Готові списки джерел за темами / PLANCK Data

Добірка наукової літератури з теми "PLANCK Data"

Автор: Grafiati
Опубліковано: 6 вересня 2023
Оновлено: 7 вересня 2023

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Статті в журналах з теми "PLANCK Data"

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Cai, Rong-Gen, Zong-Kuan Guo, and Bo Tang. "Updated reduced CMB data and constraints on cosmological parameters." International Journal of Modern Physics D 24, no. 10 (August 12, 2015): 1550071. http://dx.doi.org/10.1142/s0218271815500716.

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Анотація:
We obtain the reduced CMB data {lA, R, z∗} from WMAP9, WMAP9+BKP, Planck+WP and Planck+WP+BKP for the ΛCDM and wCDM models with or without spatial curvature. We then use these reduced CMB data in combination with low-redshift observations to put constraints on cosmological parameters. We find that including BKP results in a higher value of the Hubble constant especially when the equation of state (EOS) of dark energy and curvature are allowed to vary. For the ΛCDM model with curvature, the estimate of the Hubble constant with Planck+WP+Lensing is inconsistent with the one derived from Planck+WP+BKP at about 1.2σ confidence level (CL).
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2

Mangilli, Anna. "From data to science: Planck data and the CMB non-Gaussianity." Proceedings of the International Astronomical Union 10, S306 (May 2014): 131–34. http://dx.doi.org/10.1017/s1743921314013465.

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AbstractStudying the non-Gaussianity (NG) of the Cosmic Microwave Background (CMB) is an extremely powerful tool to investigate the properties of the very early Universe. The Planck nominal mission CMB maps yielded unprecedented constraints on primordial non-Gaussianity providing with the highest precision test of the standard model of inflation. Planck's high sensitivity also allowed to find evidence for the first time of the late-time non-Gaussianity arising from the Lensing-Integrated Sachs Wolfe (ISW) cross correlation. In this talk I will give details on the Planck data analysis and I will discuss the theoretical implications of the results.
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3

Partridge, Bruce. "Planck on Extragalactic Radio Sources: Data and Findings." Proceedings of the International Astronomical Union 11, A29B (August 2015): 51–53. http://dx.doi.org/10.1017/s174392131600449x.

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AbstractPlanck scanned the entire sky every six months at nine frequencies bands from 28 to 857 GHz with enough sensitivity to detect over a thousand radio sources. It thus provided measurements of the mm and sub-mm spectra of these sources in a regular cadence, even at wavelengths hard to observe from the ground. Polarization measurements (or upper limits) are provided for brighter sources at 28-353 GHz. Finally, Planck is calibrated to <1% accuracy in most of its frequency bands. I briefly introduce the valuable data set Planck provides on extragalactic sources, then describe some of the scientific conclusions drawn from the Planck measurements.
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4

Streblyanska, A., R. Barrena, J. A. Rubiño-Martín, R. F. J. van der Burg, N. Aghanim, A. Aguado-Barahona, A. Ferragamo, and H. Lietzen. "Characterization of a subsample of the Planck SZ source cluster catalogues using optical SDSS DR12 data." Astronomy & Astrophysics 617 (September 2018): A71. http://dx.doi.org/10.1051/0004-6361/201732306.

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Анотація:
Aims. The Planck catalogues of Sunyaev –Zeldovich (SZ) sources, PSZ1 and PSZ2, are the largest catalogues of galaxy clusters selected through their SZ signature in the full sky. In 2013, we started a long-term observational programme at Canary Island observatories with the aim of validating ∼500 unconfirmed SZ sources. In this work we present results of the initial pre-screening of possible cluster counterparts using photometric and spectroscopic data of the Sloan Digital Sky Survey DR12. Our main aim is to identify previously unconfirmed PSZ2 cluster candidates and to contribute in the determination of the actual purity and completeness of Planck SZ source sample. Methods. Using the latest version of the PSZ2 catalogue, we selected all sources overlapping with the SDSS DR12 footprint and without redshift information. We validated these cluster fields following optical criteria (mainly distance with respect to the Planck pointing, magnitude of the brightest cluster galaxy, and cluster richness), and combined these criteria with the profiles of the Planck Compton y-maps. This combined procedure allows for a more robust identification of optical counterparts compared to simply cross-matching with existing SDSS cluster catalogues that have been constructed from earlier SDSS data releases. Results. The sample contains new redshifts for 37 Planck galaxy clusters that were not included in the original release of PSZ2 Planck catalogue. We detect three cases as possible multiple counterparts. We show that a combination of all available information (optical images and profile of SZ signal) can provide correct associations between the observed Planck SZ source and the optically identified cluster. We also show that Planck SZ detection is very sensitive even to high-z (z > 0.5) clusters. In addition, we also present updated spectroscopic information for 34 Planck PSZ1 sources (33 previously photometrically confirmed and 1 new identification).
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5

Csáki, Csaba, Nemanja Kaloper, and John Terning. "Planck data and ultralight axions." Journal of Cosmology and Astroparticle Physics 2015, no. 06 (June 23, 2015): 041. http://dx.doi.org/10.1088/1475-7516/2015/06/041.

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6

Pagano, L., J. M. Delouis, S. Mottet, J. L. Puget, and L. Vibert. "Reionization optical depth determination from Planck HFI data with ten percent accuracy." Astronomy & Astrophysics 635 (March 2020): A99. http://dx.doi.org/10.1051/0004-6361/201936630.

