The Phoenix Deep Survey: X-ray properties of faint radio sources     

A. Georgakakis  A. M. Hopkins †  M. Sullivan  J. Afonso  I. Georgantopoulos  B. Mobasher  L. E. Cram 《Monthly notices of the Royal Astronomical Society》2003,345(3):939-948

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A Complete Microjansky Radio Survey     

José Afonso  Bahram Mobasher  Andrew Hopkins  Lawrence Cram 《Astrophysics and Space Science》2001,276(2-4):941-948

The Phoenix Deep Survey is an ongoing multi-wavelength survey of a 2^° diameter field aimed at studying the properties of the sub-mJy and μJy radio population. Here, we present the latest 1.4 GHz observations of this field. The new data, reaching a 5 σ flux level of 45 μJy at the centre of a 50′ diameter field, comprise more than 700 sources with flux densities less than 1 mJy (187 of which have S_1.4 < 100 μJy). This provides one of the deepest radio (1.4 GHz) surveys currently available. The 1.4 GHz source counts are presented and show a flattening down to the 50 μJy level. At flux densities around 300 μJy there are indications that the sources detected may exhibit higher clustering than those observed at higher flux levels. This suggests that deep radio surveys could be useful for studies of large-scale structure but it also presents a warning for the representativity of sources in deep pencil-beam radio surveys. The study of the optical counterparts of the μJy population seems to indicate that the median R magnitude starts to decrease below 100 μJy. Spectroscopic classification of a sample of sources in this survey confirms the trend for an increasing fraction of star-forming galaxies over other systems down to ～ 100 μJy.  相似文献   

The photometric period of 39 AY Ceti     

J. A. Eaton  D. S. Hall  G. W. Henry  J. L. Hopkins  K. Krisciunas  H. J. Landis  H. Louth  E. H. Olsen  T. R. Renner  H. J. Stelzer 《Astrophysics and Space Science》1983,93(2):271-276

Photoelectric photometry obtained in 1971 and 1972 is compared with that obtained in 1980–81 and 1981–82 to derive a photometric period of 77 ^d .65. JD 2444636.0 is an epoch of minimum light. The full amplitude has been as large as 0 ^m .18 inV. Curiously, the mean light level has dropped by almost 0 ^m .2 over the last ten years. This binary is additionally interesting because of the recently discovered white dwarf secondary component and because unpublished radial velocity measures of Fekel show a large (0.1) eccentricity and an orbital period (57 ^d .1) very different from our photometric period.  相似文献   

A QUANTITATIVE ANALYSIS OF THE INDUCED GRASSLANDS OF THE BISMARCK MOUNTAINS, PAPUA NEW GUINEA     

Harley Manner  B.A.  Ph.D.  Helen Lang  BA. 《Singapore journal of tropical geography》1981,2(1):40-48

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Thermal treatment as a method to control transfers of invasive biofouling species via vessel sea chests     

Piola RF  Hopkins GA 《Marine pollution bulletin》2012,64(8):1620-1630

This study examined the efficacy of heated seawater for the treatment and remediation of fouled vessel sea chest habitats. In laboratory trials, three temperature regimes (37.5°C for 60 min, 40°C for 30min and 42.5°C for 20 min) were tested on a range of temperate taxa commonly found in sea chests. Field validation trials further assessed the efficacy of heat treatment within a replica sea chest environment. During laboratory trials, 100% mortality was achieved across all three treatments for the majority of taxa; the exceptions being the barnacle Elminius modestus and the oyster Crassostrea gigas. Temperature tolerance limits observed in the laboratory were successfully replicated under simulated sea chest conditions; however, a failure to achieve even heat distribution was an obstacle to achieving uniform mortality. This study provides guidance on the temperature/exposure parameters required for vessels plying temperate latitudes, and demonstrates that heated seawater has potential for controlling biofouling in vessel sea chests.  相似文献   

The evolution of stellar mass and the implied star formation history     

Stephen M. Wilkins  Neil Trentham  Andrew M. Hopkins 《Monthly notices of the Royal Astronomical Society》2008,385(2):687-694

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Growth rate in a population of the freshwater crayfish,Paranephrops planifrons white   总被引：1，自引：1，他引：0  

