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1,213 results for “South Australia”
Subspecies and Distribution. C.n.nanusDesmarest,1818—TasmaniaandBassStraitIs(KingandFlinders). C. n. unicolor Krefft, 1863 — mainland Australia, from the Queensland/New South Wales border down the E coast through S Victoria to SE South Australia. in Burramyidae
Subspecies and Distribution. C.n.nanusDesmarest,1818—TasmaniaandBassStraitIs(KingandFlinders). C. n. unicolor Krefft, 1863 — mainland Australia, from the Queensland/New South Wales border down the E coast through S Victoria to SE South Australia.
Distribution. Sandy deserts of C Australia (S Northern Territory, SE Western Australia, and W South Australia), including portions of the Great Victoria, Tanami, and Great Sandy deserts, and possibly parts of the Simpson Desert; it also occurs in sandy tracts within the desert uplands around Alice Springs, S Northern Territory. in Notoryctidae
Distribution. Sandy deserts of C Australia (S Northern Territory, SE Western Australia, and W South Australia), including portions of the Great Victoria, Tanami, and Great Sandy deserts, and possibly parts of the Simpson Desert; it also occurs in sandy tracts within the desert uplands around Alice Springs, S Northern Territory.
Distribution. Coastal and subcoastal E Australia from Cape York Peninsula, NE Queensland, to far SE South Australia and inland to Adavale, Queensland; present also on islands of Fraser, Bribie, North and South Stradbroke, Peel, and Russell (all in Queensland), as well as Chinaman, Hummock, Little Snake, Phillip, Rotamah, and Sunday (all in Victoria). in Macropodidae
Distribution. Coastal and subcoastal E Australia from Cape York Peninsula, NE Queensland, to far SE South Australia and inland to Adavale, Queensland; present also on islands of Fraser, Bribie, North and South Stradbroke, Peel, and Russell (all in Queensland), as well as Chinaman, Hummock, Little Snake, Phillip, Rotamah, and Sunday (all in Victoria).
FIGURE 1 in A new species of Dinotoperla Tillyard, 1921 from the Shoalhaven Catchment, New South Wales, Australia (Plecoptera: Gripopterygidae)
FIGURE 1. Neighbour-joining tree of COI5' fragment using Tamura-Nei model of evolution, pairwise deletion, homogeneous lineage and 2000 bootstrap pseudoreplicates. Values below 75 are not shown on tree.
FIGURE 1 in Galeatylinae, a new subfamily of Atylidae for Galeatylus coripes, new genus and species, from the Bass Strait, south-eastern Australia (Amphipoda Dexaminoidea)
FIGURE 1. Galeatylus coripes gen. et sp. nov., holotype. a1 ped, antenna 1 peduncle; ll, lower lip; md, mandible; mx1 and mx2, maxilla 1 and 2; mxp, maxilliped; ul, upper lip; up1–up3, uropods 1–3; tel, telson. Scale for habitus: 1 mm.
FIGURE 5 in Could this be Australia's rarest Banksia? Banksia vincentia (Proteaceae), a new species known from fourteen plants from south-eastern New South Wales, Australia
FIGURE 5. Isotype of Banksia vincentia (M.L. Stimpson 335, S. Harris, L. Winberg, NE 99575); precise location has been withheld due to conservation status, see text for discussion.
FIGURE 1 in A new species of frogfish of the genus Kuiterichthys (Lophiiformes: Antennariidae: Histiophryninae) from New South Wales, Australia
FIGURE 1. Kuiterichthys pietschi, new species, holotype, AMS I.33555-004, 25.8 mm SL, Crowdy Head, NSW, 31.9°S, 152.9°E.
FIGURE 2 in A new species of frogfish of the genus Kuiterichthys (Lophiiformes: Antennariidae: Histiophryninae) from New South Wales, Australia
FIGURE 2. Kuiterichthys furcipilis, Hobart, Tasmania; published in Pietsch and Grobecker (1987, plate 41). Photograph by R.H. Kuiter.