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Анотація:
We present an estimation of the reionization optical depth τ from an improved analysis of data from the High Frequency Instrument (HFI) on board the Planck satellite. By using an improved version of the HFI map-making code, we greatly reduce the residual large-scale contamination affecting the data, characterised in, but not fully removed from, the Planck 2018 legacy release. This brings the dipole distortion systematic effect, contaminating the very low multipoles, below the noise level. On large-scale polarization-only data, we measure τ = 0.0566−0.0062+0.0053 at 68% C.L., reducing the Planck 2018 legacy release uncertainty by ∼40%. Within the ΛCDM model, in combination with the Planck large-scale temperature likelihood, and the high-ℓ temperature and polarization likelihood, we measure τ = 0.059 ± 0.006 at 68% C.L., which corresponds to a mid-point reionization redshift of zre = 8.14 ± 0.61 at 68% C.L. This estimation of the reionization optical depth with 10% accuracy is the strongest constraint to date.
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7

Ruiz-Granda, M., and P. Vielva. "Constraining CMB physical processes using Planck 2018 data." Journal of Cosmology and Astroparticle Physics 2022, no. 11 (November 1, 2022): 043. http://dx.doi.org/10.1088/1475-7516/2022/11/043.

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Abstract This paper aims to perform a phenomenological parametrisation of the standard cosmological model, ΛCDM, to weigh the different physical processes that define the pattern of the angular power spectra of the Cosmic Microwave Background (CMB) anisotropies. We use six phenomenological amplitudes to account for the Sachs-Wolfe, early and late Integrated Sachs-Wolfe, polarization contribution, Doppler and lensing effects. To do so, we have adapted the CLASS Boltzmann code and used the Markov Chain Monte Carlo (MCMC) sampler of Cobaya to explore the Planck 2018 likelihood to constrain different combinations of cosmological and phenomenological parameters. Observing deviations of the mean values of the phenomenological amplitudes from the predictions of the ΛCDM model could be useful to resolve existing cosmological tensions. For the first time, a comprehensive analysis of the physical processes of the CMB has been performed using the Planck 2018 temperature, polarization and lensing power spectra. In a previous work, the phenomenological amplitudes were constrained using only the TT data, however, by including the polarization and lensing data we find that the constraints on these physical contributions are tighter. In addition, some degeneracies that appear only when considering TT data are completely broken by taking into account all Planck 2018 data. Consequently, models with more than three phenomenological amplitudes can be studied, which is prohibitive when only the temperature power spectrum is used. The results presented in this paper show that the Planck experiment can constrain all phenomenological amplitudes except the late Integrated Sachs-Wolfe effect. No inconsistencies were found with the ΛCDM model, and the largest improvements were obtained for the models that include the lensing parameter, AL .
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8

Maris, Michele, Erik Romelli, Maurizio Tomasi, Anna Gregorio, Maura Sandri, Samuele Galeotta, Daniele Tavagnacco, Marco Frailis, Gianmarco Maggio, and Andrea Zacchei. "Revised planet brightness temperatures using the Planck/LFI 2018 data release." Astronomy & Astrophysics 647 (March 2021): A104. http://dx.doi.org/10.1051/0004-6361/202037788.

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Aims. We present new estimates of the brightness temperatures of Jupiter, Saturn, Uranus, and Neptune based on the measurements carried in 2009–2013 by Planck/LFI at 30, 44, and 70 GHz and released to the public in 2018. This work extends the results presented in the 2013 and 2015 Planck/LFI Calibration Papers, based on the data acquired in 2009–2011. Methods. Planck observed each planet up to eight times during the nominal mission. We processed time-ordered data from the 22 LFI radiometers to derive planet antenna temperatures for each planet and transit. We accounted for the beam shape, radiometer bandpasses, and several systematic effects. We compared our results with the results from the ninth year of WMAP, Planck/HFI observations, and existing data and models for planetary microwave emissivity. Results. For Jupiter, we obtain Tb = 144.9, 159.8, 170.5 K (± 0.2 K at 1σ, with temperatures expressed using the Rayleigh-Jeans scale) at 30, 44 and 70 GHz, respectively, or equivalently a band averaged Planck temperature Tb(ba) = 144.7, 160.3, 171.2 K in good agreement with WMAP and existing models. A slight excess at 30 GHz with respect to models is interpreted as an effect of synchrotron emission. Our measures for Saturn agree with the results from WMAP for rings Tb = 9.2 ± 1.4, 12.6 ± 2.3, 16.2 ± 0.8 K, while for the disc we obtain Tb = 140.0 ± 1.4, 147.2 ± 1.2, 150.2 ± 0.4 K, or equivalently a Tb(ba) = 139.7, 147.8, 151.0 K. Our measures for Uranus (Tb = 152 ± 6, 145 ± 3, 132.0 ± 2 K, or Tb(ba) = 152, 145, 133 K) and Neptune (Tb = 154 ± 11, 148 ± 9, 128 ± 3 K, or Tb(ba) = 154, 149, 128 K) agree closely with WMAP and previous data in literature.
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9

Nunes, Rafael C., Santosh K. Yadav, J. F. Jesus, and Armando Bernui. "Cosmological parameter analyses using transversal BAO data." Monthly Notices of the Royal Astronomical Society 497, no. 2 (July 11, 2020): 2133–41. http://dx.doi.org/10.1093/mnras/staa2036.

