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Does Gender Differences Exist in Online Newspaper Consumption among Pakistani Youth? 巴基斯坦青年网络报纸消费存在性别差异吗?
IF 0.4 Q4 COMMUNICATION Pub Date : 2021-01-01 DOI: 10.26623/themessenger.v13i1.2552
M. R. Pahore, Sumera Memon, Norsiah Abdul Hamid, Awan Ismail
It is no doubt that the popularity of ICTs in developing countries has increased the use of internet-related social networking sites along with news information consumption, production, and news distribution. As such, there has been a huge shift in the trend of news consumption from conventional media to an online newspaper. It has also been tocied that male and female youth are equally inclined to use internet for different reasons. Thus, in recent times scholars have started inspecting online newspaper consumption-related behavior, with an emphasis on young boys and girls in a way this group is one that can last longer. However, very few studies have paid attention to gender differences in motivating factors for online newspaper consumption in Pakistan. To address this gap, by using a cross-sectional design, a survey was conducted on university students from three public universities of Pakistan because university students are tech-savvy and mostly internet users. These three universities are representative of rural and urban population. Questionnaires were used to collect data which was analyzed using Partial Least Squares-Multi Group Analysis. Hypothesized results discovered that in terms of online newspaper consumption, there was no gender differences found in online newspaper consumption among Pakistani youth.
毫无疑问,信息通信技术在发展中国家的普及增加了与互联网相关的社交网站的使用,同时也增加了新闻信息的消费、生产和传播。因此,从传统媒体到网络报纸的新闻消费趋势发生了巨大的转变。研究还发现,男性和女性年轻人同样倾向于出于不同的原因使用互联网。因此,近年来学者们开始研究与在线报纸消费相关的行为,并在某种程度上强调年轻的男孩和女孩是一个可以持续更长时间的群体。然而,很少有研究关注巴基斯坦在线报纸消费激励因素的性别差异。为了解决这一差距,通过使用横断面设计,对巴基斯坦三所公立大学的大学生进行了一项调查,因为大学生是精通技术的,大多数是互联网用户。这三所大学在农村和城市人口中都具有代表性。采用问卷调查法收集数据,采用偏最小二乘-多组分析法进行分析。假设结果发现,在网络报纸消费方面,巴基斯坦青年的网络报纸消费没有性别差异。
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引用次数: 0
SUPER — AGN feedback at cosmic noon: a multi-phase and multi-scale challenge 宇宙正午的超级AGN反馈:一个多阶段和多尺度的挑战
IF 0.4 Q4 COMMUNICATION Pub Date : 2021-01-01 DOI: 10.18727/0722-6691/5222
V. Mainieri, C. Circosta, D. Kakkad, Michele Perna, G. Vietri, A. Bongiorno, M. Brusa, S. Carniani, C. Cicone, F. Civano, A. Comastri, G. Cresci, C. Feruglio, F. Fiore, A. Georgakakis, C. Harrison, B. Husemann, A. Lamastra, I. Lamperti, G. Lanzuisi, F. Mannucci, A. Marconi, N. Menci, A. Merloni, H. Netzer, P. Padovani, E. Piconcelli, A. Puglisi, M. Salvato, J. Scholtz, M. Schramm, J. Silverman, C. Vignali, G. Zamorani, L. Zappacosta
Theoretical models of galaxy evolution suggest that galaxy-wide outflows driven by active galactic nuclei (AGN), one of the so-called AGN-feedback mechanisms, are a fundamental process affecting the bulk of the baryons in the Universe. While the presence of such outflows out to kpc scales is now undisputed, their impact on the star formation, gas content and kinematics of the host galaxy is hotly debated. Here we report on the results from our Large Programme SUPER, which used the Spectrograph for INtegral Field Observations in the Near INfrared (SINFONI) on the Very Large Telescope (VLT) to carry out the first statistically sound high-spatialresolution investigation of AGN outflows at z ~ 2, covering four orders of magnitude in AGN bolometric luminosity.