Australia Telescope Hubble Deep Field-South Combined Source Catalog
Deep radio observations of a wide region centered on the Hubble Deep Field-South (HDF-S) have been performed, providing one of the most sensitive sets of radio observations acquired on the Australia Telescope Compact Array (ATCA) to date. A central rms of ~ 10 µJy is reached at four frequencies (1.4, 2.5, 5.2, and 8.7 GHz). In this table, the combined 4-frequency AT-HDFS Catalog including fluxes and spectral indices for sources detected at 1.4, 2.5, 5.2, and/or 8.7 GHz observations is presented to complement the single-frequency radio data for the 1.4 GHz observations which were presented in Paper II (Huynh et al., 2005, AJ, 130, 1373, available at the HEASARC as the ATHDFS1P4G table) in this series, and for the 2.5, 5.2, and/or 8.7 GHz observations which were presented in the reference paper (Paper III, Huynh et al., 2007, AJ, 133, 1331, available at the HEASARC as the ATHDFS3FRQ table). The details of the observations and data reduction are discussed in detail in Paper I of this series (Norris et al., 2005, AJ, 130, 1358) and summarized in Table 1 of the reference paper. The radio observations were carried out by the ATCA over 4 years from 1998 to 2001. The observations at 1.4 and 2.5 GHz consist of single pointings centered on RA (J2000.0) = 22<sup>h</sup> 33<sup>m</sup> 25.96<sup>s</sup>, Dec (J2000.0) = -60<sup>o</sup> 38' 09.0". The observations at 5.2 and 8.7 GHz consist of single pointings centered on RA (J2000.0) = 22<sup>h</sup> 32<sup>m</sup> 56.22<sup>s</sup>, Dec (J2000.0) = -60<sup>o</sup> 33' 02.7". The 5.2 and 8.7 GHz observations are centered on the HST WFPC field, while the 1.4 and 2.5 GHz observations were pointed halfway between the WFPC field and a bright confusing source to allow the bright source to be well cleaned from the 1.4 and 2.5 GHz images. This HEASARC table contains the final consolidated catalog of 473 individual sources and gives the flux densities at all frequencies for each individual radio source. It contains the 466 1.4-GHz sources from Paper II together with 5 unmatched 2.5-GHz sources and 2 unmatched 8.7-GHz sources. The procedure that the authors used to construct this catalog is discussed in Section 6 of the reference paper. This table was created by the HEASARC in December 2012 based on the <a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/AJ/130/1371">CDS Catalog J/AJ/130/1371</a> file table9.dat which contains the entire contents of Table 9 from the published paper. This is a service provided by NASA HEASARC .
Australia Telescope Hubble Deep Field-South Optical Identifications Catalog
The Australia Telescope Hubble Deep Field-South (ATHDF-S) survey of the Hubble Deep Field-South (HDF-S) reaches sensitivities of ~ 10 µJy (µJy) at 1.4, 2.5, 5.2, and 8.7 GHz, making the ATHDF-S one of the deepest surveys ever performed with the Australia Telescope Compact Array (ATCA). This table contains the optical identifications of the ATHDF-S radio sources (the radio data from which are available in summarized form in the HEASARC ATHDFSCCAT table) using data from the literature. The authors find that ~ 66% of the radio sources have optical counterparts to an I magnitude of 23.5 mags. Deep Hubble Space Telescope (HST) imaging of the area identifies a further 12% of the radio sources. In this table, the authors present data from new spectroscopic observations for 98 of the radio sources and supplement these spectroscopic redshifts with photometric ones calculated from five-band optical imaging. The radio observations and data reduction are detailed in Papers I-III of this series: <pre> I = Norris et al., 2005, AJ, 130, 1358; II = Huynh et al., 2005, AJ, 130, 1373, available at the HEASARC as the ATHDFS1P4G table; III = Huynh et al., 2007, AJ, 133, 1331, available at the HEASARC as the ATHDFSCCAT and ATHDFS3FRQ tables. </pre> Palunas et al. (2000, ApJ, 541, 61) observed the HDF-S region using the Big Throughput Camera (BTC) on the Cerro Tololo Inter-American Observatory (CTIO) 4m during 1998 September. Images were taken in the Sloan Digital Sky Survey (SDSS) u, Johnson B and V, and Cousins R and I filters. In addition, the authors obtained spectra of the ATHDF-S radio sources over two service nights in 2001 July and 2003 October using the multi-fiber 2dF instrument of the Anglo-Australian Telescope (AAT). They acquired low-resolution (9 Angstrom) spectra over the wavelength range from 3800 to 8000 Angstroms. This table was created by the HEASARC in December 2012 based on the <a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/AJ/135/2470">CDS Catalog J/AJ/135/2470</a> files table1.dat and table10.dat which contain the entire contents of Tables 1 and 10 from the published paper. This is a service provided by NASA HEASARC .
