Archaeological site monitoring: UAV photogrammetry can be an answer

During archaeological excavations it is important to monitor the new excavated areas and findings day by day in order to be able to plan future excavation activities. At present, this daily activity is usually performed by using total stations, which survey the changes of the archaeological site: the surveyors are asked to produce day by day draft plans and sections which allow archaeologists to plan their future activities. The survey is realized during the excavations or just at the end of every working day and drawings have to be produced as soon as possible in order to allow the comprehension of the work done and to plan the activities for the following day. By using this technique, all the measurements, even those not necessary for the day after, have to be acquired in order to avoid a ‘loss of memory'. A possible alternative to this traditional approach is aerial photogrammetry, if the images can be acquired quickly and at a taken distance able to guarantee the necessary accuracy of a few centimeters. Today the use of UAVs (Unmanned Aerial Vehicles) can be considered a proven technology able to acquire images at distances ranging from 4 m up to 20 m: and therefore as a possible monitoring system to provide the necessary information to the archaeologists day by day. The control network, usually present at each archaeological site, can give the stable control points useful for orienting a photogrammetric block acquired by using an UAV equipped with a calibrated digital camera and a navigation control system able to drive the aircraft following a pre-planned flight scheme. Modern digital photogrammetric software can solve for the block orientation and generate a DSM automatically, allowing rapid orthophoto generation and the possibility of producing sections and plans. The present paper describes a low cost UAV system realized by the research group of the Politecnico di Torino and tested on a Roman villa archaeological site located in Aquileia (Italy), a well-known UNESCO WHL site. The results of automatic orientation and orthophoto production are described in terms of their accuracy and the completeness of information guaranteed for archaeological site excavation managemen

Embodied carbon premium for vanity height: A case for the exclusion of decorative spires in the design of tall buildings

In measuring the height of a tall building, the Council on Tall Buildings and Urban Habitat (CTBUH) recognises three categories: “height to architectural top”; “height to highest occupied floor”; and “height to tip”. The “height to architectural top” category, which includes decorative spires, is used to define the influential CTBUH annual rankings of the “World's Tallest Buildings”. The inclusion of decorative spires in the category ranking has created an incentive for developers to maximise the vanity height of tall buildings, defined as the height difference between a tall building's architectural top and its highest occupied floor. The aim of this paper is to demonstrate the detrimental influence of spires and, by extension, vanity height on the embodied carbon of structural systems for tall buildings. This influence is evaluated using three tall building scenarios of varying heights (50, 70, and 90 storeys). Two finite element models, with and without spires, are parametrically designed for each scenario. All the modelled structural systems comprise a reinforced concrete tube-in-tube lateral load resisting system. A hybrid life cycle inventory analysis approach is used to quantify the embodied carbon of spires as well as the resulting increase in the embodied carbon of structural systems. The findings of this study indicate that even basic spires can lead to an increase of up to 14.2% in the embodied carbon of structural systems for tall buildings, underscoring the imperative to eliminate such elements in the design and construction of tall buildings to minimise overall embodied carbon

Serial Cities: Australian Literary Cities and the Rhetoric of Scale

A review essay of New South Books' 'City Series': Sophie Cunningham, Melbourne (2011)Matthew Condon, Brisbane (2010)Paul Daley, Canberra (2012)Delia Falconer, Sydney (2010)Kerryn Goldsworthy, Adelaide (2011)Eleanor Hogan, Alice Springs (2012)Tess Lea, Darwin (2014)Peter Timms, In Search of Hobart (2012)David Whish-Wilson, Perth (2013

Radio Jet Feedback and Star Formation in Heavily Obscured Quasars at Redshifts ~0.3-3, I: ALMA Observations

We present ALMA 870 micron (345 GHz) data for 49 high redshift (0.47<z<2.85), luminous (11.7 < log L(bol) (Lsun) < 14.2) radio-powerful AGN, obtained to constrain cool dust emission from starbursts concurrent with highly obscured radiative-mode black hole (BH) accretion in massive galaxies which possess a small radio jet. The sample was selected from WISE with extremely steep (red) mid-infrared (MIR) colors and with compact radio emission from NVSS/FIRST. Twenty-six sources are detected at 870 microns, and we find that the sample has large mid- to far-infrared luminosity ratios consistent with a dominant and highly obscured quasar. The rest-frame 3 GHz radio powers are 24.7 < log P3.0 GHz (W/Hz) < 27.3, and all sources are radio-intermediate or radio-loud. BH mass estimates are 7.7 < log M(BH) (Msun) < 10.2. The rest frame 1-5 um SEDs are very similar to the "Hot DOGs" (Hot Dust Obscured Galaxies), and steeper (redder) than almost any other known extragalactic sources. ISM masses estimated for the ALMA detected sources are 9.9 < log M(ISM) (Msun) < 11.75 assuming a dust temperature of 30K. The cool dust emission is consistent with star formation rates (SFRs) reaching several thousand Msun/yr, depending on the assumed dust temperature, however we cannot rule out the alternative that the AGN powers all the emission in some cases. Our best constrained source has radiative transfer solutions with ~ equal contributions from an obscured AGN and a young (10-15 Myr) compact starburst.Comment: 29 pages, 8 figures. To appear in Astrophysical Journal. Update on Sept 14 to correct the ALMA proposal id. to ADS/JAO.ALMA#2011.0.00397.S and to add a missing acknowledgemen

