13,044 research outputs found
Die Landsgemeinde in Trogen Canton Appenzell V.R. am 24. Aprill 1814 ...
No full textgezeichnet von J. Jacob Mock von HerisauAus der Sammlung von Heinrich Appenzeller (1854-1921) Exemplar der Zentralbibliothek Zürich, Graphische Sammlung und Fotoarchi
Die Brandstätte im Flecken Herisau nach dem 1. Jenner 1812
No full textgezeichnet von J. Jacob Mock in HerisauAus der Sammlung von Heinrich Appenzeller (1854-1921) Exemplar der Zentralbibliothek Zürich, Graphische Sammlung und Fotoarchi
Mock, Col. Alfred J., July 20, 1993 [Interview]
No full textCol. Alfred J. Mock was interviewed on July 20, 1993, by Michael Birkner and David Hedrick about his relationship with Gettysburg graduate Stephen H. Warner, a Public Information Officer killed in the Vietnam War.Pyle, Ernie; Safer, Morley; Rather, Dan; Arnett, Peter; Warner, Stephen H.; Abrams, Gen. Creighton; Westmoreland, Gen. William C.; Goralski, Robert
Der Molken Cur-Ort Gais, Canton Appenzell V. R
No full textJ. J. Mock del. ; F. Hegi sculp.Aus der Sammlung von Heinrich Appenzeller (1854-1921) Exemplar der Zentralbibliothek Zürich, Graphische Sammlung und Fotoarchi
Mock-up example of Cliniface 3D facial ‘Hereditary Angioedema treatment and monitoring report’ Parental consent was obtained from the parent (Gareth Baynam) of the child whose image is appearing in Fig 3 who is also the corresponding author.
No full textMock-up example of Cliniface 3D facial ‘Hereditary Angioedema treatment and monitoring report’ Parental consent was obtained from the parent (Gareth Baynam) of the child whose image is appearing in Fig 3 who is also the corresponding author.</p
H. Byron Mock, Utah Uranium Oral History Project
No full textTranscript (47 pages) of an interview by Mitch Haddard with H. Byron Mock, on August 11, 1970. From tape number 91 in the Uranium History SeriesMitch Haddard interviewed this Salt Lake City attorney. Subjects: personal background, experience with uranium law, patenting uranium claims, Atomic Energy Commission, large uranium companies, preservation and ecology, marketability test, antiquated mining laws, property, mineral, leasing, and grazing rights (47 pages)
Perspectivische Vorstellung der Appenzeller Gebirgen, wie solche von Gais auser=Rodens anzusehen sind
No full textdurch J[ohann] J[akob] M[ock] gezeichnet Ao. 1794KupferstichErläuterungen siehe: Beschreibung der Appenzellischen Grenzgebirgen, gegen dem Rheinthal und Toggenburg, wie selbige von dem Flecken Gais aus anzusehen nach der Zeichnung No.
Constraining dark energy using real and mock galaxy surveys
No full textIn this thesis, we study how dark energy may be constrained by measurements of large-scale clustering in future galaxy surveys, and through the imprint of a time-varying large-scale potential on the CMB (the integrated Sachs-Wolfe effect).
We use semi-analytical galaxy formation models implemented in N-body simulations to build mock galaxy catalogues which are well suited for use in conjunction with large photometric surveys. Using mock catalogues, we predict that Pan-STARRS1 will be able to detect 10^8 galaxies in all its 5 photometric bands. We investigate the photo-z performance of the mock survey, which is a crucial factor when measuring large-scale structure statistics from a survey of this kind. We find using Pan-STARRS1 alone, photo-z accuracy of dz/(1+z) ~ 0.06 is achievable. The accuracy can be improved by combining near infrared photometry or by choosing a red galaxy sample. We implemented the photo-z errors to investigate their influence on the detectability of dark energy in the survey via the baryonic acoustic oscillations.
We explore the challenges of using the ISW effect as a constraint on dark energy. In particular, we investigate the effect of non-linear gravitational evolution, using N-body simulations. We have quantified the non-linear contribution to the ISW measurements in terms of both its power spectrum and its cross-correlation with large-scale structure. We have discovered that the non-linear ISW effect is more important relative to the linear ISW effect at larger scales at higher redshifts. This draws attention to the need to accurately model the non-linear effect when using galaxy samples to do ISW tomography at high redshifts. We have developed a ray-tracing method for constructing full sky maps of the ISW effect including its non-linear aspect. Using these maps, we have developed a complete picture of the non-linear ISW effect in void and cluster regions. We quantify the total contribution of the linear and non-linear ISW effects to reported abnormal CMB cold spots and discuss possible confusion with the Sunyaev-Zel'dovich effect
mock beggar - n.
No full textmock beggar nOED mock v 5... 1616, 1623 J,Taylor Devine picked these odd ...1825 etc items up somewhere EDD mock beggar ballWithd? [check]Not usedNot usedWithdraw
Financial analysts' evaluation of enhanced disclosure of non-financial performance indicators
No full textAbstract not availablePaul J. Coram, Theodore J. Mock, Gary S. Monro
- …
