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Such fakes, created as social network profiles, satirize politicians or political organizations by impersonating them. I identify two modes of faking: I map the interactions of the fakes and their public s along two axes: Thirdly, I argue for fakeness as a playful, yet powerful critique of the political and its pretense to authenticity.
By focusing on how the creators of fake accounts manage their fakeness and interact with their public sthis paper provides insights on the participatory nature of satire and on the characteristics of online publics.
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University of Virginia, USA; 2: University of California - Berkeley, USA Images have historically been perceived as photographic proof of the depicted events. However, the growing ease with which digital images can be convincingly manipulated and then widely distributed on the Internet makes viewers increasingly susceptible to visual misinformation and deception.
In situations where ill-intentioned individuals seek to deliberately mislead and influence viewers through forged online images, the harmful consequences could be substantial on both personal and social levels. In this paper, we describe an exploratory study of how individuals react, respond to, and evaluate the authenticity of images that accompany online stories in Internet-enabled communications channels social networking site, blogs, email.
Our preliminary findings suggest that people perform poorly at detecting skillful image manipulation, and that they often fail to question the authenticity of images even when primed regarding image forgery through discussion. We thus far found that viewers make credibility evaluation based mainly on non-image cues rather that the content depicted.
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Moreover, our study have revealed that in cases where context leads to suspicion, viewers apply post hoc analysis to support their suspicions regarding the authenticity of the image. Ryan Payne 1Jeremy Shtern 2 1: The thing is, recently someone — something — did observe this.
Or parts of it, at least. Built and operated by the European Space agency, Herschel was at its launch in the largest infrared telescope ever to be hurled into the skies. It is this orbiting telescope — it circled as far as 1. Those instruments, mostly imaging cameras and spectrometers, read the light and energy signals jumping off HXMM01, emitted between the far infrared and submillimetre wavebands, or the 55— micrometre range of the electromagnetic spectrum, where conventional optical telescopes cannot see.
These signals told the scientists quite a lot about HXMM Such as that the new galaxy is about ten times the size of our Milky Way, and is located at a redshift of 2.
The redshift of an astronomical source measures the reddening of its light emission, due to the expansion of the universe, on its way to the observer. It can thus be used to determine how long it took for light observed today to travel to us, and a redshift of 2.
This data bonanza has provided scientists with a rare opportunity to compare their math notes with actual observations. HXMM01 is appealing for a number of reasons.
For one, very rarely do scientists get to witness the formation of a new galaxy out of two. As a result, it could upset the cart of mathematical models that scientists use to guesstimate the nuts and bolts of galaxy formation.
Understandably, HXMM01 is giving scientists some pause for thought. That temperature, combined with the vast gas stores mostly hydrogen and heliumhas meant that HXMM01 was extremely efficient at forming stars, most the size of our Sun.