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1

Monaghan, Nigel T. "Matthew Alastair Parkes." Geological Curator 11, no. 4 (December 2020): 322–32. http://dx.doi.org/10.55468/gc1501.

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2

Amann, Markus, and Jerome A. Dempsey. "Reply to Parkes." Journal of Applied Physiology 110, no. 3 (March 2011): 861. http://dx.doi.org/10.1152/japplphysiol.01445.2010.

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3

Kumar, V., P. Jorwal, A. Biswas, and V. Deorari. "Parkes Weber syndrome." QJM: An International Journal of Medicine 112, no. 12 (May 14, 2019): 936. http://dx.doi.org/10.1093/qjmed/hcz101.

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4

Stefanov-Kiuri, Stefan, and Alvaro Fernandez-Heredero. "Parkes Weber Syndrome." New England Journal of Medicine 371, no. 22 (November 27, 2014): 2114. http://dx.doi.org/10.1056/nejmicm1312948.

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5

Manresa-Manresa, Francisco, María Alcázar Iribarren-Marín, and Francisco Tadeo Gómez-Ruiz. "Parkes-Weber Syndrome." Revista Española de Cardiología (English Edition) 68, no. 1 (January 2015): 67. http://dx.doi.org/10.1016/j.rec.2014.02.022.

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6

Néill, Máire Ní. "Susan Parkes, staraí." Comhar 64, no. 6 (2004): 17. http://dx.doi.org/10.2307/25574926.

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7

Strohschneider, T., S. Lange, and H. Hanke. "Parkes-Weber-Syndrom." Gefässchirurgie 14, no. 2 (August 15, 2008): 129–33. http://dx.doi.org/10.1007/s00772-008-0630-8.

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8

Davis. "Reply to Graham Parkes." Journal of Nietzsche Studies 46, no. 1 (2015): 62. http://dx.doi.org/10.5325/jnietstud.46.1.0062.

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9

Manchester, R. N. "Finding Pulsars at Parkes." Publications of the Astronomical Society of Australia 18, no. 1 (2001): 1–11. http://dx.doi.org/10.1071/as01002.

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AbstractThere are many reasons why it is important to increase the number of known pulsars. Not only do pulsar searches continue to improve statistical estimates of, for example, pulsar birthrates, lifetimes and the Galactic distribution, but they continue to turn up interesting and, in some cases, unique individual pulsars. In the early days of pulsar astronomy, the Molonglo radio telescope led the world as a pulsar detection instrument. However, the Parkes radio telescope, with its frequency versatility and greater tracking ablility, combined with sensitive receivers and powerful computer detection algorithms, is now the world’s most successful telescope at finding pulsars. The Parkes multibeam survey, begun in 1997, by itself will come close to doubling the number of known pulsars. Parkes has also been very successful at finding millisecond pulsars (MSPs), especially in globular clusters. One third of the known MSPs have been found in just one cluster, 47 Tucanae.
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10

Norris, R. P., M. J. Kesteven, K. J. Wellington, and M. J. Batty. "The Parkes-Tidbinbilla interferometer." Astrophysical Journal Supplement Series 67 (May 1988): 85. http://dx.doi.org/10.1086/191267.

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11

Morris, Meaghan. "At Henry Parkes motel." Cultural Studies 2, no. 1 (January 1988): 1–47. http://dx.doi.org/10.1080/09502388800490011.

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12

Norris, R. P., Michael J. Batty, M. J. Kesteven, and K. J. Wellington. "The Parkes-Tidbinbilla Interferometer." Publications of the Astronomical Society of Australia 6, no. 2 (1985): 137–40. http://dx.doi.org/10.1017/s1323358000017938.