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ABSTRACT We investigate observational constraints on cosmological parameters combining 15 measurements of the transversal BAO scale (obtained free of any fiducial cosmology) with Planck–CMB data to explore the parametric space of some cosmological models. We investigate how much Planck + transversal BAO data can constraint the minimum Lambda cold dark matter (ΛCDM) model, and extensions, including neutrinos mass scale Mν, and the possibility for a dynamical dark energy (DE) scenario. Assuming the ΛCDM cosmology, we find H0 = 69.23 ± 0.50 km s−1 Mpc−1, Mν &lt; 0.11 eV, and rdrag = 147.59 ± 0.26 Mpc (the sound horizon at drag epoch) from Planck + transversal BAO data. When assuming a dynamical DE cosmology, we find that the inclusion of the BAO data can indeed break the degeneracy of the DE free parameters, improving the constraints on the full parameter space significantly. We note that the model is compatible with local measurements of H0 and there is no tension on H0 estimates in this dynamical DE context. Also, we discuss constraints and consequences from a joint analysis with the local H0 measurement from SH0ES. Finally, we perform a model-independent analysis for the deceleration parameter, q(z), using only information from transversal BAO data.
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10

Davidson, Aharon. "Holographic shell model: Stack data structure inside black holes?" International Journal of Modern Physics D 23, no. 05 (April 30, 2014): 1450041. http://dx.doi.org/10.1142/s0218271814500412.

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Анотація:
Rather than tiling the black hole horizon by Planck area patches, we suggest that bits of information inhabit, universally and holographically, the entire black core interior, a bit per a light sheet unit interval of order Planck area difference. The number of distinguishable (tagged by a binary code) configurations, counted within the context of a discrete holographic shell model, is given by the Catalan series. The area entropy formula is recovered, including Cardy's universal logarithmic correction, and the equipartition of mass per degree of freedom is proven. The black hole information storage resembles, in the count procedure, the so-called stack data structure.
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Більше джерел

Дисертації з теми "PLANCK Data"

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Zonca, Andrea. "Advanced modelling and combined data analysis of planck focal plane instruments." Paris 7, 2008. http://www.theses.fr/2008PA077169.

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Анотація:
Le sujet principal de mon travail de thèse est le logiciel de modélisation des radiomètres de l'instrument basse fréquence (LFI). LFI est l'un des deux instruments embarqués sur le satellite Planck de l'Agence spatiale européenne pour le mesurage de haute précision des anisotropies du rayonnement fossile. Le modèle logiciel s'appuie sur la réponse en fréquence mesurée des radiomètres éléments sur un simulateur de guide d'ondes analytique dans le but de simuler la réponse en fréquence du LFI canal par canal. Sa mise en œuvre est basée sur QUCS, un simulateur de circuit libre. La bande passante modélisée a montré la bonne cohérence avec les performances mesurées et moins a souffert des effets systématiques, ils sont donc les meilleures estimations disponibles pour la réponse en fréquence des radiomètres. Grâce à la collaboration avec Jean-Michel Lamarre, Instrument Scientist du HFI, l'instrument bolometrique de Planck, l'accent de mor activité a été élargie et a inclus l'étude de la corrélation croisée entre HFI et LFI données, sur deux aspects principaux: le calcul des fonctions de transfert thermique de l'étape à 4K au cours des tests et des simulations. Le 4K étape est un élément clé da la chaîne cryogénique de HFI, et c'est utilisée comme une charge de référence stable par LFI. Le projet des sessions de quick look analysis (QLA) que exploitent données scientifiques et housekeeping de ces deux instruments dans le but d'identifier les effets systématiques. Les sessions reposent sur le logiciel de visualisation de données KST et sont composées d'un ensemble de sessions de base déjà mis en œuvre et testées, permettant par exemple de produire spectra et corrélations croisée et une série de sessions avancées, dédiées à l'étude d'un aspect spécifique, par exemple la corrélation entre canaux de 70 GHz de Ll de 100 GHz de HFI
The main topic of my PhD work is the software modelling of the Low Frequency Instrument (LFI) radiometers. The LFI is one of the two instruments on-board the European Space Agency Planck Mission for high precision measurements of the anisotropies of the Cosmic Microwave Background (CMB). The software model relies on measured frequency response of the LFI radiometers components and on an analytical waveguide simu in order to simulate the LFI bandpasses channel by channel. Its implementation is based on QUCS, an open-source circuit Simulator. Modelled bandpasses showed good consistency with the measured performance and suffered less systematic effects, they are therefore the best estimate available for the radiometers frequency response. Thanks to the collaboration with Jean-Michel Lamarre, HFI Instrument Scientist, the bolometric instrument on-board Planck, the focus my activity was broadened and included the study of cross-correlation between HFI and LFI data, on two main aspects: The computation of the thermal transfer functions of the stage at 4K during tests and from simulations. The 4K stage is a key element the HFI cryogenic chain and it is used as a stable reference load by LFI. The design of quick look analysis sessions exploiting both instruments scientific and housekeeping data in order to identify systematic effects. Sessions relies on the data visualization software KST and consist of a set of already implemented and tested basic sessions allowing for example to produce spectra and cross-correlations, and a set of advanced sessions, dedicated on the study of a specific aspect, for example the correlation between LFI 70 GHz and HFI 100 GHz channels
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2

Zonca, A. "Advanced modelling and combined data analysis of Planck focal plane instruments." Doctoral thesis, Università degli Studi di Milano, 2009. http://hdl.handle.net/2434/64581.

