1,725,384 research outputs found
King, I N, 3894
No full textThis record was harvested from a previous catalogue system and will be withdrawn in 2025. Information in this record may be superseded or incomplete. Visit this record in UMA's new catalogue at: https://archives.library.unimelb.edu.au/nodes/view/397207Surname: KING. Given Name(s) or Initials: I N. Military Service Number or Last Known Location: 3894. Missing, Wounded and Prisoner of War Enquiry Card Index Number: SEA-3001.234451
Item: [2016.0049.29500] "King, I N, 3894
Going Beyond Counting First Authors in Author Co-citation Analysis
Get PDFThe present study examines one of the fundamental aspects of author co-citation analysis (ACA) - the way co-citation
counts are defined. Co-citation counting provides the data on which all subsequent statistical analyses and mappings
are based, and we compare ACA results based on two different types of co-citation counting - the traditional type that
only counts the first one among a cited work's authors on the one hand and a non-traditional type that takes into
account the first 5 authors of a cited work on the other hand. Results indicate that the picture produced through this non-traditional author co-citation counting contains more coherent author groups and is therefore considerably clearer. However, this picture represents fewer specialties in the research field being studied than that produced through the traditional first-author co-citation counting when the same number of top-ranked authors is selected and analyzed. Reasons for these effects are discussed
Variations on the Author
Get PDF“Variations on the Author” discusses two of Eduardo Coutinho’s recent films (Um Dia na Vida, from 2010, and Últimas Conversas, posthumously released in 2015) and their contribution to the general question of documentary authorship. The director’s filmography is characterized by a consistent yet self-effacing form of authorial self-inscription: Coutinho often features as an interviewer that rather than express opinions propels discourses; an interviewer that is good at listening. This mode of self-inscription characterizes him as an author who is not expressive but who is nonetheless markedly present on the screen. In Um Dia na Vida, however, Coutinho is completely absent form the image, while Últimas Conversas, on the contrary, includes a confessional prologue that moves the director from the margins to the center of his films. This article examines the ways in which these works stand out in the filmography of a director who offers new insights into the notion of cinematic authorship
Appropriate Similarity Measures for Author Cocitation Analysis
Get PDFWe provide a number of new insights into the methodological discussion about author cocitation analysis. We first argue that the use of the Pearson correlation for measuring the similarity between authors’ cocitation profiles is not very satisfactory. We then discuss what kind of similarity measures may be used as an alternative to the Pearson correlation. We consider three similarity measures in particular. One is the well-known cosine. The other two similarity measures have not been used before in the bibliometric literature. Finally, we show by means of an example that our findings have a high practical relevance.information science;Pearson correlation;cosine;similarity measure;author cocitation analysis
PEMAHAMAN HADIS RIWAYAT AHMAD NO. 3894 TENTANG DIANGKATNYA ILMU SEBAGAI TANDA KIAMAT STUDI MA’ANIL HADIS
Get PDFKehidupan ini bersifat fana dan kehidupan abadi merupakan kehidupan setelah terjadiya kehancuran. Kiamat di dalam al-Qur’an dijelaskan terbagi menjadi dua: kiamat sugra dan kiamat kubra. Allah memberikan beberapa tanda atau ciri-ciri datangnya hari kiamat di dalam al-Qur’an sebagi salah satu bentuk kehati-hatian manusia dalam mengenali hari kiamat. Tanda-tanda kiamat bisa membagi tanda-tanda kiamat menjadi dua pembagian diantaranya.
Tanda-tanda sugra merupakan peristiwa yang telah terjadi dan masih berlangsung serta kadang terulang sampai saat ini. Tanda-tanda kubra ini sudah tidak bisa di ganggu gugat. Al-Qur’an dan hadis juga menjelaskannya oleh karenanya. Rumusan masalah penelitan ini yaitu Bagaimana pemahaman tentang di angkatnya ilmu sebagai tanda kiamat dalam hadis riwayat Ahmad no. 3894, Bagaimana kontekstualisasi hadis Ahmad no. 3894 tentang di angkatnya ilmu sebagai tanda kiamat?