星系演化的理论模型表明,由活动星系核(AGN)驱动的全星系范围的外流,即所谓的AGN反馈机制之一,是影响宇宙中大部分重子的基本过程。虽然这种kpc尺度的外流物的存在现在是无可争议的,但它们对恒星形成、气体含量和宿主星系运动学的影响仍在激烈争论中。在这里,我们报告了我们的大型项目SUPER的结果,该项目使用甚大望远镜(VLT)上的近红外积分场观测光谱仪(SINFONI)对z ~ 2的AGN流出进行了第一次统计上合理的高空间分辨率调查,覆盖了AGN的4个数量级的热光度。
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引用次数: 1
An Era Comes to an End: The Legacy of LABOCA at APEX 一个时代的终结:LABOCA在APEX的遗产
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-09-01 DOI: 10.18727/0722-6691/5205
A. Lundgren, C. Breuck, G. Siringo, A. Weiss, C. Agurto, F. Azagra, A. Belloche, M. Dumke, C. Durán, A. Eckart, E. González, R. Güsten, Á. Hacar, A. Kovács, E. Kreysa, F. Mac-Auliffe, Miguel Ángel Martínez, K. Menten, F. Montenegro, L. Nyman, R. Parra, J. Perez-Beaupuits, V. Révéret, C. Risacher, F. Schuller, T. Stanke, K. Torstensson, Percy Venegas, H. Wiesemeyer, F. Wyrowski
and the Hubble Deep Field (Smail et al., 1997; Hughes et al., 1998). Its main limitation was the small field of view and further progress was only possible by increasing the bolometer array sizes by an order of magnitude. This motivated the bolometer development group led by Ernst Kreysa at the Max Planck Institute for Radio Astronomy in Bonn (MPIfR), who had already provided the community with MAMBO, SIMBA and its line of predecessors, to build LABOCA (Siringo et al., 2009) for the new Atacama Pathfinder Experiment (APEX) 12-m submillimetre telescope as one of its main facility instruments (Güsten et al., 2006). With as many as 295 bolometers covering a circular field of 11.4 arcminutes, LABOCA would remain the largest submillimetre array till the SCUBA-2 instrument became available on the JCMT in 2012 (Holland et al., 2013). Being installed on APEX, LABOCA could also make optimal use of the excellent weather conditions on Chajnantor, where the 870-μm atmospheric window is observable for almost two-thirds of the available weather conditions (Otarola et al., 2019). In addition, seeing the same sky as ALMA optimised LABOCA’s synergy as the ideal source finder for ALMA. Andreas Lundgren1 Carlos De Breuck1 Giorgio Siringo1 Axel Weiß2 Claudio Agurto1 Francisco Azagra1 Arnaud Belloche2 Michael Dumke1 Carlos Durán1 Andreas Eckart2 Edouard González1 Rolf Güsten2 Alvaro Hacar3 Attila Kovács 4 Ernst Kreysa2 Felipe Mac-Auliffe1 Mauricio Martínez1 Karl M. Menten2 Francisco Montenegro1 Lars-Åke Nyman1 Rodrigo Parra1 Juan Pablo Pérez-Beaupuits1 Vincent Reveret5, 6 Christophe Risacher7 Frédéric Schuller8 Thomas Stanke1 Karl Torstensson1 Paulina Venegas1 Helmut Wiesemeyer2 Friedrich Wyrowski2
和哈勃深空(small et al., 1997);Hughes et al., 1998)。它的主要限制是视野小,进一步的进展只能通过增加一个数量级的辐射热计阵列的尺寸。这促使波恩马克斯普朗克射电天文研究所(MPIfR)的Ernst Kreysa领导的辐射热计开发小组为新的阿塔卡马探路者实验(APEX)建造LABOCA (Siringo等人,2009年),作为其主要设施仪器之一(g斯坦等人,2006年),该小组已经为社区提供了MAMBO, SIMBA及其前身系列。多达295个辐射热计覆盖11.4弧分的圆形场,LABOCA将保持最大的亚毫米阵列,直到2012年在JCMT上使用SCUBA-2仪器(Holland et al, 2013)。安装在APEX上,LABOCA还可以最佳地利用Chajnantor上良好的天气条件,在那里几乎三分之二的可用天气条件下都可以观察到870 μm的大气窗口(Otarola等人,2019)。此外,看到与ALMA相同的天空,优化了LABOCA作为ALMA理想的光源发现者的协同作用。Andreas lundgre1 Carlos De breuc1 Giorgio Siringo1 Axel wei1 Claudio Agurto1 Francisco Azagra1 Arnaud Belloche2 Michael Dumke1 Carlos Durán1 Andreas eckar2 Edouard González1 Rolf g sten2 Alvaro Hacar3 Attila Kovács 4 Ernst kreys2 Felipe macauliff1 Mauricio Martínez1 Karl M. Menten2 Francisco montegro1 Lars-Åke Nyman1 Rodrigo Parra1 Juan Pablo p - beaupuits1 Vincent Reveret5,克里斯托夫·里切尔·弗莱姆·萨勒克·托马斯·斯坦克·卡尔·托尔斯滕森·宝琳娜·维内加斯·赫尔穆特·维泽迈耶·弗里德里希·维罗斯基
