Exp Clause Samples

Exp. Med. 203, 2817−2827.

Exp. Date / 3 Digit Security Code Billing Zip

Exp. Date: CVC:

Exp. Phys. 12 (2017) A101. [3] ▇. ▇▇▇▇▇▇▇▇▇ and ▇. ▇▇▇▇▇▇, Progress in high-energy cosmic ray physics, Prog. Part. Nucl. Phys. 98 (2018) 85 [arXiv:1710.11155] [INSPIRE]. [4] ▇▇▇▇▇▇ ▇▇▇▇▇ collaboration, Observation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above 8 1018 eV, Science 357 (2017) 1266 [arXiv:1709.07321] [INSPIRE]. [5] ▇▇▇▇▇▇ ▇▇▇▇▇ collaboration, Large-scale cosmic-ray anisotropies above 4 EeV measured by the ▇▇▇▇▇▇ ▇▇▇▇▇ Observatory, Astrophys. J. 868 (2018) 4 [arXiv:1808.03579] [INSPIRE]. [6] ▇▇▇▇▇▇ ▇▇▇▇▇ collaboration, An Indication of anisotropy in arrival directions of ultra-high-energy cosmic rays through comparison to the flux pattern of extragalactic gamma-ray sources, Astrophys. ▇. ▇▇▇▇. 853 (2018) L29 [arXiv:1801.06160] [INSPIRE]. [7] HiRes collaboration, First observation of the ▇▇▇▇▇▇▇-▇▇▇▇▇▇▇▇-▇▇▇▇▇▇ suppression, Phys. Rev. Lett. 100 (2008) 101101 [astro-ph/0703099] [INSPIRE]. [8] ▇▇▇▇▇▇ ▇▇▇▇▇ collaboration, Observation of the suppression of the flux of cosmic rays above 4 × 1019 eV, Phys. Rev. Lett. 101 (2008) 061101 [arXiv:0806.4302] [INSPIRE]. [9] ▇▇▇▇▇▇ ▇▇▇▇▇ collaboration, Measurement of the Energy Spectrum of Cosmic Rays above 1018 eV Using the ▇▇▇▇▇▇ ▇▇▇▇▇ Observatory, Phys. Lett. B 685 (2010) 239 [arXiv:1002.1975] [INSPIRE]. [10] ▇. ▇▇▇▇▇▇▇, End to the cosmic ray spectrum?, Phys. Rev. Lett. 16 (1966) 748 [INSPIRE]. [11] G.T. Zatsepin and V.A. ▇▇▇▇▇▇, Upper limit of the spectrum of cosmic rays, JETP Lett. 4 (1966) 78 [Pisma Zh. Eksp. Teor. Fiz 4 (1996) 114] [INSPIRE]. [12] ▇▇▇▇▇▇ ▇▇▇▇▇ collaboration, Measurement of the Depth of Maximum of Extensive Air Showers above 1018 eV, Phys. Rev. Lett. 104 (2010) 091101 [arXiv:1002.0699] [INSPIRE]. [13] ▇▇▇▇▇▇ ▇▇▇▇▇ collaboration, Depth of maximum of air-shower profiles at the ▇▇▇▇▇▇ ▇▇▇▇▇ Observatory. I. Measurements at energies above 1017.8 eV, Phys. Rev. D 90 (2014) 122005 [arXiv:1409.4809] [INSPIRE]. [14] ▇. ▇▇▇▇▇▇ and A.M. ▇▇▇▇▇▇, On The Heavy Chemical Composition of the Ultra-High Energy Cosmic Rays, Astropart. Phys. 33 (2010) 151 [arXiv:0910.1842] [INSPIRE]. [15] A.M. ▇▇▇▇▇▇, ▇. ▇▇▇▇▇▇ and ▇.▇. ▇▇▇▇▇▇▇▇▇, The need for a local source of ▇▇▇ ▇▇ nuclei, Phys. Rev. D 84 (2011) 105007 [arXiv:1107.2055] [INSPIRE]. [16] ▇. ▇▇▇▇▇▇, Propagation of extragalactic ultra-high energy cosmic-ray nuclei: implications for the observed spectrum and composition, Astropart. Phys. 33 (2012) 39. [17] ▇. ▇▇▇▇▇▇, N.G. ▇▇▇▇▇, ▇. ▇▇▇▇▇▇▇▇▇, ▇.▇. ▇▇▇▇▇▇ and ▇. ▇▇▇▇▇▇▇, Implications of ...

Exp. SEPT 2, ▇▇▇▇ ---------------------------------- ▇▇▇▇▇ ▇▇ ▇▇▇▇▇ (S) (S) COUNTY OF DALLAS (S) BEFORE ME, the undersigned, a Notary Public in and for said County and State on this 29TH day of MAY, 1996, personally appeared ▇▇▇▇▇▇ ▇. ▇▇▇▇▇, to me known to be the identical person who subscribed his name to the foregoing instrument as Trustee, and acknowledged to me that he executed the same as his free and voluntary act and deed for the uses and purposes therein set forth. GIVEN UNDER MY HAND AND SEAL OF OFFICE, the day and year last above written. /s/ ▇▇▇▇▇ ▇. ▇▇▇▇▇▇▇ ---------------------------- Notary public in and for the State of Texas My Commission Expires: Printed Name of Notary Public:

Exp. Date Home Phone Mobile Phone D.O.B. This agreement between (“Card” holder) and Purgatory Golf Club, (Club), as stated in the Terms and Conditions constitute the entire agreement between the parties. The “card” holder agrees that they have read the Terms and Conditions and agree to comply with them. A valid major Credit Card is required to be kept on file for the purpose of charging NO-SHOW tee times. No-show tee times are considered non-cancelled tee times (within 24 hours and having valid cancellation number) and card holder will be charged $25 per player that no-showed. The Golf Club will provide a $25 gift certificate per player in return for the no-showfee. Applicant’s Signature Date Assigned Card No. Print Name Staff Member Devotional Pass Senior Devotional Pass Return this application to the PRO SHOP or go on-line to ▇▇▇.▇▇▇▇▇▇▇▇▇▇▇▇▇.▇▇▇ and purchase yourcard. FOR Staff USE ONLY MemberNumber: Fee Received: Date received: Associate Name:

Exp. Exact types. Both dependent classes and prefix types of depen- dent classes are exact types [6]: all instances of these types must have the same run-time class. Simple types may be exact too. If A is a class, the exact type A! represents values of the run-time class A. Even if class B in- herits from A, neither B nor B! is a subtype of A!. Exactness ap- plies to the entire type preceding “!”, so supertypes of a sim- ple exact type can be obtained by shifting the exactness outward. For example, ASTDisplay.Exp! is not a subtype of AST.Exp!,

Exp. Exact types also restrict the subtyping relationships of nested types. For example, ASTDisplay!.▇▇▇▇▇▇ is not a subtype of AST!.Binary, even though ASTDisplay.Binary is a subtype of AST.Binary. Therefore exact types can mark the boundary of a family: classes nested in ASTDisplay! form one family and those nested in AST! form another. Non-dependent exact types provide a locally closed world: at compile time, one can enumerate all classes that are subtypes of A!.C, without inspecting subclasses of A. Exact types are important for the modularity of J&s (Section 2.5).

Exp. 1: Single view methods compared