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AbstractWe report the development of a radio-linked interferometer which uses the 64-m telescope at Parkes, NSW, and one of the NASA antennas (64-m or 34-m) at Tidbinbilla, ACT. With a baseline of approximately 275 km, this is the world’s longest real-time interferometer; it will be usable at frequencies of 1.6, 2.3, 8.4, and 22 GHz to give angular resolutions of 0.13, 0.09, 0.03, and 0.01 arcsec respectively. The interferometer has already operated successfully in a limited mode and is expected to become fully operational in its initial configuration by September 1985. Operation at a range of frequencies and with progressive enhancements is planned up to the commissioning of the Australia Telescope in 1988.
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13

Webster, R. L., P. J. Francis, B. A. Holman, F. J. Masci, M. J. Drinkwater, and B. A. Peterson. "The Parkes Lens Survey." Symposium - International Astronomical Union 173 (1996): 393–98. http://dx.doi.org/10.1017/s0074180900231872.

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We are undertaking an extensive survey of a sample of radio-selected flat-spectrum sources, which are predominantly quasars. The sample will be used for a range of gravitational lensing studies as well as studies of the generic properties of radio quasars. As yet we have not found any instances of multiply-imaged quasars, however we have found evidence for dust which we believe is reddening the observed spectra of many of the quasars. Samples which are selected to be complete in the radio are the best way to account for the effects of dust.
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14

Manresa-Manresa, Francisco, María Alcázar Iribarren-Marín, and Francisco Tadeo Gómez-Ruiz. "Síndrome de Parkes-Weber." Revista Española de Cardiología 68, no. 1 (January 2015): 67. http://dx.doi.org/10.1016/j.recesp.2014.02.024.

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15

Norris, R. P., M. J. Batty, M. J. Kesteven, and K. J. Wellington. "The Parkes - Tidbinbilla Interferometer." Symposium - International Astronomical Union 129 (1988): 487–88. http://dx.doi.org/10.1017/s0074180900135351.

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The Parkes - Tidbinbilla Interferometer is a radio-linked interferometer using the 64-m telescope at Parkes together with one of the NASA antennas (34-m or 64-m) at Tidbinbilla. With a baseline of 275km, it is currently the world's longest real-time interferometer, and is usable at frequencies of 1.6, 2.3, and 8.4 GHz to give angular resolutions of 0.13, 0.09, and 0.03 arcsec respectively, with a sensitivity of 1–2 mJy rms in 5 minutes at a bandwidth of up to 10MHz.
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16

Poole, Jon. "Parkes’ Occupational Lung Disorders." Occupational Medicine 67, no. 5 (July 2017): 406. http://dx.doi.org/10.1093/occmed/kqx061.

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17

Hobbs, G., D. Miller, R. N. Manchester, J. Dempsey, J. M. Chapman, J. Khoo, J. Applegate, et al. "The Parkes Observatory Pulsar Data Archive." Publications of the Astronomical Society of Australia 28, no. 3 (2011): 202–14. http://dx.doi.org/10.1071/as11016.

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AbstractThe Parkes pulsar data archive currently provides access to 144044 data files obtained from observations carried out at the Parkes observatory since the year 1991. Around 105 files are from surveys of the sky, the remainder are observations of 775 individual pulsars and their corresponding calibration signals. Survey observations are included from the Parkes 70 cm and the Swinburne Intermediate Latitude surveys. Individual pulsar observations are included from young pulsar timing projects, the Parkes Pulsar Timing Array and from the PULSE@Parkes outreach program. The data files and access methods are compatible with Virtual Observatory protocols. This paper describes the data currently stored in the archive and presents ways in which these data can be searched and downloaded.
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18

Osłowski, S., R. M. Shannon, V. Ravi, J. F. Kaczmarek, S. Zhang, G. Hobbs, M. Bailes, et al. "Commensal discovery of four fast radio bursts during Parkes Pulsar Timing Array observations." Monthly Notices of the Royal Astronomical Society 488, no. 1 (June 28, 2019): 868–75. http://dx.doi.org/10.1093/mnras/stz1751.

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ABSTRACT The Parkes Pulsar Timing Array (PPTA) project monitors two dozen millisecond pulsars (MSPs) in order to undertake a variety of fundamental physics experiments using the Parkes 64-m radio telescope. Since 2017 June, we have been undertaking commensal searches for fast radio bursts (FRBs) during the MSP observations. Here, we report the discovery of four FRBs (171209, 180309, 180311, and 180714). The detected events include an FRB with the highest signal-to-noise ratio ever detected at the Parkes Observatory, which exhibits unusual spectral properties. All four FRBs are highly polarized. We discuss the future of commensal searches for FRBs at Parkes.
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19

Manchester, R. N. "The Parkes Pulsar Timing Array." Chinese Journal of Astronomy and Astrophysics 6, S2 (October 2006): 139–47. http://dx.doi.org/10.1088/1009-9271/6/s2/27.