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引用次数: 0
NGTS - Uncovering New Worlds with Ultra-Precise Photometry NGTS -用超精确光度法发现新世界
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-09-01 DOI: 10.18727/0722-6691/5208
D. Bayliss, P. Wheatley, R. West, D. Pollacco, D. Anderson, David J Armstrong, E. Bryant, H. Cegla, B. Cooke, B. Gänsicke, S. Gill, J. Jackman, T. Loudon, J. McCormac, J. Acton, M. Burleigh, S. Casewell, M. Goad, B. Henderson, A. Hogan, L. Raynard, R. Tilbrook, J. Briegal, E. Gillen, D. Queloz, G. Smith, P. Eigmüller, Alexis M. S. Smith, C. Watson, F. Bouchy, M. Lendl, L. Nielsen, S. Udry, J. Jenkins, J. Vines, A. Jordán, M. Moyano, M. Günther
The Messenger 181 – Quarter 3 | 2020 Daniel Bayliss1 Peter Wheatley1 Richard West1 Don Pollacco1 David R. Anderson1 David Armstrong1 Edward Bryant1 Heather Cegla1 Benjamin Cooke1 Boris Gänsicke1 Samuel Gill1 James Jackman1 Tom Loudon1 James McCormac1 Jack Acton2 Matthew R. Burleigh2 Sarah Casewell2 Michael Goad2 Beth Henderson2 Aleisha Hogan2 Liam Raynard2 Rosanna H. Tilbrook2 Joshua Briegal3 Edward Gillen3 Didier Queloz3 Gareth Smith3 Philipp Eigmüller4 Alexis M. S. Smith4 Christopher Watson5 François Bouchy6 Monika Lendl6 Louise D. Nielsen6 Stéphane Udry6 James Jenkins7 José Vines7 Andrés Jordán8 Maximiliano Moyano9 Maximilian N. Günther10
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引用次数: 0
The ESO Cosmic Duologues
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-09-01 DOI: 10.18727/0722-6691/5209
G. Beccari, H. Boffin
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引用次数: 0
ESPRESSO Science Verification ESPRESSO科学验证
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-09-01 DOI: 10.18727/0722-6691/5204
B. Leibundgut, R. Anderson, T. Berg, S. Cristiani, P. Figueira, G. Curto, A. Mehner, E. Sedaghati, J. Pritchard, M. Wittkowski
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引用次数: 0
ALMA Data Quality Assurance and the Products it Delivers - The Contribution of the European ARC ALMA数据质量保证和它提供的产品-欧洲ARC的贡献
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-09-01 DOI: 10.18727/0722-6691/5206
D. Petry, T. Stanke, A. Biggs, M. D. Trigo, F. Guglielmetti, E. Hatziminaoglou, E. V. Kampen, L. Maud, A. Miotello, G. Popping, S. Randall, F. Stoehr, M. Zwaan
From its inception, the Atacama Large Millimeter/submillimeter Array (ALMA) was intended to be accessible to all astronomers, including those who are more used to carrying out their research at other wavelengths. Since the beginning of science observations in September 2011, ALMA has therefore applied a comprehensive Quality Assurance (QA) process to the observed data before delivering them to the principal investigators (PIs). This huge investment, unique for a ground-based (non-survey) observatory of this calibre, results in fully calibrated datasets as well as high-quality images that allow the PIs to assess the quality of their data upon delivery and that provide an advanced starting point for the scientific analysis. In this article we provide a summary of the purpose and status of ALMA QA, a brief description of the QA process and the resulting ALMA data products, and a discussion of how the ALMA user profits from them.