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Анотація:
The main topic of my PhD work is the software modelling of the ESA Planck Low Frequency Instrument (LFI) radiometers. The software model, implemented in QUCS, relies on measured frequency response of the LFI radiometers components and on an analytical waveguide simulator in order to simulate the LFI bandpasses channel by channel. Modelled bandpasses showed good consistency with the measured performance and suffered less systematic effects, they are therefore the best estimate available for the radiometers frequency response. Thanks to the collaboration with Jean-Michel Lamarre, HFI Instrument Scientist, the bolometric instrument on-board Planck, the focus of my activity was broadened and included the study of cross-correlation between HFI and LFI data, on two main aspects: The computation of the thermal transfer functions of the stage at 4K during tests and from simulations. The 4K stage is a key element in the HFI cryogenic chain and it is used as a stable reference load by LFI. The design of quick look analysis sessions exploiting both instruments scientific and housekeeping data in order to identify systematic effects. Sessions relies on the data visualization software KST and consist of a set of already implemented and tested basic sessions, allowing for example to produce spectra and cross-correlations, and a set of advanced sessions, dedicated on the study of a specific aspect, for example the correlation between LFI 70 GHz and HFI 100 GHz channels.
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3

Crawford, T. M., R. Chown, G. P. Holder, K. A. Aird, B. A. Benson, L. E. Bleem, J. E. Carlstrom, et al. "MAPS OF THE MAGELLANIC CLOUDS FROM COMBINED SOUTH POLE TELESCOPE AND PLANCK DATA." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/622699.

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Анотація:
We present maps of the Large and Small Magellanic Clouds from combined South Pole Telescope (SPT) and Planck data. The Planck satellite observes in nine bands, while the SPT data used in this work were taken with the three-band SPT-SZ camera, The SPT-SZ bands correspond closely to three of the nine Planck bands, namely those centered at 1.4, 2.1, and 3.0 mm. The angular resolution of the Planck data ranges from 5 to 10 arcmin, while the SPT resolution ranges from 1.0 to 1.7 arcmin. The combined maps take advantage of the high resolution of the SPT data and the long-timescale stability of the space-based Planck observations to deliver robust brightness measurements on scales from the size of the maps down to similar to 1 arcmin. In each band, we first calibrate and color-correct the SPT data to match the Planck data, then we use noise estimates from each instrument and knowledge of each instrument's beam to make the inverse-variance-weighted combination of the two instruments' data as a function of angular scale. We create maps assuming a range of underlying emission spectra and at a range of final resolutions. We perform several consistency tests on the combined maps and estimate the expected noise in measurements of features in them. We compare maps from this work to those from the Herschel HERITAGE survey, finding general consistency between the data sets. All data products described in this paper are available for download from the NASA Legacy Archive for Microwave Background Data Analysis server.
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4

Alina, Dana. "Analysis of the interstellar dust polarized emission with the Planck Satellite Survey data." Thesis, Toulouse 3, 2015. http://www.theses.fr/2015TOU30032.

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Cette thèse est dédiée à l'étude de la polarisation de la poussière interstellaire et est principalement basée sur l'analyse des données du satellite Planck. Tout d'abord, nous caractérisons le biais sur les paramètres de polarisation déduits des données. Nous avons mis en évidence que ce biais dépend non seulement du niveau de bruit, mais également de la corrélation entre les bruits sur les paramètres de Stokes. Nous avons développé des méthodes optimisées d'estimation de la fraction de polarisation, de l'angle de polarisation et de la fonction de dispersion de l'angle de polarisation, qui tiennent compte de la forme des matrices de covariance du bruit. Nous avons montré pour la première fois que le comportement du biais sur la fonction de dispersion d'angle est non trivial, et nous avons proposé une méthode pour évaluer la limite supérieure du biais que nous avons appliqué aux données Planck de la bande à 353 GHz. Nous avons étudié la corrélation entre la fraction de polarisation et la fonction de dispersion d'angle, ainsi que la corrélation entre la fraction de polarisation et la densité de colonne de gaz, sur de grandes fractions du ciel. Ceci nous a permis de mettre en évidence que la structure à 3 dimensions du champ magnétique affecte fortement la fraction de polarisation observée. Lorsque la direction du champ magnétique change le long de la ligne de visée ou dans le faisceau du télescope, on observe que la fraction de polarisation diminue. Nous avons comparé ce résultat à des simulations numériques basées sur la MHD magnétohydrodynamique). Une dépendance similaire de la fraction de polarisation avec la géométrie du champ magnétique y est observée. La diminution de la fraction de polarisation avec la densité de colonne était observée dans les nuages moléculaires dans des études précédentes. Nous avons généralisé ce résultat comme étant également caractéristique du milieu diffus à grande échelle. En combinaison avec les résultats des simulations MHD où un comportement similaire est observé, ceci indique que la diminution de la fraction de polarisation est principalement due aux changements de direction du champ magnétique le long de la ligne de visée. Nous avons pour la première fois déterminé la limite inférieure de la fraction de polarisation maximale réelle bservée avec Planck. Cette limite pourrait correspondre au niveau de polarisation intrinsèque de la poussière interstellaire dans les conditions les plus favorables de la géométrie du champ magnétique. De plus, la comparaison entre la polarisation en émission et en extinction nous a permis d'établir le rapport entre la fraction de polarisation dans les domaines sub-millimétrique et visible. Ce résultat apporte une contrainte forte pour de futurs modèles de la poussière interstellaire. Enfin, nous avons effectué une étude préliminaire sur les propriétés en polarisation des associations de coeurs froid détectés avec Planck. Cette analyse statistique nous permet de confirmer la diminution de la fraction de polarisation dans ces milieux, par rapport à l'environnement local à grande échelle. Nous discutons son origine en termes de perte d'efficacité de l'alignement des grains dans ces associations de coeurs denses
This thesis is dedicated to the study of Galactic dust polarization and is mostly based on the analysis of the Planck satellite data. First, we characterize the bias on polarization parameters which are derived from the measurements. We have evidenced that it depends not only on the noise level but also on the noise correlation between the Stokes parameters. We have developed optimized methods to estimate the polarization fraction, angle and angle dispersion function, that take into account the shape of the noise covariance matrices. The peculiarity of the bias on the polarization angle dispersion function is shown for the first time, and a method for the evaluation of the upper limit on the bias is proposed and applied to the Planck 353 GHz data. We study the correlation between the polarization fraction and the polarization angle dispersion function, and also the correlation between the polarization fraction and the gas column density, over large fractions of the sky. As a result, we show that the three-dimensional structure of the magnetic field highly affects the observed polarization fraction. When the magnetic field direction changes along the line of sight or within the telescope beam, the observed polarization decreases. We observe a similar dependance of the polarization fraction with the magnetic field geometry in MHD (magnetohydrodynamics) simulations. We have evidenced the systematic decrease of the polarization fraction with column density, previously observed only in dense molecular clouds, to be general also at large scales and in the diffuse ISM. In combination with the results from MHD simulations, where a similar behavior is observed, this observational fact indicates that the decrease in the polarization fraction is mostly due to the magnetic field tangling along the line of sight. We derive for the first time the lower limit of the maximum polarization fraction observed with Planck, which could correspond to the dust intrinsic polarization fraction when the field geometry is most favorable. In addition, comparing polarization in emission with Planck and in extinction from stars observations, we find a high sub-millimeter to visible polarization fraction ratio, which will be a strong constraint for future dust models. Finally, we have performed a preliminary study on the polarization properties of Galactic cold clumps detected with Planck. This statistical analysis allows us to confirm the existence of a significant drop of the polarization fraction in the clumps, relatively to the local large scale environment. We discuss its origin in terms of efficiency loss of grain alignment in these dense clumps
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5