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20

Cohen, R. J., J. L. Caswell, K. Brooks, M. G. Burton, A. Chrysostomou, J. Cox, P. J. Diamond, et al. "The Parkes methanol multibeam survey." Proceedings of the International Astronomical Union 2, S237 (August 2006): 403. http://dx.doi.org/10.1017/s1743921307001913.

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AbstractA new 7-beam methanol multibeam receiver was successfully commissioned at Parkes Observatory in January 2006, and has begun surveying the Milky Way for newly forming massive stars, that are pinpointed by strong methanol maser emission at 6.7 GHz. The receiver was jointly constructed by Jodrell Bank Observatory and the Australia Telescope National Facility for use on the Parkes and Lovell Telescopes. The whole galactic plane is being surveyed within latitudes ±2°, with a velocity resolution of 0.1 km s−1 and a 5-σ sensitivity of ~0.7 Jy. Altogether 200 days of observing will be required.
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21

Ables, J. G., C. E. Jacka, D. McConnell, A. E. Schinckel, and A. J. Hunt. "The Parkes Radio Telescope — 1986." Publications of the Astronomical Society of Australia 6, no. 4 (1986): 507–12. http://dx.doi.org/10.1017/s1323358000018440.

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AbstractThe Parkes radio telescope was commissioned in 1961, with an anticipated operational life of 15 years. Twentyfive years later the telescope has been refurbished with the aim of extending its life yet another decade or two. A major undertaking has been the complete replacement of the drive and control System. This presentation outlines the main features of the new System and its effect on the observing facilities offered at the observatory.
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22

Courivaud, D., A. Delerue, C. Delerue, L. Boon, F. Piette, and P. Modiano. "Syndrome de Parkes-Weber familial." Annales de Dermatologie et de Vénéréologie 133, no. 5 (May 2006): 445–47. http://dx.doi.org/10.1016/s0151-9638(06)70936-x.

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23

Camilo, F., A. G. Lyne, R. N. Manchester, J. F. Bell, V. M. Kaspi, N. D’Amico, N. P. F. McKay, et al. "The Parkes Multibeam Pulsar Survey." International Astronomical Union Colloquium 177 (2000): 3–8. http://dx.doi.org/10.1017/s025292110005884x.

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AbstractThe Parkes multibeam pulsar survey uses a 13-element receiver operating at a wavelength of 20 cm to survey the inner Galactic plane with remarkable sensitivity. To date we have collected and analyzed data from 45% of the survey region (|b| < 5°; 260° <l< 50°), and have discovered 440 pulsars, in addition to re-detecting 190 previously known ones. Most of the newly discovered pulsars are at great distances, as inferred from a median dispersion measure (DM) of 400 cm−3pc.
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24

Manchester, R. N., A. G. Lyne, F. Camilo, V. M. Kaspi, I. H. Stairs, F. Crawford, D. J. Morris, J. F. Bell, and N. D’Amico. "Timing the Parkes Multibeam Pulsars." International Astronomical Union Colloquium 177 (2000): 49–54. http://dx.doi.org/10.1017/s0252921100058991.

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AbstractMeasurement of accurate positions, pulse periods and period derivatives is an essential follow-up to any pulsar survey. The procedures being used to obtain timing parameters for the pulsars discovered in the Parkes multibeam pulsar survey are described. Completed solutions have been obtained so far for about 80 pulsars. They show that the survey is preferentially finding pulsars with higher than average surface dipole magnetic fields. Eight pulsars have been shown to be members of binary systems and some of the more interesting results relating to these are presented.
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25

Hobbs, G. "The Parkes Pulsar Timing Array." Classical and Quantum Gravity 30, no. 22 (November 4, 2013): 224007. http://dx.doi.org/10.1088/0264-9381/30/22/224007.

