Search

23 Jul 2014: With nightly data-rates of a few hundredGbytes (i.e. 10,000 individual 2k 2k images) automatedpipeline processing and data management requirements areparamount. ... which governs the requirement on the magnitude of the cross-talkterms. source of the cross

9 Nov 2018: The solution to remove this class of events is to empiri-cally look at the comet entry and exit parameters, θ and λ.If one was found to be more than ... MNRAS 000, 1–11 (2015). 10 GMK et al. requirement less stringent.

22 Nov 2018: Neutrinos 0.001. Photons (CMB) 5 105. Comparing the entries in the third and fourth row, we see that stars andtheir remnants (mostly white dwarfs) account for less than 10% of ... In any case, the search continues for a WIMP that may fit theastronomical

18 Apr 2022: Astronomy & Astrophysics manuscript no. LIFE_paper_1_FINAL_EDITED ESO 2022April 11, 2022. Large Interferometer For Exoplanets (LIFE):. I. Improved exoplanet detection yield estimates for a large mid-infraredspace-interferometer mission. S.P. Quanz1,

19 Feb 2018: The requirement for planetesimals,themselves a step in the planet formation process, makes debrisdiscs a fundamental component of planetary systems. ... 2013), who use a 3σ excess detection at any PACS wavelengthas their disc detection requirement.

11 Mar 2014: In mathematical termswe may write this requirement as. v. vk |v(t t) v(t)|. ... This arisesfrom the requirement that the new orbit of a particle must passthrough the point at which the kick is applied that is responsiblefor the apocentre and pericentre

29 Sep 2022: MNRAS 000, 1–21 (2022) Preprint 28September 2022 Compiled usingMNRASLATEXstyle file v3.0. High resolution ALMA and HST imaging of 𝜅 CrB: a broad debrisdisc around a post-main sequence star with low-mass companions. J. B. Lovell1,M.C.Wyatt1,

7 Jun 2007: DRS dictionaries Update vircam_standard_process, modify vircam_jitter_microstep_process, and modify entries in table 10-1. ... 0001, issue 3.2 2005-02-24. [RD 3] VISTA Science Requirements Document, VIS-SPE-VSC-00000-0001, issue.

10 Feb 2014: arX. iv:1. 402. 1184. v1 [. astr. o-ph. SR. ] 5. Feb. 201. 4. Spatially resolved imaging of the two-component η Crv debris disk with Herschel. G. Duchêne1, P. Arriaga. Astronomy Department, University of California, Berkeley, CA 94720, USA. and.