Australia Telescope Chandra Deep Field-South and SDSS Stripe 82 20-GHz Sources
This table contains a source catalog, one of the first results from a deep, blind radio survey carried out at 20 GHz with the Australia Telescope Compact Array, with follow-up observations at 5.5, 9 and 18 GHz. The Australia Telescope 20GHz (AT20G) deep pilot survey covers a total area of 5 deg<sup>2</sup> in the Chandra Deep Field South and in Stripe 82 of the Sloan Digital Sky Survey. The authors estimate the survey to be 90% complete above 2.5 mJy. Of the 85 sources detected, 55% have steep spectra (spectral index alpha<sub>1.4</sub><sup>20</sup> < -0.5) and 45% have flat or inverted spectra (alpha<sub>1.4</sub><sup>20</sup> >= -0.5). The steep-spectrum sources tend to have single power-law spectra between 1.4 and 18 GHz, while the spectral indices of the flat- or inverted-spectrum sources tend to steepen with frequency. Among the 18 inverted-spectrum (alpha<sub>1.4</sub><sup>20</sup> >= 0.0) sources, 10 have clearly defined peaks in their spectra with alpha<sub>1.4</sub><sup>5.5</sup> > 0.15 and alpha<sub>9</sub><sup>18</sup> < -0.15. On a 3-yr time-scale, at least 10 sources varied by more than 15 percent at 20 GHz, showing that variability is still common at the low flux densities probed by the AT20G-Deep Pilot (AT20GDP) survey. The AT20G-Deep Pilot survey was carried out with he ATCA in 2009 July, shortly after the telescope was provided with a new wide-bandwidth correlator, the CABB. As a result of this upgrade to the telescope, the observing bandwidth was increased by a factor of 16, from 2x128 to 2x2048 MHz, in all bands (ranging from 1.1 to 105 GHz), greatly increasing the sensitivity of continuum observations. These observations were made in continuum mode using two 2048-MHz CABB bands centered at 19 and 21 GHz, with each 2048-MHz band divided into 2048 1-MHz channels. All four Stokes parameters were measured. This table was created by the HEASARC in August 2015 based on the union of <a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/MNRAS/439/1212">CDS Catalog J/MNRAS/439/1212</a> files table2.dat (the 50 sources in the 3-hr field) and table3.dat (the 35 sources in the 21-hr field). This is a service provided by NASA HEASARC .
Australia Telescope Hubble Deep Field-South 1.4-GHz Source Catalog
This table derives from a paper which is part of a series describing the results from the Australia Telescope Hubble Deep Field-South (ATHDFS) survey obtained with the Australia Telescope Compact Array. This survey consists of observations at 1.4, 2.5, 5.2, and 8.7 GHz, all centered on the Hubble Deep Field-South. Herein are presented the first results from the extended observing campaign at 1.4 GHz. A total of 466 sources have been cataloged to a local sensitivity of 5-sigma (11 µJy rms). A source extraction technique is developed that (1) successfully excludes spurious sources from the final source catalogs and (2) accounts for the nonuniform noise in the image. A source catalog is presented, and the general properties of the 1.4-GHz image are discussed in the reference paper. In the latter, the authors also present source counts derived from their ATHDFS 1.4-GHz catalog. The 1.4 GHz observations were carried out by the Australia Telescope Compact Array over 4 years from 1998 to 2001. They consist of single pointings centered on RA (J2000.0) = 22<sup>h</sup> 33<sup>m</sup> 25.96<sup>s</sup>, Dec (J2000.0) = -60<sup>o</sup> 38' 09.0". This table was created by the HEASARC in November 2012 based on the <a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/AJ/130/1371">CDS Catalog J/AJ/130/1371</a> file table1.dat. This is a service provided by NASA HEASARC .