The phyllophorid sea cucumbers of southern Australia (Echinodermata: Holothuroidea: Dendrochirotida: Phyllophoridae)

A new monotypic Phyllophoridae (Phyllophorinae) genus Phyllostauros, with author O’Loughlin, is erected for Thyone vercoi Joshua and Creed. We raise Phyllophorella Heding and Panning (subgenus of Phyllophorus Grube) to generic rank. The holotype and three paratypes of Phyllophorus ventripes Joshua and Creed are conspecific with Thyone vercoi Joshua and Creed. We make Phyllophorus ventripes Joshua and Creed a subjective junior synonym of Thyone vercoi Joshua and Creed. One paratype of Phyllophorus ventripes Joshua and Creed is conspecific with Phyllophorus thyonoides H. L. Clark. We reject the synonymy of Thyone okeni Bell with Thyone venusta Selenka. Twelve new species of Phyllophoridae are described for southern Australia, with author O’Loughlin: Lipotrapeza eichleri, Lipotrapeza litusi,Massinium melanieae, Massinium vimsi, Massinium watsonae, Phyllophorella notialis, Thyone flindersi, Thyone joshuai, Thyone kerkosa, Thyone spenceri, Thyone tourvillei, Thyonidiella kungi. Phyllophoridae species reported previously for southern Australia are reviewed: Lipotrapeza ventripes (Joshua and Creed); Lipotrapeza vestiens (Joshua); Neothyonidium dearmatum (Dendy and Hindle); Phyrella thyonoides (H. L. Clark); Thyone nigra Joshua and Creed; Thyone okeni Bell; Thyone vercoi Joshua and Creed. Species Phyrella thyonoides (H. L. Clark) is re-assigned to genus Phyllophorella Heding and Panning. A key is provided for the southern Australian species of Phyllophoridae. We acknowledge the rejection for nomenclatorial purposes by the ICZN (Opinion 417) of the publication by Oken 1815, and hence the current invalid statusof genus Thyone Oken. A petition has been sent to the ICZN for re-validation of Thyone Oken and we retain the use of Thyone Oken provisionally. The petition includes a similar request for re-validation of Psolus Oken

Project pathogens: The anatomy of omission errors in construction and resource engineering project

Construction and engineering projects are typically complex in nature and are prone to cost and schedule overruns. A significant factor that often contributes to these overruns is rework. Omissions errors, in particular, have been found to account for as much as 38% of the total rework costs experienced. To date, there has been limited research that has sought to determine the underlying factors that contribute to omission errors in construction and engineering projects. Using data derived from59 in-depth interviews undertaken with various project participants, a generic systemic causal model of the key factors that contributed to omission errors is presented. The developed causal model can improve understanding of the archetypal nature and underlying dynamics of omission errors. Error management strategies that can be considered for implementation in projects are also discussed

A subarcsecond near-infrared view of massive galaxies at z > 1 with Gemini Multiconjugate Adaptive Optics

We present images taken using the Gemini South Adaptive Optics Imager (GSAOI) with the Gemini Multiconjugate Adaptive Optics System (GeMS) in three 2 arcmin$^2$ fields in the Spitzer Extragalactic Representative Volume Survey. These GeMS/GSAOI observations are among the first $\approx 0.1^{''}$ resolution data in the near-infrared spanning extragalactic fields exceeding $1.5^{\prime}$ in size. We use these data to estimate galaxy sizes, obtaining results similar to those from studies with the Hubble Space Telescope, though we find a higher fraction of compact star forming galaxies at $z>2$. To disentangle the star-forming galaxies from active galactic nuclei (AGN), we use multiwavelength data from surveys in the optical and infrared, including far-infrared data from Herschel, as well as new radio continuum data from the Australia Telescope Compact Array and Very Large Array. We identify ultraluminous infrared galaxies (ULIRGs) at $z \sim 1-3$, which consist of a combination of pure starburst galaxies and Active Galactic Nuclei (AGN)/starburst composites. The ULIRGs show signs of recent merger activity, such as highly disturbed morphologies and include a rare candidate triple AGN. We find that AGN tend to reside in hosts with smaller scale sizes than purely star-forming galaxies of similar infrared luminosity. Our observations demonstrate the potential for MCAO to complement the deeper galaxy surveys to be made with the James Webb Space Telescope.Comment: 20 pages, AJ, in pres

The urban sanctuary: Algae and marine invertebrates of ricketts point marine sanctuary

&quot;This book has been designed to help keen naturalists, high-school students and university undergraduates identify the aquatic plants and invertebrates within Ricketts Point Marine Sanctuary&quot; -- page viii