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Sá-Leite AR, Lago S. The role of word form in gender processing during lexical access: A theoretical review and novel proposal in language comprehension. Psychon Bull Rev 2024:10.3758/s13423-023-02426-8. [PMID: 38383840 DOI: 10.3758/s13423-023-02426-8] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Accepted: 11/14/2023] [Indexed: 02/23/2024]
Abstract
In contrast to language production, there are few comprehension models of the representation and use of grammatical gender in long-term memory. To bridge this gap, we conducted a systematic review of empirical studies on the role of gender-form regularities in the recognition of nouns in isolation and within sentences. The results of a final sample of 40 studies suggest that there are two routes for the retrieval of gender during real-time comprehension: a form-based route and a lexical-based route. Our review indicates that the use of these routes depends on the degree of gender transparency of the language and the degree of overtness of the experimental paradigm. To accommodate these findings, we incorporate a dual-route mechanism within a general model of lexical access in comprehension, the AUSTRAL (Activation Using Structurally Tiered Representations and Lemmas) model, and identify directions for future research.
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Affiliation(s)
- A R Sá-Leite
- Institut für Romanische Sprachen und Literaturen, Goethe University Frankfurt, Frankfurt, Germany.
- Cognitive Processes and Behaviour Research Group, Department of Social Psychology, Basic Psychology and Methodology, University of Santiago de Compostela, 15782, Santiago de Compostela, Spain.
| | - S Lago
- Institut für Romanische Sprachen und Literaturen, Goethe University Frankfurt, Frankfurt, Germany
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McCallum L, Chin Chuan L, Krásná H, McCallum J, Böhm J, McCarthy T, Gruber J, Schartner M, Quick J, Rogers A. The Australian mixed-mode observing program. J Geod 2022; 96:67. [PMID: 36188100 PMCID: PMC9515051 DOI: 10.1007/s00190-022-01657-2] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 12/09/2021] [Accepted: 08/22/2022] [Indexed: 06/16/2023]
Abstract
Global geodetic VLBI is upgrading to its next-generation observing system, VGOS. This upgrade has turned out to be a process over multiple years, until VGOS reaches its full capabilities with the envisaged continuous observations. Until then, for the Australian stations, the upgrade means ceasing their legacy S/X observations, leaving a large gap in the global network as well as in the station time series. The Australian mixed-mode observing program is a series of sessions where the VGOS stations in Hobart and Katherine observe legacy S/X VLBI together with other stations in the region. This paper describes the technical details of these observations and their processing strategies and discusses their suitability for geodetic results by comparison with those of standard legacy S/X sessions. The presented mixed-mode sessions allow a continuation of the station time series, a benefit for the stations themselves as well as for future realisations of the terrestrial and celestial reference frames. A novel mode of observing is introduced and tested. The results are promising and it is suggested for acceptance into standard legacy S/X IVS observations, overcoming current gaps in the network due to VGOS upgrades and preventing a worsening of global results otherwise.
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Affiliation(s)
- Lucia McCallum
- University of Tasmania, Private Bag 37, Hobart, 7001 Australia
| | - Lim Chin Chuan
- University of Tasmania, Private Bag 37, Hobart, 7001 Australia
| | - Hana Krásná
- Technische Universität Wien, Vienna, Austria
| | - Jamie McCallum
- University of Tasmania, Private Bag 37, Hobart, 7001 Australia
| | | | - Tiege McCarthy
- University of Tasmania, Private Bag 37, Hobart, 7001 Australia
| | | | | | - Jonathan Quick
- Hartebeesthoek Radio Astronomy Observatory, Krugersdorp, South Africa
| | - Axl Rogers
- Auckland University of Technology, Auckland, New Zealand
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Plank L, Lovell JEJ, McCallum JN, Mayer D, Reynolds C, Quick J, Weston S, Titov O, Shabala SS, Böhm J, Natusch T, Nickola M, Gulyaev S. The AUSTRAL VLBI observing program. J Geod 2016; 91:803-817. [PMID: 32025105 PMCID: PMC6979662 DOI: 10.1007/s00190-016-0949-y] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 05/13/2016] [Accepted: 08/19/2016] [Indexed: 06/10/2023]
Abstract
The AUSTRAL observing program was started in 2011, performing geodetic and astrometric very long baseline interferometry (VLBI) sessions using the new Australian AuScope VLBI antennas at Hobart, Katherine, and Yarragadee, with contribution from the Warkworth (New Zealand) 12 m and Hartebeesthoek (South Africa) 15 m antennas to make a southern hemisphere array of telescopes with similar design and capability. Designed in the style of the next-generation VLBI system, these small and fast antennas allow for a new way of observing, comprising higher data rates and more observations than the standard observing sessions coordinated by the International VLBI Service for Geodesy and Astrometry (IVS). In this contribution, the continuous development of the AUSTRAL sessions is described, leading to an improvement of the results in terms of baseline length repeatabilities by a factor of two since the start of this program. The focus is on the scheduling strategy and increased number of observations, aspects of automated operation, and data logistics, as well as results of the 151 AUSTRAL sessions performed so far. The high number of the AUSTRAL sessions makes them an important contributor to VLBI end-products, such as the terrestrial and celestial reference frames and Earth orientation parameters. We compare AUSTRAL results with other IVS sessions and discuss their suitability for the determination of baselines, station coordinates, source coordinates, and Earth orientation parameters.
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Affiliation(s)
- L. Plank
- University of Tasmania, Private Bag 37, Hobart, 7001 Australia
| | - J. E. J. Lovell
- University of Tasmania, Private Bag 37, Hobart, 7001 Australia
| | - J. N. McCallum
- University of Tasmania, Private Bag 37, Hobart, 7001 Australia
| | - D. Mayer
- Technische Universität Wien, Vienna, Austria
| | - C. Reynolds
- ICRAR/Curtin University, Bentley, Australia
- Present Address: CSIRO Astronomy and Space Science, Kensington, Australia
| | - J. Quick
- Hartebeesthoek Radio Astronomy Observatory, Krugersdorp, South Africa
| | - S. Weston
- Institute for Radio Astronomy and Space Research, Auckland University of Technology, Auckland, New Zealand
| | - O. Titov
- Geoscience Australia, Canberra, Australia
| | - S. S. Shabala
- University of Tasmania, Private Bag 37, Hobart, 7001 Australia
| | - J. Böhm
- Technische Universität Wien, Vienna, Austria
| | - T. Natusch
- Institute for Radio Astronomy and Space Research, Auckland University of Technology, Auckland, New Zealand
| | - M. Nickola
- Hartebeesthoek Radio Astronomy Observatory, Krugersdorp, South Africa
| | - S. Gulyaev
- Institute for Radio Astronomy and Space Research, Auckland University of Technology, Auckland, New Zealand
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