Paci, Francesco <1980&gt. "Gravitational waves and cosmic microwave anisotropies: from theory to data analysis for Planck." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2009. http://amsdottorato.unibo.it/1859/1/paci_francesco_tesi.pdf.

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6

Paci, Francesco <1980&gt. "Gravitational waves and cosmic microwave anisotropies: from theory to data analysis for Planck." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2009. http://amsdottorato.unibo.it/1859/.

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7

Omori, Y., R. Chown, G. Simard, K. T. Story, K. Aylor, E. J. Baxter, B. A. Benson, et al. "A 2500 deg2 CMB Lensing Map from Combined South Pole Telescope and Planck Data." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/626179.

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Анотація:
We present a cosmic microwave background (CMB) lensing map produced from a linear combination of South Pole Telescope (SPT) and Planck temperature data. The 150 GHz temperature data from the 2500 deg(2) SPT-SZ survey is combined with the Planck 143 GHz data in harmonic space to obtain a temperature map that has a broader l coverage and less noise than either individual map. Using a quadratic estimator technique on this combined temperature map, we produce a map of the gravitational lensing potential projected along the line of sight. We measure the auto-spectrum of the lensing potential C-L(phi phi), and compare it to the theoretical prediction for a.CDM cosmology consistent with the Planck 2015 data set, finding a best-fit amplitude of 0.95(-0.06)(+0.06) (stat.)(-0.01)(+0.01)+ (sys.). The null hypothesis of no lensing is rejected at a significance of 24 sigma. One important use of such a lensing potential map is in cross-correlations with other dark matter tracers. We demonstrate this cross-correlation in practice by calculating the cross-spectrum, C-L(phi) G, between the SPT+ Planck lensing map and Wide-field Infrared Survey Explorer (WISE) galaxies. We fit C-L(phi G) to a power law of the form p(L) = a(L/L-0)(-b) with a, L-0, and b fixed, and find eta(phi G) = C-L(phi G)/p(L) = 0.94(-0.04)(+0.04), which is marginally lower, but in good agreement with eta(phi G) = 1.00-(+0.02)(0.01), the best-fit amplitude for the cross-correlation of Planck-2015 CMB lensing and WISE galaxies over similar to 67% of the sky. The lensing potential map presented here will be used for cross-correlation studies with the Dark Energy Survey, whose footprint nearly completely covers the SPT 2500 deg(2) field.
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Hou, Z., K. Aylor, B. A. Benson, L. E. Bleem, J. E. Carlstrom, C. L. Chang, H.-M. Cho, et al. "A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data." IOP PUBLISHING LTD, 2018. http://hdl.handle.net/10150/626533.

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We study the consistency of 150 GHz data from the South Pole Telescope (SPT) and 143 GHz data from the Planck satellite over the patch of sky covered by the SPT-SZ survey. We first visually compare the maps and find that the residuals appear consistent with noise after accounting for differences in angular resolution and filtering. We then calculate (1) the cross-spectrum between two independent halves of SPT data, (2) the cross-spectrum between two independent halves of Planck data, and (3) the cross-spectrum between SPT and Planck data. We find that the three cross-spectra are well fit (PTE = 0.30) by the null hypothesis in which both experiments have measured the same sky map up to a single free calibration parameter-i.e., we find no evidence for systematic errors in either data set. As a by-product, we improve the precision of the SPT calibration by nearly an order of magnitude, from 2.6% to 0.3% in power. Finally, we compare all three cross-spectra to the full-sky Planck power spectrum and find marginal evidence for differences between the power spectra from the SPT-SZ footprint and the full sky. We model these differences as a power law in spherical harmonic multipole number. The best-fit value of this tilt is consistent among the three cross-spectra in the SPT-SZ footprint, implying that the source of this tilt is a sample variance fluctuation in the SPT-SZ region relative to the full sky. The consistency of cosmological parameters derived from these data sets is discussed in a companion paper.
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9

Kirk, D., Y. Omori, A. Benoit-Lévy, R. Cawthon, C. Chang, P. Larsen, A. Amara, et al. "Cross-correlation of gravitational lensing from DES Science Verification data with SPT and Planck lensing." OXFORD UNIV PRESS, 2016. http://hdl.handle.net/10150/614994.