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26

Doka, Kenneth J. "Parkes, C. M. (2015). The Price of Love: The Selected Works of Colin Murray Parkes." OMEGA - Journal of Death and Dying 73, no. 4 (August 2, 2016): 400–401. http://dx.doi.org/10.1177/0030222816642374.

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27

Eng, Whitney, Christopher L. Sudduth, Dennis J. Konczyk, Patrick J. Smits, Amir H. Taghinia, Steven J. Fishman, Ahmad Alomari, Denise M. Adams, and Arin K. Greene. "Parkes Weber syndrome with lymphedema caused by a somatic KRAS variant." Molecular Case Studies 7, no. 6 (October 4, 2021): a006118. http://dx.doi.org/10.1101/mcs.a006118.

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Parkes Weber syndrome is a vascular malformation overgrowth condition typically involving the legs. Its main features are diffuse arteriovenous fistulas and enlargement of the limb. The condition has been associated with pathogenic germline variants in RASA1 and EPHB4. We report two individuals with Parkes Weber syndrome of the leg and primary lymphedema containing a somatic KRAS variant (NM_004985.5:c.35G > A; p.Gly12Asp). KRAS variants, which cause somatic intracranial and extracranial arteriovenous malformations, also result in Parkes Weber syndrome with lymphatic malformations.
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28

Eng, Whitney, Christopher L. Sudduth, Dennis J. Konczyk, Patrick J. Smits, Amir H. Taghinia, Steven J. Fishman, Ahmad Alomari, Denise M. Adams, and Arin K. Greene. "Parkes Weber syndrome with lymphedema caused by a somatic KRAS variant." Molecular Case Studies 7, no. 6 (October 4, 2021): a006118. http://dx.doi.org/10.1101/mcs.a006118.

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Parkes Weber syndrome is a vascular malformation overgrowth condition typically involving the legs. Its main features are diffuse arteriovenous fistulas and enlargement of the limb. The condition has been associated with pathogenic germline variants in RASA1 and EPHB4. We report two individuals with Parkes Weber syndrome of the leg and primary lymphedema containing a somatic KRAS variant (NM_004985.5:c.35G > A; p.Gly12Asp). KRAS variants, which cause somatic intracranial and extracranial arteriovenous malformations, also result in Parkes Weber syndrome with lymphatic malformations.
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29

Adams, Jenny. "Thomas Hunt's Monograms." Library 22, no. 3 (September 1, 2021): 376–82. http://dx.doi.org/10.1093/library/22.3.376.

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Abstract This note expands on an article by Malcolm Parkes, published posthumously in The Library. In his article, Parkes looks at monograms left by Oxford stationer Thomas Hunt in the manuscripts that Hunt appraised. He argues that Hunt capitalized on these manuscripts, using them as securities for borrowed money he in turn invested in his printing business. Thos note shows that Hunt appraised several more books than Parkes found and suggest that Hunt’s work as a university stationer was possibly more lucrative than previously imagined.
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30

Payne, Paul. "Sky Brightness and Atmospheric Extinction at A.N.R.A.O., Parkes and Siding Spring Observatory." Publications of the Astronomical Society of Australia 6, no. 2 (1985): 182–86. http://dx.doi.org/10.1017/s1323358000018051.

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AbstractIn May 1984 site testing began for the Automated Patrol Telescope. A series of atmospheric extinction and night sky brightness measurements were made over the following year at Parkes and Siding Spring Mountain using B and V filters. Parkes revealed an extinction greater than that of Siding Spring and more prone to variation. Results for the night sky brightness indicated Parkes has a sky slightly brighter than that at Siding Spring. The paper discusses the procedures used for obtaining the results and their limitations.
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31

Hobbs, G., R. Hollow, D. Champion, J. Khoo, D. Yardley, M. Carr, M. Keith, et al. "The PULSE@Parkes Project: a New Observing Technique for Long-Term Pulsar Monitoring." Publications of the Astronomical Society of Australia 26, no. 4 (2009): 468–75. http://dx.doi.org/10.1071/as09021.