从一开始,阿塔卡马大型毫米波/亚毫米波阵列(ALMA)就打算向所有天文学家开放,包括那些更习惯于在其他波长进行研究的天文学家。因此,自2011年9月开始科学观测以来,ALMA在将观测数据交付给主要研究人员之前,对观测数据采用了全面的质量保证(QA)流程。这种巨大的投资,对于这种口径的地面(非调查)天文台来说是独一无二的,结果是完全校准的数据集以及高质量的图像,使pi能够在交付时评估其数据的质量,并为科学分析提供了一个先进的起点。本文概述了ALMA质量保证的目的和现状,简要描述了质量保证过程和由此产生的ALMA数据产品,并讨论了ALMA用户如何从中获益。
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引用次数: 2
Fellows at ESO ESO研究员
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-09-01 DOI: 10.18727/0722-6691/5213
M. Gendron-Marsolais, M. Jones
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引用次数: 0
Report on the ESO Workshop "A Synoptic View of the Magellanic Clouds: VMC, Gaia, and Beyond" ESO研讨会报告“麦哲伦云的概观:VMC、盖亚和更远”
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-09-01 DOI: 10.18727/0722-6691/5211
M. Cioni, M. Romaniello, R. I. Anderson
The year 2019 marked the quincentenary of the arrival in the southern hemisphere of Ferdinand Magellan, the namesake of the Magellanic Clouds, our nearest example of dwarf galaxies in the early stages of a minor merging event. These galaxies have been firmly established as laboratories for the study of variable stars, stellar evolution, and galaxy interaction, as well as being anchors for the extragalactic distance scale. The goal of this conference was to provide fertile ground for shaping future research related to the Magellanic Clouds by combining state-of-the-art results based on advanced observational programmes with discussions of the highly multiplexed wide-field spectroscopic surveys that will come online in the 2020s.
2019年是费迪南德·麦哲伦(Ferdinand Magellan)抵达南半球的50周年纪念,麦哲伦星云与我们最近的矮星系处于一次小型合并事件的早期阶段。这些星系已经被牢固地建立为研究变星、恒星演化和星系相互作用的实验室,同时也是星系外距离尺度的锚点。本次会议的目标是通过将基于先进观测计划的最新成果与将于2020年代在线的高复用宽视场光谱调查的讨论相结合,为塑造与麦哲伦云相关的未来研究提供肥沃的土壤。
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引用次数: 0
The Use of Social Media in Searching for Information about Papua 利用社交媒体搜索巴布亚信息
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-07-31 DOI: 10.26623/themessenger.v12i2.1939
Panji Dwi Ashrianto, Senja Yustitia
The use of social media in searching for information relating to political issues has become immensely crucial since in those domains the information appearing is often biased and dominated by certain parties or groups. One of the political information that has frequently emerged in Indonesia is about Papua. The significance of this research because Papua is a crucial problem in Indonesian history, and its conversation has continued, especially in social media. This study intends to examine the use of social media in searching for information about Papua. That is a novelty of research because no one has examined Papua in terms of the use of social media. The Uses and Gratification Theory is used in the study with a mixed method approach as both quantitative and qualitative data were concurrently utilized. Quantitative data obtained from a questionnaire distributed to 100 UPN "Veteran" Yogyakarta students. UPN was selected because they are a state defense campus and provide state defense material to students. While qualitative data from in-depth interviews with some sources. In conclusion, social media cannot be used as the only media for seeking information about Papua. Audiences actively choose the media based on their motivation, experience, and satisfaction.
利用社交媒体搜索与政治问题有关的信息已变得极其重要,因为在这些领域中出现的信息往往是有偏见的,并由某些政党或团体主导。印度尼西亚经常出现的政治信息之一是关于巴布亚的。这项研究的重要性在于,巴布亚岛是印尼历史上的一个关键问题,有关它的讨论一直在继续,尤其是在社交媒体上。本研究旨在调查社交媒体在搜索巴布亚信息方面的使用情况。这是一项新颖的研究,因为没有人从社交媒体使用的角度研究过巴布亚。使用与满足理论在研究中使用混合方法方法,同时使用定量和定性数据。定量数据来自分发给100名UPN“资深”日惹学生的问卷。UPN被选中是因为他们是国家国防校园,并为学生提供国家国防材料。而定性数据则来自一些来源的深度访谈。综上所述,社交媒体不能作为寻求有关巴布亚信息的唯一媒体。受众根据自己的动机、体验和满意度来主动选择媒介。
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引用次数: 6
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Jurnal The Messenger
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