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We measure the cross-correlation between weak lensing of galaxy images and of the cosmic microwave background (CMB). The effects of gravitational lensing on different sources will be correlated if the lensing is caused by the same mass fluctuations. We use galaxy shape measurements from 139 deg(2) of the Dark Energy Survey (DES) Science Verification data and overlapping CMB lensing from the South Pole Telescope (SPT) and Planck. The DES source galaxies have a median redshift of z(med) similar to 0.7, while the CMB lensing kernel is broad and peaks at z similar to 2. The resulting cross-correlation is maximally sensitive to mass fluctuations at z similar to 0.44. Assuming the Planck 2015 best-fitting cosmology, the amplitude of the DESxSPT cross-power is found to be A(SPT) = 0.88 +/- 0.30 and that from DESxPlanck to be A(Planck) = 0.86 +/- 0.39, where A = 1 corresponds to the theoretical prediction. These are consistent with the expected signal and correspond to significances of 2.9 sigma and 2.2 sigma, respectively. We demonstrate that our results are robust to a number of important systematic effects including the shear measurement method, estimator choice, photo-z uncertainty and CMB lensing systematics. We calculate a value of A = 1.08 +/- 0.36 for DESxSPT when we correct the observations with a simple intrinsic alignment model. With three measurements of this cross-correlation now existing in the literature, there is not yet reliable evidence for any deviation from the expected LCDM level of cross-correlation. We provide forecasts for the expected signal-to-noise ratio of the combination of the five-year DES survey and SPT-3G.
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Hankeln, Wolfgang Matthias [Verfasser]. "Data integration in microbial genomics Contextualizing sequence data in aid of biological knowledge / Wolfgang Matthias Hankeln. Max Planck Institute for Marine Microbiology." Bremen : IRC-Library, Information Resource Center der Jacobs University Bremen, 2012. http://d-nb.info/1035209020/34.

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Книги з теми "PLANCK Data"

1

EDV-Benutzertreffen, Max-Planck-Gesellschaft zur Förderung der Wissenschaften. Forschung und wissenschaftliches Rechnen: Beiträge anässlich des 10. EDV-Benutzertreffens der Max-Planck-Gesellschaft in Göttingen, November 1993. München: Die Gesellschaft, 1993.

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International Summer School on Crystallographic Computing (1984 Mülheim an der Ruhr). Crystallographic computing 3: Data collection, structure determination, proteins and databases : papers presented at the International Summer School on Crystallographic Computing held at the Max-Planck-Institut für Kohlenforschung, Mülheim an der Ruhr FRG, 30 July-8 August 1984. Oxford: Clarendon, 1985.

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J, Maarse F., Kontaktgroep voor Instrumentatie in de Psychologie (Netherlands), and Max Planck Institut für Psycholinguistik (Nijmegen, Netherlands), eds. Computers in de psychologie: Verslag van een workshop van de Kontaktgroep voor Instrumentatie in de Psychologie (KIP) op 17 en 18 mei 1984 in het Max Planck Institut für Psychologie te Nijmegen. Lisse: Swets & Zeitlinger, 1985.

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4

P, Nayar M., Sastry, A. R. K. 1938-, and Botanical Survey of India, eds. Red data book of Indian plants. Calcutta: Botanical Survey of India, 1987.

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Hilton-Taylor, Craig. Red data list of southern African plants. Edited by Leistner O. A. Pretoria: National Botanical Institute, 1996.

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6

Salar, Khan M., Rahman M. Matiur, Ali M. Arshad, Bangladesh National Herbarium, and Bāṃlādeśa Kr̥shi Gabeshaṇā Kāunsila, eds. Red data book of vascular plants of Bangladesh. Dhaka: Bangladesh National Herbarium, 2001.

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7

Planar graph drawing. Singapore: World Scientific, 2005.

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8

Nature Protection Trust of Seychelles. Scientific Committee. Seychelles red data book, 1997. Edited by Gerlach Justin. Victoria, Mahe, Seychelles: Nature Protection Trust of Seychelles, 1997.

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9

Abd El Ghani, Monier M. and Fahmy Ahmed G, eds. The plant red data book of Egypt. Cairo: Palm Press, 1992.

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10

Intersection and decomposition algorithms for planar arrangements. Cambridge: Cambridge University Press, 1991.

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Частини книг з теми "PLANCK Data"

1

Lang, Kenneth R. "Planet Earth." In Astrophysical Data, 29–40. New York, NY: Springer US, 1992. http://dx.doi.org/10.1007/978-1-4684-0640-5_2.

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Max, Nelson, Peter Williams, and Claudio Silva. "Cell Projection of Meshes with Non-Planar Faces." In Data Visualization, 157–68. Boston, MA: Springer US, 2003. http://dx.doi.org/10.1007/978-1-4615-1177-9_11.

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Srivastava, Anuj, and Eric P. Klassen. "Shapes of Planar Curves." In Functional and Shape Data Analysis, 125–65. New York, NY: Springer New York, 2016. http://dx.doi.org/10.1007/978-1-4939-4020-2_5.

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Akhtar, Mohd Sayeed, Mallappa Kumara Swamy, Ibrahim A. Alaraidh, and Jitendra Panwar. "Genomic Data Resources and Data Mining." In Plant Bioinformatics, 267–78. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-67156-7_10.

