Decline of the space density of quasars between z=2 and z=4

We define a new complete sample of 13 optically-luminous radio quasars M_AB(1450 Angstrom) 25.7 with redshift 3.8 < z < 4.5, obtained by cross-correlating the FIRST radio survey and the APM catalogue of POSS-I. We measure the space density to be 1.0 +/- 0.3 /Gpc^3, a factor 1.9 +/- 0.7 smaller than the space density of similar quasars at z=2. Using a new measurement of the radio-loud fraction of quasars we find that at z=4 the total space density of quasars with M_AB(1450 Angstrom) < -26.9 is 7.4 +/- 2.6/Gpc^3. This is a factor 1.8 +/- 0.8 less than the space density at z=2, found by the 2dF quasar survey. This (z=2)/(z=4) ratio, consistent with that of the radio-loud quasars, is significantly different from the ratio of about 10 found for samples including lower-luminosity quasars. This suggests that the decline of the space density beyond z=2 is slower for optically-luminous quasars than for less-luminous ones.Comment: 13 pages, 6 postscript figures, to be published in Astrophys. Journal, July 2003 issu

Effects of soil moisture and nitrogen fertilizer on pole beans

Published September 1966. Facts and recommendations in this publication may no longer be valid. Please look for up-to-date information in the OSU Extension Catalog: http://extension.oregonstate.edu/catalo

Ordinary-derivative formulation of conformal totally symmetric arbitrary spin bosonic fields

Conformal totally symmetric arbitrary spin bosonic fields in flat space-time of even dimension greater than or equal to four are studied. Second-derivative (ordinary-derivative) formulation for such fields is developed. We obtain gauge invariant Lagrangian and the corresponding gauge transformations. Gauge symmetries are realized by involving the Stueckelberg and auxiliary fields. Realization of global conformal boost symmetries on conformal gauge fields is obtained. Modified de Donder gauge condition and de Donder-Stueckelberg gauge condition are introduced. Using the de Donder-Stueckelberg gauge frame, equivalence of the ordinary-derivative and higher-derivative approaches is demonstrated. On-shell degrees of freedom of the arbitrary spin conformal field are analyzed. Ordinary-derivative light-cone gauge Lagrangian of conformal fields is also presented. Interrelations between the ordinary-derivative gauge invariant formulation of conformal fields and the gauge invariant formulation of massive fields are discussed.Comment: 51 pages, v2: Results and conclusions of v1 unchanged. In Sec.3, brief review of higher-derivative approaches added. In Sec.4, new representations for Lagrangian, modified de Donder gauge, and de Donder-Stueckelberg gauge added. In Sec.5, discussion of interrelations between the ordinary-derivative and higher-derivative approaches added. Appendices A,B,C,D and references adde

Bricoleurs Extraordinaire: Sports Coaches in Inter War Britain

In Inter War Britain, individuals exploited their athletic skills by pursuing professional careers, or adopting amateur roles, as instructors, trainers and coaches, invariably drawing from, and elaborating on, existing practices. The coach was the master of a body of specialist craft knowledge, the tacit nature of which was transmitted through ‘stealing with the eyes’ as the apprentice watched the master in action (Gamble, 2001). Professional coaches saw themselves as practical men whose experiential knowledge concerning diet, physiological and psychological preparation, stimulants, massaging, medical treatments, talent identification, and so on provided critical components in their coaching ‘toolbox’ (Nelson, 1924, 25-26). Craft knowledge was never static. Coaching expertise is a fluid, cyclical process with practitioners continuously redeveloping their competencies (Turner, Nelson and Potrac, 2012, 323), and part of traditional craft expertise was the ability to react positively to shifting circumstances. Coaches were constantly stimulated to experiment by competitors, commercialisation, and emerging technologies (Clegg, 1977, 244), and they exemplified the notion of the ‘Bricoleur’ in constantly trialling emerging knowledge, intuitively accepting or rejecting appropriate material. This paper explores the ways in which practitioners developed their coaching ‘toolbox’ in Inter War Britain by drawing on examples from newspaper reports, personal and public archives, and instructional texts (eg. Tilden, 1920; Gent, 1922; Nelson, 1924; Mussabini, 1926; Lowe and Porritt, 1929; Abrahams and Abrahams, 1936). The author highlights the range of knowledge that coaches had at their command, well before the emergence of sports science and coaching certification programmes, and questions assumptions that coaches can no longer rely solely on ‘learning the trade’ through experience (Evans and Light, 2007). As Winchester et al. (2013) have emphasised, knowledge, skills, attitudes, and insights are developed from daily experiences in sport, work and at home, as well as through exposure to the coaching environment, and contemporary coaches still employ a largely implicit form of knowledge, closely connected to past experiences, which shares similarities with Inter War craft knowledge (Smith and Cushion, 2006, 363; Jones, Armour and Potrac, 2003), while identifying experimentation and experience as key reference points (Irwin, Hanton and Kerwin, 2004, 436, 439; Potrac, Jones and Cushion, 2007)

Improved Gamma Bang Time Measurements on Omega and Implications for the National Ignition Facility

The time of peak fusion reactivity with respect to the impingement of laser light on an ICF capsule is known as Bang Time (BT). This is an essential parameter in the understanding of ICF implosions. Traditionally, BT has been determined through temporal measurements of 14 MeV fusion neutrons. Because the neutron energy spectrum is Doppler broadened, the detector must be positioned close to target-chamber center in order to minimize the neutron temporal spreading which can compromise such a measurement. Fusion gammas, on the other hand, are not subject to temporal spreading, making proximity of the detector to the source a lesser concern. However, the low branching ratio for DT fusion reactions producing gammas ({approx}1e-4) presents detector sensitivity challenges

The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey

The Sloan Digital Sky Survey III (SDSS-III) presents the first spectroscopic data from the Baryon Oscillation Spectroscopic Survey (BOSS). This ninth data release (DR9) of the SDSS project includes 535,995 new galaxy spectra (median z=0.52), 102,100 new quasar spectra (median z=2.32), and 90,897 new stellar spectra, along with the data presented in previous data releases. These spectra were obtained with the new BOSS spectrograph and were taken between 2009 December and 2011 July. In addition, the stellar parameters pipeline, which determines radial velocities, surface temperatures, surface gravities, and metallicities of stars, has been updated and refined with improvements in temperature estimates for stars with T_eff<5000 K and in metallicity estimates for stars with [Fe/H]>-0.5. DR9 includes new stellar parameters for all stars presented in DR8, including stars from SDSS-I and II, as well as those observed as part of the SDSS-III Sloan Extension for Galactic Understanding and Exploration-2 (SEGUE-2). The astrometry error introduced in the DR8 imaging catalogs has been corrected in the DR9 data products. The next data release for SDSS-III will be in Summer 2013, which will present the first data from the Apache Point Observatory Galactic Evolution Experiment (APOGEE) along with another year of data from BOSS, followed by the final SDSS-III data release in December 2014.Comment: 9 figures; 2 tables. Submitted to ApJS. DR9 is available at http://www.sdss3.org/dr

The state of the Martian climate

60°N was +2.0°C, relative to the 1981–2010 average value (Fig. 5.1). This marks a new high for the record. The average annual surface air temperature (SAT) anomaly for 2016 for land stations north of starting in 1900, and is a significant increase over the previous highest value of +1.2°C, which was observed in 2007, 2011, and 2015. Average global annual temperatures also showed record values in 2015 and 2016. Currently, the Arctic is warming at more than twice the rate of lower latitudes