scholarly journals 3D Mirrored Object Selection for Occluded Objects in Virtual Environments

IEEE Access ◽  
2020 ◽  
Vol 8 ◽  
pp. 200259-200274
Author(s):  
Joong-Jae Lee ◽  
Jung-Min Park
2021 ◽  
Vol 2 ◽  
Author(s):  
Rene Weller ◽  
Waldemar Wegele ◽  
Christoph Schröder ◽  
Gabriel Zachmann

AbstractWe present a novel selection technique for VR called LenSelect. The main idea is to decrease the Index of Difficulty (ID) according to Fitts’ Law by dynamically increasing the size of the potentially selectable objects. This facilitates the selection process especially in cases of small, distant or partly occluded objects, but also for moving targets. In order to evaluate our method, we have defined a set of test scenarios that covers a broad range of use cases, in contrast to often used simpler scenes. Our test scenarios include practically relevant scenarios with realistic objects but also synthetic scenes, all of which are available for download. We have evaluated our method in a user study and compared the results to two state-of-the-art selection techniques and the standard ray-based selection. Our results show that LenSelect performs similar to the fastest method, which is ray-based selection, while significantly reducing the error rate by 44%.


2012 ◽  
Vol 18 (4) ◽  
pp. 634-642 ◽  
Author(s):  
J. Cashion ◽  
C. Wingrave ◽  
J. J. LaViola

2013 ◽  
Vol 37 (3) ◽  
pp. 121-136 ◽  
Author(s):  
Ferran Argelaguet ◽  
Carlos Andujar

2012 ◽  
Vol 8 (S293) ◽  
pp. 165-167
Author(s):  
Emil Kundra ◽  
Theodor Pribulla ◽  
Martin Vaňko ◽  
Ľubomír Hambálek

AbstractProject Dwarf is a new observing campaign focused on the detection of substellar companions to low-mass (composed of late-type, subdwarf (sd) or/and white dwarf (WD) components) detached eclipsing binaries using minima timing. The crucial condition for the object selection for this campaign is possibility to determine times of the minima with high precision. This is naturally fullfilled for eclipsing binaries with deep and narrow minima or systems hosting a WD component showing fast ingress or egress.The observing project includes three groups of close eclipsing binaries indicating presence of substellar circum-binary components: (i)systems with K or/and M dwarf components(ii)systems with hot subdwarf (sd) and M dwarf components(iii)systems with white dwarf (WD) component(s). The sample of the eclipsing systems have orbital periods in range of 0.1 to almost 3 days and their brightness fits possibilities of small telescopes equipped with a low-end CCD camera and at least VRI filter set. Such kind of telescopes allow us to develop observing network including also amateur astronomers.


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