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We note that we use the KR2 sample in this study both as the source of the properties of the void galaxies as well as for the higher-density comparison sample. While the minimum values shown in Table 2 reveal that there are a few void galaxies with extreme properties (lower luminosities, masses, abundances and SFRs), the overall distributions are indistinguishable. It is worth noting that our density analysis measures the local galaxy environment on scales of hundreds of kiloparsecs to a few megaparsecs. The mean and median values for each of the parameters considered in our analysis are essentially the same for the galaxies in the two density regimes. We conclude that the KR2 galaxies found in the Boötes Void have evolved in a manner that is quite similar to the star-forming galaxies located at much higher densities. All 1029 KR2 galaxies possess follow-up spectra. Our primary result is that there are no significant differences in the metallicities or the star-formation rates between the KR2 galaxies located in higher density regions and those found in voids. Of course, the KR2 sample should correctly reflect all star-formation activity, regardless of the nature of the triggering event. Hence, we stress that in our study the local "environment" is being measured on scales that may not capture the full picture of what is driving the star-formation activity

Once again, the people who don't like it should be able to turn it off. I, for example, would like the keyboard clicks to be much louder than they are but without it affecting the volume on the entire phone or the ring and notifications volume. 2. after Face-ID recognizes you, go directly into the phone home screen. Solar shingles on a home in San Diego, Calif. Note that some of the distortion is due to the night conditions here in foggy San Francisco. SplitView and SlideOver are here to stay… As long as you understand that the N4 is 1440p when using all three channels, it’s a good deal, though it would be a better one with GPS already on board The captures are hardly the best we’ve seen, but they’re colorful and present a serviceable amount of detail. On the always-on screen we should also be able to choose if we want to see if we have any notifications (the amount and the app) or if we to just want to see the clock. Allow us to change the colors of the LED light based on what the notification app is. 10. make it possible to customize the texting app in every conceivable way

Voids in the large-scale structure of the universe can yield information on cosmological parameters, be used to study dark energy, and test non-standard models of gravity (e.g., Liebscher et al., 1992; Moss et al., 2011; Li et al., 2012; Clampitt et al., 2013; Lam et al., 2015). Substantial numbers of voids are now found from redshift data (e.g., Patiri et al., 2006; Platen et al., 2007; Pustilnik & Tepliakova, 2011; Pan et al., 2012; Varela et al., 2012; Pustilnik et al., 2013; Mao et al., 2017; Libeskind et al., 2018) using a variety of void-finding algorithms. Several previous studies have considered the metallicities of void galaxies (e.g., Peimbert & Torres-Peimbert, 1992; Cruzen et al., 2002; Kreckel et al., 2015; Douglas et al., 2018), with the latter two studies focusing primarily on dwarf galaxies. Many studies of void galaxies’ properties, including optical spectra and photometry, have been published (e.g., Popescu et al., 1997, 1999; Grogin & Geller, 2000; Hogg et al., 2004; Rojas et al., 2005; Collobert et al., 2006; Patiri et al., 2006; Wegner & Grogin, 2008; Hoyle et al., 2012). Combined with H I surveys (Szomoru et al., 1996; Huchtmeier et al., 1997; Kreckel et al., 2011a, 2012, 2015; Ricciardelli et al., 2014; Moorman et al., 2014, 2015, 2016; Douglas et al., 2018), this has resulted in a general consensus that the lower density environments within which the void galaxies reside has only a small effect on their properties