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Srivastava, Anuj, and Eric P. Klassen. "Shapes of Planar Closed Curves." In Functional and Shape Data Analysis, 167–231. New York, NY: Springer New York, 2016. http://dx.doi.org/10.1007/978-1-4939-4020-2_6.

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Srivastava, Anuj, and Eric P. Klassen. "Statistical Modeling of Planar Shapes." In Functional and Shape Data Analysis, 305–47. New York, NY: Springer New York, 2016. http://dx.doi.org/10.1007/978-1-4939-4020-2_9.

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Fait, Aaron, and Alisdair R. Fernie. "Data Integration." In Plant Metabolic Networks, 151–71. New York, NY: Springer New York, 2008. http://dx.doi.org/10.1007/978-0-387-78745-9_6.

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Pearcy, Robert W. "Field data acquisition." In Plant Physiological Ecology, 15–27. Dordrecht: Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-010-9013-1_2.

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Pearcy, Robert W. "Field data acquisition." In Plant Physiological Ecology, 15–27. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2221-1_2.

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Mu, Xuelan, Zhixin Hou, and Yigong Zhang. "Egomotion Estimation Under Planar Motion with an RGB-D Camera." In Intelligence Science and Big Data Engineering. Visual Data Engineering, 68–79. Cham: Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-36189-1_6.

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Тези доповідей конференцій з теми "PLANCK Data"

1

Pasian, Fabio, and Jean-Fran‡ois Sygnet. "Planck data processing centers." In Astronomical Telescopes and Instrumentation. SPIE, 2002. http://dx.doi.org/10.1117/12.461140.

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Sébastien, Clesse. "Analysis of the Planck data." In 10th Modave Summer School in Mathematical Physics. Trieste, Italy: Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.232.0003.

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"Cosmological constraints on neutrinos with Planck data." In XXVI INTERNATIONAL CONFERENCE ON NEUTRINO PHYSICS AND ASTROPHYSICS: Neutrino 2014. AIP Publishing LLC, 2015. http://dx.doi.org/10.1063/1.4915585.

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GUBITOSI, GIULIA. "PLANCK-SCALE INDUCED BIREFRINGENCE AND CMB POLARIZATION DATA." In Proceedings of the MG12 Meeting on General Relativity. WORLD SCIENTIFIC, 2012. http://dx.doi.org/10.1142/9789814374552_0497.

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Zhou, Yixue. "Photoelectric effect, Planck constant, and MATLAB data processing." In Third International Conference on Optics and Image Processing (ICOIP 2023), edited by Bingxiang Li and Chao Ren. SPIE, 2023. http://dx.doi.org/10.1117/12.2689113.

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Schmidt, Micha, and Ed Chester. "Herschel/Planck Data Flow - Design Challenges and Operational Solutions." In SpaceOps 2006 Conference. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2006. http://dx.doi.org/10.2514/6.2006-5749.

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Tomasi, Maurizio, Paola Battaglia, Marco Bersanelli, Francesco Cuttaia, Cristian Franceschet, Marco Lapolla, Rodrigo Leonardi, et al. "Data analysis of the Planck/LFI ground-test campaign." In SPIE Astronomical Telescopes + Instrumentation, edited by Jonas Zmuidzinas, Wayne S. Holland, Stafford Withington, and William D. Duncan. SPIE, 2006. http://dx.doi.org/10.1117/12.671522.

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Ramazanov, Sabir. "Probing primordial statistical anisotropy with WMAP and Planck data." In Frontiers of Fundamental Physics 14. Trieste, Italy: Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.224.0093.

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Frailis, M., A. Zacchei, M. Maris, N. Morisset, R. Rohlfs, M. Meharga, P. Binko, et al. "The Planck/LFI data processing: real-time analysis, data management and scientific workflows." In Proceedings of the 11th Conference. WORLD SCIENTIFIC, 2010. http://dx.doi.org/10.1142/9789814307529_0114.

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Di Girolamo, Gianpiero, Daniel Werner, Eduardo Valido Cabrera, Mariella Spada, and John Dodsworth. "Herschel-Planck Mission Data System: A Remarkable Collection of Challenges." In SpaceOps 2010 Conference: Delivering on the Dream (Hosted by NASA Marshall Space Flight Center and Organized by AIAA). Reston, Virigina: American Institute of Aeronautics and Astronautics, 2010. http://dx.doi.org/10.2514/6.2010-2087.

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Звіти організацій з теми "PLANCK Data"

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Fluhr, Robert, and Volker Brendel. Harnessing the genetic diversity engendered by alternative gene splicing. United States Department of Agriculture, December 2005. http://dx.doi.org/10.32747/2005.7696517.bard.

