gas and dark matter fractions of typical z~1 star-forming galaxies (2016)
Journal Article
Stott, J., Swinbank, A., Johnson, H., Tiley, A., Magdis, G., Bower, R., …Cirasuolo, M. (2016). The KMOS Redshift One Spectroscopic Survey (KROSS): dynamical properties, gas and dark matter fractions of typical z~1 star-forming galaxies. Monthly Notices of the Royal Astronomical Society, 457(2), 1888-1904. https://doi.org/10.1093/mnras/stw129

The KMOS Redshift One Spectroscopic Survey (KROSS) is an ESO-guaranteed time survey of 795 typical star-forming galaxies in the redshift range z = 0.8–1.0 with the KMOS instrument on the Very Large Telescope. In this paper, we present resolved kinema... Read More about The KMOS Redshift One Spectroscopic Survey (KROSS): dynamical properties, gas and dark matter fractions of typical z~1 star-forming galaxies.

The most luminous H α emitters at z ∼ 0.8–2.23 from HiZELS: evolution of AGN and star-forming galaxies (2016)
Journal Article
Sobral, D., Kohn, S., Best, P., Smail, I., Harrison, C., Stott, J., …Matthee, J. (2016). The most luminous H α emitters at z ∼ 0.8–2.23 from HiZELS: evolution of AGN and star-forming galaxies. Monthly Notices of the Royal Astronomical Society, 457(2), 1739-1752. https://doi.org/10.1093/mnras/stw022

We use new near-infrared spectroscopic observations to investigate the nature and evolution of the most luminous Hα emitters at z ∼ 0.8–2.23, which evolve strongly in number density over this period, and compare them to more typical Hα emitters. We s... Read More about The most luminous H α emitters at z ∼ 0.8–2.23 from HiZELS: evolution of AGN and star-forming galaxies.

ALMA resolves extended star formation in high-z AGN host galaxies (2016)
Journal Article
Harrison, C., Simpson, J., Stanley, F., Alexander, D., Daddi, E., Mullaney, J., …Smail, I. (2016). ALMA resolves extended star formation in high-z AGN host galaxies. Monthly Notices of the Royal Astronomical Society: Letters, 457(1), L122-L126. https://doi.org/10.1093/mnrasl/slw001

We present high-resolution (0.3 arcsec) Atacama Large Millimeter Array (ALMA) 870 μm imaging of five z ≈ 1.5–4.5 X-ray detected AGN (with luminosities of L2–8keV > 1042 erg s−1). These data provide a ≳20 times improvement in spatial resolution over s... Read More about ALMA resolves extended star formation in high-z AGN host galaxies.