Way do I have to start here as Recrut. And how could I get in my first Swat Match silver5 Level even if i was last place in this 10 Matches. and why is the date Fall Winter 2017 even if I played first time in 2018. And why don’t I get my Weppon Card for Spartan Apereance even if I have it in Halo 5. And last question way is my Wepon power redcuced but all others can shoot with füll power on me?
You have to start here as recruit because everyone started as a recruit.
You got silver 5 because the ranking system is based upon how many matches you win and not how well you perform.
Its Fall 2017,because the new season hasnt started yet.
I dont know what you mean with that,but you cant use special stances for your waypoint picture.
And lastly,because of lag.
> 2535473431828738;1:
> Way do I have to start here as Recrut.
Because that is what everyone starts as; you can view more about the forum ranks here. And take a moment to read the rules linked in my signature please.
> And how could I get in my first Swat Match silver 5 Level even if i was last place in this 10 Matches.
Ranking depends on the level of your opposition and how well (or poorly) your team did against them. You can learn a bit more here. .
> why is the date Fall Winter 2017 even if I played first time in 2018.
That was the season you competed in. I don’t really concern myself with arena rank, so I don’t really keep track of when they start and stop.
> And why don’t I get my Weppon Card for Spartan Apereance even if I have it in Halo 5.
I don’t know what you mean.
> And last question way is my Wepon power redcuced but all others can shoot with füll power on me?
It isn’t. Everything is pretty much equal.
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Ok i will do the Beginner for the last Time but that is first kontackt
arXiv:astro-ph/9804232v1 22 Apr 1998
New Astronomy, in press
UMN-TH-1620/98
Massive Compact Halo Objects Viewed from a Cosmological Perspective:
Contribution to the Baryonic Mass Density of the Universe
Brian D. Fields
University of Minnesota, School of Physics and Astronomy
Minneapolis, Minnesota 55455, USA
fields@mnhepw.hep.umn.edu
Katherine Freese
University of Michigan, Department of Physics
Ann Arbor, Michigan 48109-1120, USA
freese@mich.physics.lsa.umich.edu
David S. Graff
DAPNIA/SPP, CEA Saclay
91191 Gif-sur-Yvette cedex, France
graff@hep.saclay.cea.fr
ABSTRACT
We estimate the contribution of Massive Compact Halo Objects (Machos) and their stellar
progenitors to the mass density of the Universe. If the Machos that have been detected reside
in the Halo of our Galaxy, then a simple extrapolation of the Galactic population (out to 50
kpc) of Machos to cosmic scales gives a cosmic density ρMacho = (1 − 5) × 109 hM⊙Mpc−3,
which in terms of the critical density corresponds to
Macho = (0.0036 − 0.017)h−1. Should the
Macho Halo extend out to much further than 50 kpc, then
…
… (Geschwärzt)
We thank Elisabeth Vangioni-Flam, Grant Mathews, Scott Burles, Joe Silk, Julien Devriendt, Michel
Cass´e, Jim Truran (who warned us from the beginning that carbon overproduction would be a serious
problem for white dwarfs), Sean Scully, and Dave Spergel for helpful discussions. We especially wish to
thank Dave Schramm, whom we already miss as a friend, colleague, and mentor, and without whom the
field of cosmology will not be the same. We are grateful for the hospitality of the Aspen Center for Physics,
where part of this work was done. DG acknowledges the financial support of the French Ministry of Foreign
Affairs’ Bourse Chateaubriand. KF acknowledges support from the DOE at the University of Michigan.
The work of BDF was supported in part by DoE grant DE-FG02-94ER-40823.
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This preprint was prepared with the AAS LATEX macros v4.0.
It is an Index
> 2535473431828738;4:
> Ok i will do the Beginner for the last Time but that is first kontackt
How does this relate at all to your own post?