Are you a good employee or simply a good guy? influence costs and contract design

We develop a principal–agent model with a moral hazard problem in which the principal has access to a hard signal (the level of output) and a soft behavioral signal (the supervision signal) about the agent's level of effort. In our model, the agent can initiate influence activities and manipulate the behavioral signal. These activities are costly for the principal as they detract the agent from the productive task. We show that the agent's ability to manipulate the behavioral signal leads to low-powered incentives and increases the cost of implementing the efficient equilibrium as a result. Interestingly, the fact that manipulation activities entail productivity losses may lead to the design of influence-free contracts that deter manipulation and lead to high-powered incentives. This result implies that the optimal contract (and whether manipulation is tolerated in equilibrium or not) depends on the magnitude of the productivity-based influence costs. We show that it may be optimal for the principal not to supervise the agent, even if the cost of supervision is arbitrarily low

Hydrodynamic identification of NAUTILUS FOWT platform from small scale tests

A small-scale tank test campaign of the NAUTILUS offshore wind floating semisub-mersible platform was held at the Ifremer Deep Water Basin within the framework of the MaRINET 2 project. The support structure consists in four stabilized columns on a square pontoon supporting a generic 8-MW wind turbine. The tests were carried out at 1:36 Froude scale in parked conditions, and the mooring system was modelled as a set of aerial mooring springs providing a nonlinear stiffness. The hydrodynamic characterization of the floater from experimental data was tackled by using traditional techniques in naval architecture), as well as approaches derived from operational modal analysis in the frequency domain, such as the Sub Space Identification—Covariance (SSI-COV) method. The validity of this approach and its potential application to the identification of such kind of structures is discussed against the results of a more traditional technique based on the fitting of decay tests

Degradabilidade in situ da matéria seca e da proteína bruta das silagens de seis genótipos de sorgo (Sorghum bicolor (L.) Moench), com e sem tanino no grão, ensilados no estádio de grão farináceo.

Este experimento foi conduzido para avaliar o valor nutricional (materia seca e proteina bruta) de seis genotipos de sorgo para silagem, com e sem tanino no grao, colhidos no estadio de grao farinaceo, utilizando a tecnica da degradabilidade in situ. Seis genotipos de sorgo para ensilagens foram utilizadas: BR 303, BR 304, BR 601 e AG 2006 (sem tanino no grao) e BR 700 e BR 701 (com tanino no grao). quatro bovinos machos, canulados no rumen foram utilizados. os tempos de incubacao foram: 6, 12, 24, 48, 72 e 96 horas. Utilizou-se o tempo zero (t0) para calculo da solubilidade das silagens. A silagem do sorgo BR 304 apresentou os melhores resultados para a media de desaparecimento da MS e da PB as 96 horas de incubacao, seguida pela do AG 2006. O tanino presente nos graos dos genotipos BR 700 e BR 701 ensilados no estadio de grao farinaceo, nao respondeu por nenhum efeito sobre os parametros estudados de degradacao da materia seca e da proteina bruta

Degradabilidade in situ da matéria seca e da proteína bruta das silagens de seis genótipos de sorgo (Sorghum bicolor (L.) Moench), com e sem tanino no grão, ensilados no estádio de grão farináceo.

Este experimento foi conduzido para avaliar o valor nutricional (matéria seca e proteína bruta) de seis genótipos de sorgo para silagem, com e sem tanino no grão, colhidos no estádio de grão farináceo, utilizando a técnica da degradabilidade in situ. Seis silagens de genótipos de sorgo foram utilizadas: BR 303, BR 304, BR 601 e AG 2006 (sem tanino no grão) e BR 700 e BR 701 (com tanino no grão). Quatro bovinos machos, canulados no rúmen foram utilizados. Os tempos de incubação foram: 6, 12, 24, 48, 72 e 96 horas. Utilizou-se o tempo zero (t0) para cálculo da solubilidade das silagens. A silagem do sorgo BR 304 apresentou os melhores resultados para a média de desaparecimento da MS e da PB às 96 horas de incubação, seguida pela do AG 2006. O tanino presente nos grãos dos genótipos BR 700 e BR 701 ensilados no estádio de grão farináceo, não respondeu por nenhum efeito depressivo sobre os parâmetros estudados de degradação da matéria seca e da proteína bruta

Feasibility and anticipated acceptability of community health worker-facilitated HPV self-sampling for cervical cancer screening around Lake County, Indiana

Abstract Background/Objective: In light of calls to engage community health workers (CHWs) in the delivery of cervical cancer screening innovations, this study explores CHW perspectives on i) barriers to cervical cancer screening in a predominantly Hispanic community in Lake County, Indiana, the county with the highest cervical mortality in the state; and ii) the acceptability and feasibility of CHW-facilitated human papillomavirus (HPV) self-sampling as a means of reducing screening disparities. Methods: In 2021, in-depth interviews were conducted with 15 CHWs employed by Lake County community-based organizations including clinics, schools, and faith-based organizations. Results: Harnessing CHWs’ voices as insiders with knowledge of their communities’ health landscape, our analysis identified multilevel barriers to screening that spanned individual, interpersonal, and community levels of the socio-ecological model. CHW-facilitated HPV self-sampling shows promise of mitigating several barriers to cervical cancer screening. Privacy, time saved, and comfort were perceived to be facilitators for acceptability, with concerns about the novelty of this approach and trust in provider (as opposed to CHW) expertise emerging as key barriers. In terms of feasibility, synergies with existing CHW work, and some community members' prior experience with self-sampling were found to be facilitators, while CHW’s time limitations and self-efficacy in providing adequate medical support were areas of concern. Considerations for adoption included CHW training, gender concordance, safety, and respect, among others. Conclusion: This study provides critical insights from CHWs as key stakeholders on a screening model that directly engages them, which can inform implementation to increase screening in medically-underserved communities in the US

Wide field CO J = 3->2 mapping of the Serpens Cloud Core

Context. Outflows provide indirect means to get an insight on diverse star formation associated phenomena. On scales of individual protostellar cores, outflows combined with intrinsic core properties can be used to study the mass accretion/ejection process of heavily embedded protostellar sources. Methods. An area comprising 460"x230" of the Serpens cloud core has been mapped in 12 CO J = 3\to 2 with the HARP-B heterodyne array at the James Clerk Maxwell Telescope; J = 3\to 2 observations are more sensitive tracers of hot outflow gas than lower J CO transitions; combined with the high sensitivity of the HARP-B receptors outflows are sharply outlined, enabling their association with individual protostellar cores. Results. Most of ~20 observed outflows are found to be associated with known protostellar sources in bipolar or unipolar configurations. All but two outflow/core pairs in our sample tend to have a projected orientation spanning roughly NW-SE. The overall momentum driven by outflows in Serpens lies between 3.2 and 5.1 x 10^(-1) M\odot km s^(-1), the kinetic energy from 4.3 to 6.7 x 10^(43) erg and momentum flux is between 2.8 and 4.4 x 10^(-4) M\odot km s^(-1) yr^(-1). Bolometric luminosities of protostellar cores based on Spitzer photometry are found up to an order of magnitude lower than previous estimations derived with IRAS/ISO data. Conclusions. We confirm the validity of the existing correlations between the momentum flux and bolometric luminosity of Class I sources for the homogenous sample of Serpens, though we suggest that they should be revised by a shift to lower luminosities. All protostars classified as Class 0 sources stand well above the known Class I correlations, indicating a decline in momentum flux between the two classes.Comment: 15 pages, 10 figures, accepted for publication in A&