Suchergebnisse

Stable revenue flows are paramount for policy makers at all levels of government in order to effectively and efficiently provide goods and services to constituents. This work examines the relationship between tax and expenditure limitations (TELs) and municipal revenue volatility. The current literature suggests that more stringently binding TELs at the state level are associated with greater levels of revenue volatility. This work tests whether this finding extends to the local level of government as well. Examining ninety-nine municipalities over eight years (2004–2011), this work provides evidence that the stringency level of TELs is associated with reduced fluctuations in municipal revenue streams.

Behavioral variance among telephone interviewers (interviewer effect) was investigated using data from 11 national polls conducted by CBS News & the New York Times in 1980. The polls involved a total of 300 interviewers, of whom 245 submitted completed questionnaires; selected effects examined were generally small & tended to be inconsistent between one poll & another. Explanations for the inconsistencies were found in the political context in which the polls were held & the variable associations with the nonrandom regional distribution of Rs. Demographic variables -- sex, region, size of place, & number of household adults -- were used to test for random distribution of Ss. Implications for further research on interaction between interviewer & S characteristics are discussed. 1 Table. Modified HA.

Current Population Survey (CPS) data from the U.S. Bureau of the Census quite clearly document continued population redistribution away from SMSAs to nonmetropolitan areas in the United States in the second half of the 1970s. Also, despite popular and some professional allegations of a return of population to cities from suburban rings-which would herald another dramatic migration turnaround during the 1970s CPS data reveal even heavier migration away from central cities to both suburbs and nonmetropolitan areas than in earlier years. Suburban rings are continuing to gain and central cities are continuing to lose population as a result of migration patterns. Decline in population growth rates in the suburban sector is clearly associated with lowered levels of natural increase not to a decline in net immigration. Overall, from a strictly demographic perspective, the data reveal no evidence of a "return-to-the-city" trend.

Five political generations in the US national electorate are identified, using data drawn from the 1980 New York Times/CBS News poll of 11,312 white registered voters. Each generation of voters is hypothesized to form its political identification based on experiences gained in early adulthood. The utility of the theory of operant conditioning in the analysis of political behavior is stressed. Future research should examine the issue positions of members in each generation & the changing behavior of generations during the campaign session. 4 Tables, 41 References. Modified HA

High-resolution mapping of the intracluster medium (ICM) up to high redshift and down to low masses is crucial to derive accurate mass estimates of the galaxy cluster and to understand the systematic eects aecting cosmological studies based on galaxy clusters. We present a spatially resolved Sunyaev-Zel'dovich (SZ)/X-ray analysis of ACT-CL J0215.4+0030, a high-redshift (z = 0:865) galaxy cluster of intermediate mass (M500 ' 3:5 1014 M) observed as part of the ongoing NIKA2 SZ large program, which is a follow-up of a representative sample of objects at 0:5 z 0:9. In addition to the faintness and small angular size induced by its mass and redshift, the cluster is contaminated by point sources that significantly aect the SZ signal. This is therefore an interesting case study for the most challenging sources of the NIKA2 cluster sample. We present the NIKA2 observations of this cluster and the resulting data.We identified the point sources that aect the NIKA2 maps of the cluster as submillimeter galaxies with counterparts in catalogs of sources constructed by the SPIRE instrument on board the Herschel observatory. We reconstructed the ICM pressure profile by performing a joint analysis of the SZ signal and of the point-source component in the NIKA2 150 GHz map. This cluster is a very weak source that lies below the selection limit of the Planck catalog. Nonetheless, we obtained high-quality estimates of the ICM thermodynamical properties with NIKA2. We compared the pressure profile extracted from the NIKA2 map to the pressure profile obtained from X-ray data alone by deprojecting the public XMM-Newton observations of the cluster.We combined the NIKA2 pressure profile with the X-ray deprojected density to extract detailed information on the ICM. The radial distribution of its thermodynamic properties (the pressure, temperature and entropy) indicate that the cluster has a highly disturbed core. We also computed the hydrostatic mass of the cluster, which is compatible with estimations from SZ and X-ray scaling relations. We conclude that the NIKA2 SZ large program can deliver quality information on the thermodynamics of the ICM even for one of its faintest clusters after a careful treatment of the contamination by point sources. ; With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737)

Context. NIKA2 is a dual-band millimetre continuum camera of 2 900 kinetic inductance detectors, operating at 150 and 260 GHz, installed at the IRAM 30-m telescope in Spain. Open to the scientific community since October 2017, NIKA2 will provide key observations for the next decade to address a wide range of open questions in astrophysics and cosmology. Aims. Our aim is to present the calibration method and the performance assessment of NIKA2 after one year of observation. Methods. We used a large data set acquired between January 2017 and February 2018 including observations of primary and secondary calibrators and faint sources that span the whole range of observing elevations and atmospheric conditions encountered by the IRAM 30-m telescope. This allowed us to test the stability of the performance parameters against time evolution and observing conditions. We describe a standard calibration method, referred to as the "Baseline"method, to translate raw data into flux density measurements. This includes the determination of the detector positions in the sky, the selection of the detectors, the measurement of the beam pattern, the estimation of the atmospheric opacity, the calibration of absolute flux density scale, the flat fielding, and the photometry. We assessed the robustness of the performance results using the Baseline method against systematic effects by comparing results using alternative methods. Results. We report an instantaneous field of view of 6.5′ in diameter, filled with an average fraction of 84%, and 90% of valid detectors at 150 and 260 GHz, respectively. The beam pattern is characterised by a FWHM of 17.6″ ± 0.1″ and 11.1″ ± 0.2″, and a main-beam efficiency of 47%±3%, and 64%±3% at 150 and 260 GHz, respectively. The point-source rms calibration uncertainties are about 3% at 150 GHz and 6% at 260 GHz. This demonstrates the accuracy of the methods that we deployed to correct for atmospheric attenuation. The absolute calibration uncertainties are of 5%, and the systematic calibration uncertainties evaluated at the IRAM 30-m reference Winter observing conditions are below 1% in both channels. The noise equivalent flux density at 150 and 260 GHz are of 9 ± 1 mJy s1/2 and 30 ± 3 mJy s1/2. This state-of-the-art performance confers NIKA2 with mapping speeds of 1388 ± 174 and 111 ± 11 arcmin2 mJy-2 h-1 at 150 and 260 GHz. Conclusions. With these unique capabilities of fast dual-band mapping at high (better that 18″) angular resolution, NIKA2 is providing an unprecedented view of the millimetre Universe. ; With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737)