Metode penelitian yang digunakan adalah library research, yaitu mengumpukan data dari berbagai sumber. Data primer penulis yaitu al-Kutub al-Tis’ah baik berbentuk buku maupun software, sedangkan data sekunder yang penulis gunakan yaitu seperti buku, jurnal, artikel, skripsi dll. Metode pengumpulan data menggunakan metode dokumentasi dan analisis deskriptif sehingga memberikan pemahaman yang lebih komprehensif tentang pertanyaan penelitian. Penulis menggunakan metode yusuf al-Qardhawi dalam meneliti hadis riwayat ahmad no.3894.
Pemahama hadis riwayat Ahmad no. 3894, yang berbicara tentang tanda kiamat dengan diangkatnya ilmu. Yaitu dengan mewafatkan orang yang memiliki ilmu dan mengamalkannya dan memunculkan orang-orang yang memiliki pengetahuan yang sama, akan tetapi ilmu tersebut menjadi sia-sia karena tidak adanya keistimewaan seperti orang yang sebelumnya
NGC 3894: a young radio galaxy seen by
Get PDFContext. According to radiative models, radio galaxies may produce γ-ray emission from the first stages of their evolution. However, very few such galaxies have been detected by the Fermi Large Area Telescope (LAT) so far.
Aims. NGC 3894 is a nearby (z = 0.0108) object that belongs to the class of compact symmetric objects (CSOs, i.e., the most compact and youngest radio galaxies), which is associated with a γ-ray counterpart in the Fourth Fermi-LAT source catalog. Here we present a study of the source in the γ-ray and radio bands aimed at investigating its high-energy emission and assess its young nature.
Methods. We analyzed 10.8 years of Fermi-LAT data between 100 MeV and 300 GeV and determined the spectral and variability characteristics of the source. Multi-epoch very long baseline array (VLBA) observations between 5 and 15 GHz over a period of 35years were used to study the radio morphology of NGC 3894 and its evolution.
Results. NGC 3894 is detected in γ-rays with a significance >9σ over the full period, and no significant variability has been observed in the γ-ray flux on a yearly time-scale. The spectrum is modeled with a flat power law (Γ = 2.0 ± 0.1) and a flux on the order of 2.2 × 10−9 ph cm−2 s−1. For the first time, the VLBA data allow us to constrain with high precision the apparent velocity of the jet and counter-jet side to be βapp, NW = 0.132 ± 0.004 and βapp, SE = 0.065 ± 0.003, respectively.
Conclusions. Fermi-LAT and VLBA results favor the youth scenario for the inner structure of this object, with an estimated dynamical age of 59 ± 5 years. The estimated range of viewing angle (10° < θ < 21°) does not exclude a possible jet-like origin of the γ-ray emission
NGC 3894: a young radio galaxy seen by Fermi-LAT
Get PDFContext. According to radiative models, radio galaxies may produce γ-ray emission from the first stages of their evolution. However, very few such galaxies have been detected by the Fermi Large Area Telescope (LAT) so far.
Aims: NGC 3894 is a nearby (z = 0.0108) object that belongs to the class of compact symmetric objects (CSOs, i.e., the most compact and youngest radio galaxies), which is associated with a γ-ray counterpart in the Fourth Fermi-LAT source catalog. Here we present a study of the source in the γ-ray and radio bands aimed at investigating its high-energy emission and assess its young nature.
Methods: We analyzed 10.8 years of Fermi-LAT data between 100 MeV and 300 GeV and determined the spectral and variability characteristics of the source. Multi-epoch very long baseline array (VLBA) observations between 5 and 15 GHz over a period of 35years were used to study the radio morphology of NGC 3894 and its evolution.
Results: NGC 3894 is detected in γ-rays with a significance >9σ over the full period, and no significant variability has been observed in the γ-ray flux on a yearly time-scale. The spectrum is modeled with a flat power law (Γ = 2.0 ± 0.1) and a flux on the order of 2.2 × 10-9 ph cm-2 s-1. For the first time, the VLBA data allow us to constrain with high precision the apparent velocity of the jet and counter-jet side to be βapp, NW = 0.132 ± 0.004 and βapp, SE = 0.065 ± 0.003, respectively.
Conclusions: Fermi-LAT and VLBA results favor the youth scenario for the inner structure of this object, with an estimated dynamical age of 59 ± 5 years. The estimated range of viewing angle (10° < θ < 21°) does not exclude a possible jet-like origin of the γ-ray emission
- …