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AbstractThe PULSE@Parkes project has been designed to monitor the rotation of radio pulsars over time spans of days to years. The observations are obtained using the Parkes 64-m and 12-m radio telescopes by Australian and international high school students. These students learn the basis of radio astronomy and undertake small projects with their observations. The data are fully calibrated and obtained with the state-of-the-art pulsar hardware available at Parkes. The final data sets are archived and are currently being used to carry out studies of 1) pulsar glitches, 2) timing noise, 3) pulse profile stability over long time scales and 4) the extreme nulling phenomenon. The data are also included in other projects such as gamma-ray observatory support and for the Parkes Pulsar Timing Array project. In this paper we describe the current status of the project and present the first scientific results from the Parkes 12-m radio telescope. We emphasise that this project offers a straightforward means to enthuse high school students and the general public about radio astronomy while obtaining scientifically valuable data sets.
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32

Roebuck, D. J. "Klippel-Trénaunay and Parkes-Weber syndromes." American Journal of Roentgenology 169, no. 1 (July 1997): 311–12. http://dx.doi.org/10.2214/ajr.169.1.9207562.

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33

Fyfe, Julian. "Recycled Water for a Greener Parkes." Water e-Journal 6, no. 2 (2021): 1–14. http://dx.doi.org/10.21139/wej.2021.010.

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34

HOBBS, GEORGE. "THE PARKES PULSAR TIMING ARRAY PROJECT." Publications of The Korean Astronomical Society 30, no. 2 (September 30, 2015): 577–81. http://dx.doi.org/10.5303/pkas.2015.30.2.577.

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35

Whiting, M. T., R. L. Webster, and P. J. Francis. "Red synchrotron jets in Parkes quasars." Monthly Notices of the Royal Astronomical Society 323, no. 3 (May 21, 2001): 718–32. http://dx.doi.org/10.1046/j.1365-8711.2001.04287.x.

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36

Bojakowski, Krzysztof, Gabriela Janusz, Iwona Grabowska, Oliwia Zegrocka-Stendel, Agnieszka Surowiecka-Pastewka, Magdalena Kowalewska, Dorota Maciejko, and Katarzyna Koziak. "Rat Model of Parkes Weber Syndrome." PLOS ONE 10, no. 7 (July 28, 2015): e0133752. http://dx.doi.org/10.1371/journal.pone.0133752.

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37

Janssens, P. "Shorter notice. Understanding Contemporary Germany. Parkes." English Historical Review 114, no. 455 (February 1999): 276–77. http://dx.doi.org/10.1093/enghis/114.455.276.

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38

Staveley-Smith, L., W. E. Wilson, T. S. Bird, M. J. Disney, R. D. Ekers, K. C. Freeman, R. F. Haynes, et al. "The Parkes 21 cm Multibeam Receiver." Publications of the Astronomical Society of Australia 13, no. 3 (June 1996): 243–48. http://dx.doi.org/10.1017/s1323358000020919.

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Several extragalactic HI surveys using a λ21 cm 13-beam focal plane array will begin in early 1997 using the Parkes 64 m telescope. These surveys are designed to detect efficiently nearby galaxies that have failed to be identified optically because of low optical surface brightness or high optical extinction. We discuss scientific and technical aspects of the multibeam receiver, including astronomical objectives, feed, receiver and correlator design and data acquisition. A comparison with other telescopes shows that the Parkes multibeam receiver has significant speed advantages for any large-area λ21 cm galaxy survey in the velocity range range 0–14000 km s−1.
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39

Backus, Peter R. "The Phoenix search results at Parkes." Acta Astronautica 42, no. 10-12 (May 1998): 651–54. http://dx.doi.org/10.1016/s0094-5765(98)00020-4.

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40

Manchester, R. N. "The Parkes Pulsar Timing Array Project." Proceedings of the International Astronomical Union 5, H15 (November 2009): 233. http://dx.doi.org/10.1017/s1743921310008987.