Australia Telescope Hubble Deep Field-South 2.5, 5.2 and 8.7-GHz Source Catalog
Deep radio observations of a wide region centered on the Hubble Deep Field-South (HDF-S) have been performed, providing one of the most sensitive sets of radio observations acquired on the Australia Telescope Compact Array (ATCA) to date. A central rms of ~ 10 µJy is reached at four frequencies (1.4, 2.5, 5.2, and 8.7 GHz). In this table, the full source catalogs from the 2.5, 5.2, and 8.7 GHz observations are presented to complement the data for the 1.4 GHz observations which were presented in Paper II (Huynh et al., 2005, AJ, 130, 1373, available at the HEASARC as the ATHDFS1P4G table) in this series, along with a detailed analysis of image quality and noise. The authors also have produced a consolidated catalog of all of their ATCA observations of the HDF-S by matching sources across all four of the frequencies in their survey (available at the HEASARC as the ATHDFSCCAT table). The details of the observations and data reduction are discussed in detail in Paper I of this series (Norris et al., 2005, AJ, 130, 1358) and summarized in Table 1 of the reference paper. The observations consist of single pointings centered on RA (J2000.0) = 22<sup>h</sup> 33<sup>m</sup> 25.96<sup>s</sup>, Dec (J2000.0) = -60<sup>o</sup> 38' 09.0" (2.5 GHz), and RA (J2000.0) = 22<sup>h</sup> 32<sup>m</sup> 56.22<sup>s</sup>, Dec (J2000.0) = -60<sup>o</sup> 33' 02.7" (5.2 and 8.7 GHz). The 5.2 and 8.7 GHz observations are centered on the HST WFPC field, while the 2.5 GHz observations were pointed halfway between the WFPC field and a bright confusing source to allow the bright source to be well cleaned from the 2.5 GHz image. At 5 sigma, the 5.2 and 8.7 GHz catalogs have over 96% reliability. At 2.5 GHz, the authors have enough statistics to examine the 5 - 5.5 sigma sources, and find that these are only about 40% reliable. With a SNR greater than 5.5 sigma, the 2.5 GHz catalog would have about 99% reliability. The authors thus cut off the catalogs at 5.5, 5, and 5 sigma for 2.5, 5.2, and 8.7 GHz, respectively. The final catalogs have 71, 24, and 6 sources at 2.5, 5.2, and 8.7 GHz, respectively. Given a prior 1.4 GHz position, it may be feasible to push the detection limit lower than 5 sigma. The authors searched for low-SNR sources by matching 3 - 5 sigma sources that lie within 2 sigma positional uncertainty of a 1.4 GHz source. The positional uncertainty was determined by adding the average 1.4 GHz uncertainty (1.1") in quadrature with the positional uncertainty of a 3 sigma source. At 2.5 GHz the allowed positional offset is 3.8", and for 5.2 and 8.7 GHz it is 2.8". Thus, there are 71, 18, and 2 sources at 2.5, 5.2, and 8.7 GHz, respectively, which are low-SNR high-frequency counterparts to 1.4 GHz sources. The authors included these sources in supplementary catalogs. This HEASARC table contains all 101 primary sources detected at 2.5, 5.2, and 8.7 GHz, as well as the 91 supplementary sources described above (the latter are flagged by having source_flag values of 'S'), for a grand total of 192 radio sources. This table was created by the HEASARC in December 2012 based on the <a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/AJ/130/1371">CDS Catalog J/AJ/130/1371</a> files table47.dat, table58.dat and table68.dat, which contain the entire contents of Tables 4, 5, 6, 7 and 8 from the published paper. This is a service provided by NASA HEASARC .