C. L. Hopkins 《新西兰海洋与淡水研究杂志》2013,47(4):464-474

Observations on growth increments at moult in a population of freshwater crayfish, Paranephrops planifrons, were made from periodic recaptures of marked animals. The growth increment increased with increasing size of crayfish up to about 20 mm carapace length (65 mm total length) after which a slight decrease was evident. By analysis of the size distributions in samples taken at different times of year it was found that four to five year classes were normally present. Growth of these age components could be followed through consecutive samples. Mean size at leaving the parent in December was 3.5 mm, after one year 11.4–11.8 mm, after two years 18.2–19.3 mm, after three years 22.1–23.8 mm, and after four years 26.7–29.6 mm, all sizes quoted as carapace lengths. After sexual maturity growth in the females was less than in the males. The number of moults completed by each year class was found by relating data on growth increment per moult to growth shown in consecutive quantitative samples. In the first year of life nine moults were completed, in the second year three moults, in the third year two moults, and in the fourth one moult. Independent data on moult frequency recorded from marked crayfish agreed well with these figures.  相似文献   

Reproduction in Galaxias fasciatus Gray (Salmoniformes : Galaxiidae)   总被引：2，自引：2，他引：0  

C. L. Hopkins 《新西兰海洋与淡水研究杂志》2013,47(2):225-230

A study of the reproductive cycle was made on Galaxias fasciatus Gray from streams on Banks Peninsula, South Island, New Zealand. There was no spawning migration; adults remained in the usual adult habitat to breed. The course of gonad maturation showed that spawning occurred in the autumn, from the end of April to mid‐June. Most males matured at 2 years of age and most females at 4 years old. Egg numbers in the females varied from 3800 to 23 600. Males were predominant in age groups 1–4, females in the older age groups. Amongst fish of potential breeding age there was an excess of males. Circumstantial evidence suggested that eggs were laid among piles of water‐logged debris lodged in pools and backwaters. The larvae, which are briefly described, probably hatch during floods to be swept quickly downstream to the sea.  相似文献   

Life history of Galaxias divergens (Salmonoidea: Galaxiidae)     

C. L. Hopkins 《新西兰海洋与淡水研究杂志》2013,47(1):41-57

Galaxias divergent Stokell is a small, bottom‐dwelling fish inhabiting streams in the North Island and the northern part of the South Island. Its ecology is similar in many respects to that of G. vulgaris. The fry develop in the same environment as the adults, unlike the sea‐going young of several other Galaxias spec'es. Spawning occurs in spring and summer, and at least some of the fish mature at the beginning of their second year. The maximum age attained seems to be about 3 years, and the fish can reach a length of about 80 mm in this time. The food consists mostly of small benthic invertebrates taken from both the stream bed and the drift fauna.  相似文献   

Performance evaluation of three DEM‐based fluvial terrace mapping methods          下载免费PDF全文

Austin J Hopkins  Noah P Snyder 《地球表面变化过程与地形》2016,41(8):1144-1152

The availability of high‐resolution digital elevation models (DEMs) derived from airborne light detection and ranging (LiDAR) surveys has spurred the development of several methods to identify and map fluvial terraces. The post‐glacial landscape of the Sheepscot River watershed, Maine, where land‐use change has produced fill terraces upstream of historic dam sites, was selected to implement a comparison between terrace mapping methodologies. At four study sites within the watershed, terraces were manually mapped on LiDAR‐DEM‐derived hillshade images to facilitate the comparison among fully and semi‐automated DEM‐based procedures, including: (1) spatial relationships between interpreted terraces and surrounding natural topography, (2) feature classification algorithms, and (3) the TerEx terrace mapping toolbox. Each method was evaluated based on its accuracy and ease of implementation. The four study sites have varying longitudinal slope (0.0008–0.006 m/m), channel width (< 5–30 m), surrounding landscape relief (20–80 m), type and density of surrounding land use, and mapped surficial geologic units. All methods generally overestimate terrace areas (average predicted area 210% of manually defined area) with the most accurate results achieved within confined river valleys surrounded by the steep hillslopes. Accuracy generally decreases for study sites surrounded by low‐relief landscapes (predicted areas ranged 4–953% of manual delineations). We conclude with the advantages and drawbacks of each method tested and make recommendations for the scenarios where the use of each method is most appropriate. Copyright © 2016 John Wiley & Sons, Ltd.  相似文献