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AbstractThe Parkes Pulsar Timing Array project is timing 20 millisecond pulsars with the aims of detecting gravitational waves, establishing a time scale based on pulsar periods and improving solar-system ephemerides.
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41

Janssens, P. "Shorter notice. Understanding Contemporary Germany. Parkes." English Historical Review 114, no. 454 (February 1, 1999): 276–77. http://dx.doi.org/10.1093/ehr/114.454.276.

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42

Janssens, P. "Shorter notice. Understanding Contemporary Germany. Parkes." English Historical Review 114, no. 455 (February 1, 1999): 276–77. http://dx.doi.org/10.1093/ehr/114.455.276.

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43

Webster, R. L., V. Kilborn, J. C. O’Brien, L. Staveley-Smith, M. E. Putman, and G. Banks. "The Parkes Multibeam Blind HI Survey." International Astronomical Union Colloquium 171 (1999): 291–98. http://dx.doi.org/10.1017/s0252921100054464.

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AbstractA thirteen-beam HI receiver has been constructed for the Parkes radio telescope. When this instrument is used in active scanning mode, it can rapidly survey large areas of sky, with a relatively uniform sensitivity. The Multibeam Working Group, comprising about 30 astronomers from more than a dozen institutions, is undertaking a blind HI survey of the entire southern sky. The status of the survey is described, with some of the first scientific results.
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44

Wright, Alan E., Niven J. Tasker, Ann Savage, and Alan E. Vaughan. "The Parkes-MIT-NRAO Radio Surveys." Symposium - International Astronomical Union 175 (1996): 507–12. http://dx.doi.org/10.1017/s0074180900081663.

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During 1990, the Parkes radio telescope made a new, deep survey of the southern sky at 4850 MHz (the PMN Survey: see e.g. Griffith and Wright, 1993; Wright et al., 1994). The declination coverage of the survey was from δ = −87° to +10°. The flux limit of the survey was around 30 mJy, although dependent on declination. This survey increased the number of known, southern radio sources by a factor of about 6 to over 65,000.
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45

Espitia, O., J. Connault, R. Clairand, A. S. Boureau, P. Pottier, M. Hamidou, and B. Planchon. "Syndrome de Parkes-Weber et POEMS." La Revue de Médecine Interne 31 (June 2010): S111. http://dx.doi.org/10.1016/j.revmed.2010.03.151.

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46

Bhat, N. D. R., F. Camilo, J. M. Cordes, D. J. Nice, D. R. Lorimer, and S. Chatterjee. "Arecibo observations of Parkes multibeam pulsars." Journal of Astrophysics and Astronomy 23, no. 1-2 (March 2002): 53–57. http://dx.doi.org/10.1007/bf02702465.

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47

E Wright, Alan. "From the Parkes Catalogue to COMRAD." Australian Journal of Physics 47, no. 5 (1994): 585. http://dx.doi.org/10.1071/ph940585.

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I present a brief description of John Bolton's work in establishing the Parkes Catalogue as the first of the major radio source databases. I also discuss how this Catalogue evolved over the years from a paper card format to a sophisticated computer database.
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48

Tucker, W. F. G., and C. I. Harrington. "(7) Klippel-Trenaunay-Parkes-Weber syndrome." British Journal of Dermatology 115, s30 (July 1986): 49–50. http://dx.doi.org/10.1111/j.1365-2133.1986.tb07702.x.

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49

Burgay, M., B. C. Joshi, N. D'Amico, A. Possenti, A. G. Lyne, R. N. Manchester, M. A. McLaughlin, M. Kramer, F. Camilo, and P. C. C. Freire. "The Parkes High-Latitude pulsar survey." Monthly Notices of the Royal Astronomical Society 368, no. 1 (May 1, 2006): 283–92. http://dx.doi.org/10.1111/j.1365-2966.2006.10100.x.

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Rojas Esquivel, Diego José, Elena Marín Manzano, Nieves Aleicel Concepción, Juan Carlos Lopéz Gutierréz, and Luis Riera de Cubas. "Nodular Proliferation in Parkes Weber Syndrome." Annals of Vascular Surgery 38 (January 2017): 321.e1–321.e4. http://dx.doi.org/10.1016/j.avsg.2016.06.015.

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