Australia Telescope Compact Array AKARI Deep Field South 20-cm Source Catalog
The results of a deep radio survey at a wavelength of 20 cm are reported for a region containing the AKARI Deep Field South (ADF-S) near the South Ecliptic Pole (SEP), using the Australia Telescope Compact Array (ATCA). The survey (hereafter referred to as the ATCA-ADFS survey) has 1-sigma detection limits ranging from 18.7 to 50 microJansky per beam (µJy/beam, over an area of ~1.1 deg<sup>2</sup>, and ~2.5 deg<sup>2</sup> to lower sensitivity. The observations, data reduction and source count analysis are presented in the paper, along with a description of the overall scientific objectives, and a catalog containing 530 radio sources detected with a resolution of 6.2 x 4.9 arcseconds (contained herein). The AKARI Deep Field South survey was primarily made in the far-infrared at wavelengths of 65, 90, 140, 160 micron (µm) over a 12 deg<sup>2</sup> area with the AKARI Far-Infrared Surveyor (FIS) instrument, with shallower mid-infrared coverage at 9 and 18 um using the AKARI Infrared Camera (IRC) instrument. In addition to the wide survey, deeper mid-infrared pointed observations, using the IRC, covering ~0.8 deg<sup>2</sup> and reaching 5-sigma sensitivities of 16, 16, 74, 132, 280 and 580 uJy at 3.2, 4.6, 7, 11, 15 and 24 um, respectively, were also carried out. The radio observations were collected over a 13 day period in 2007 July using the ATCA operated at 1.344 and 1.432 GHz. The total integration time for the 2007 observations was 120 hours. The 2007 data were augmented with a further deep observation made in 2008 December over five nights towards a single pointing position at the ADF-S, which lay just off center of the larger ATCA-ADFS field reported here. This added a further 50 h of integration time. The data were processed in exactly the same way as that from the 2007 observing sessions. Note that in the terminology of the authors, a radio component is described as a region of radio emission represented by a Gaussian shaped object in the map. Close radio doubles are represented by two Gaussians and are deemed to consist of two components, which make up a single source. A selection of radio sources with multiple components is shown in Fig. 3 of the reference paper. This table was created by the HEASARC in November 2013 based on <a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/MNRAS/427/1830">CDS Catalog J/MNRAS/427/1830</a> file table2.dat. This is a service provided by NASA HEASARC .
Grape berry developmental series comparing pruning treatments from a vineyard in Clare Valley, South Australia (CLA-05)
GEO Series GSE7680. Vitis vinifera. 68 samples. Type: Expression profiling by array.
FIgure 106 in Seven new peacock spiders from Western Australia and South Australia (Araneae: Salticidae: Euophryini: Maratus)
<p>FIgure 106. Medial to lateral views of the left pedipalp of two male Maratus vultus (types) in alcohol. In a lateral view (5, 10), bifurcation of the wide tip of the outer apex of the embolus can be seen. The inner apex is much shorter, smaller, and sharply pointed. This configuration is characteristic of the anomalus group.</p>
FIgure 105. Living male Maratus vultus. 1, Expanded fan during display. 2, 4 in Seven new peacock spiders from Western Australia and South Australia (Araneae: Salticidae: Euophryini: Maratus)
<p>FIgure 105. Living male Maratus vultus. 1, Expanded fan during display. 2, 4, Detail of dorsal opisthosoma from the rear. 3, Rear view of opisthosoma, showing small median tract of white scales behind and below the dorsal plate, continuous with a small triangular, colular patch of white scales, above the black spinnerets. 5, Ventral view.</p>
FIgure 103 in Seven new peacock spiders from Western Australia and South Australia (Araneae: Salticidae: Euophryini: Maratus)
<p>FIgure 103. Comparison of male Maratus vultus (1 - 3) with other male Maratus. 4, M. amabilis from Mt. Kaputar NP, NSW. 5, M. cf. amabilis from Barrington Tops NP, NSW. 6 - 8, M. anomalus from Ku-ring-gai Chase NP, NSW. 9 - 11, M. cf. anomalus from Warby-Ovens NP, Victoria.</p>
Figure 100. Consecutive frames from a 25 in Seven new peacock spiders from Western Australia and South Australia (Araneae: Salticidae: Euophryini: Maratus)
<p>Figure 100. Consecutive frames from a 25 fps video of display by a male Maratus vespa, showing ' pincher' movement of legs III above the carapace (double or paired arrows at top), accompanied by limited movement of the fan from side to side (arrows) and some side-stepping (large arrows in 15, 16, 26). All arrows indicate movement relative to the previous frame. The pedipalps were held apart to reveal the black face and chelicerae during this display.</p>
Figure 99. Consecutive frames from a 25 in Seven new peacock spiders from Western Australia and South Australia (Araneae: Salticidae: Euophryini: Maratus)
<p>Figure 99. Consecutive frames from a 25 fps video showing movement of the fan (arrows) by a male Maratus vespa during display in front of a female. Before the fan was rotated to the side (28 - 36), it was rotated from side to side in a more vertical position (1 - 24). During this sequence only the fan was moved. Each pedipalp was held to the side to display the black face and chelicerae.</p>
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