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Our original objectives were to assess the unexplored dimension of alternative splicing as a source of genetic variation. In particular, we sought to initially establish an alternative splicing database for Arabidopsis, the only plant for which a near-complete genome has been assembled. Our goal was to then use the database, in part, to advance plant gene prediction programs that are currently a limiting factor in annotating genomic sequence data and thus will facilitate the exploitation of the ever increasing quantity of raw genomic data accumulating for plants. Additionally, the database was to be used to generate probes for establishing high-throughput alternative transcriptome analysis in the form of a splicing-specific oligonucleotide microarray. We achieved the first goal and established a database and web site termed Alternative Splicing In Plants (ASIP, http://www.plantgdb.org/ASIP/). We also thoroughly reviewed the extent of alternative splicing in plants (Arabidopsis and rice) and proposed mechanisms for transcript processing. We noted that the repertoire of plant alternative splicing differs from that encountered in animals. For example, intron retention turned out to be the major type. This surprising development was proven by direct RNA isolation techniques. We further analyzed EST databases available from many plants and developed a process to assess their alternative splicing rate. Our results show that the lager genome-sized plant species have enhanced rates of alternative splicing. We did advance gene prediction accuracy in plants by incorporating scoring for non-canonical introns. Our data and programs are now being used in the continuing annotation of plant genomes of agronomic importance, including corn, soybean, and tomato. Based on the gene annotation data developed in the early part of the project, it turned out that specific probes for different exons could not be scaled up to a large array because no uniform hybridization conditions could be found. Therefore, we modified our original objective to design and produce an oligonucleotide microarray for probing alternative splicing and realized that it may be reasonable to investigate the extent of alternative splicing using novel commercial whole genome arrays. This possibility was directly examined by establishing algorithms for the analysis of such arrays. The predictive value of the algorithms was then shown by isolation and verification of alternative splicing predictions from the published whole genome array databases. The BARD-funded work provides a significant advance in understanding the extent and possible roles of alternative splicing in plants as well as a foundation for advances in computational gene prediction.
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Wright, Kirsten. Collecting Plant Phenology Data In Imperiled Oregon White Oak Ecosystems: Analysis and Recommendations for Metro. Portland State University, March 2020. http://dx.doi.org/10.15760/mem.64.

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Highly imperiled Oregon white oak ecosystems are a regional conservation priority of numerous organizations, including Oregon Metro, a regional government serving over one million people in the Portland area. Previously dominant systems in the Pacific Northwest, upland prairie and oak woodlands are now experiencing significant threat, with only 2% remaining in the Willamette Valley in small fragments (Hulse et al. 2002). These fragments are of high conservation value because of the rich biodiversity they support, including rare and endemic species, such as Delphinium leucophaeum (Oregon Department of Agriculture, 2020). Since 2010, Metro scientists and volunteers have collected phenology data on approximately 140 species of forbs and graminoids in regional oak prairie and woodlands. Phenology is the study of life-stage events in plants and animals, such as budbreak and senescence in flowering plants, and widely acknowledged as a sensitive indicator of environmental change (Parmesan 2007). Indeed, shifts in plant phenology have been observed over the last few decades as a result of climate change (Parmesan 2006). In oak systems, these changes have profound implications for plant community composition and diversity, as well as trophic interactions and general ecosystem function (Willis 2008). While the original intent of Metro’s phenology data-collection was to track long-term phenology trends, limitations in data collection methods have made such analysis difficult. Rather, these data are currently used to inform seasonal management decisions on Metro properties, such as when to collect seed for propagation and when to spray herbicide to control invasive species. Metro is now interested in fine-tuning their data-collection methods to better capture long-term phenology trends to guide future conservation strategies. Addressing the regional and global conservation issues of our time will require unprecedented collaboration. Phenology data collected on Metro properties is not only an important asset for Metro’s conservation plan, but holds potential to support broader research on a larger scale. As a leader in urban conservation, Metro is poised to make a meaningful scientific contribution by sharing phenology data with regional and national organizations. Data-sharing will benefit the common goal of conservation and create avenues for collaboration with other scientists and conservation practitioners (Rosemartin 2013). In order to support Metro’s ongoing conservation efforts in Oregon white oak systems, I have implemented a three-part master’s project. Part one of the project examines Metro’s previously collected phenology data, providing descriptive statistics and assessing the strengths and weaknesses of the methods by which the data were collected. Part two makes recommendations for improving future phenology data-collection methods, and includes recommendations for datasharing with regional and national organizations. Part three is a collection of scientific vouchers documenting key plant species in varying phases of phenology for Metro’s teaching herbarium. The purpose of these vouchers is to provide a visual tool for Metro staff and volunteers who rely on plant identification to carry out aspects of their job in plant conservation. Each component of this project addresses specific aspects of Metro’s conservation program, from day-to-day management concerns to long-term scientific inquiry.
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Morin, Shai, Gregory Walker, Linda Walling, and Asaph Aharoni. Identifying Arabidopsis thaliana Defense Genes to Phloem-feeding Insects. United States Department of Agriculture, February 2013. http://dx.doi.org/10.32747/2013.7699836.bard.

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The whitefly (Bemisia tabaci) is a serious agricultural pest that afflicts a wide variety of ornamental and vegetable crop species. To enable survival on a great diversity of host plants, whiteflies must have the ability to avoid or detoxify numerous different plant defensive chemicals. Such toxins include a group of insect-deterrent molecules called glucosinolates (GSs), which also provide the pungent taste of Brassica vegetables such as radish and cabbage. In our BARD grant, we used the whitefly B. tabaci and Arabidopsis (a Brassica plant model) defense mutants and transgenic lines, to gain comprehensive understanding both on plant defense pathways against whiteflies and whitefly defense strategies against plants. Our major focus was on GSs. We produced transgenic Arabidopsis plants accumulating high levels of GSs. At the first step, we examined how exposure to high levels of GSs affects decision making and performance of whiteflies when provided plants with normal levels or high levels of GSs. Our major conclusions can be divided into three: (I) exposure to plants accumulating high levels of GSs, negatively affected the performance of both whitefly adult females and immature; (II) whitefly adult females are likely to be capable of sensing different levels of GSs in their host plants and are able to choose, for oviposition, the host plant on which their offspring survive and develop better (preference-performance relationship); (III) the dual presence of plants with normal levels and high levels of GSs, confused whitefly adult females, and led to difficulties in making a choice between the different host plants. These findings have an applicative perspective. Whiteflies are known as a serious pest of Brassica cropping systems. If the differences found here on adjacent small plants translate to field situations, intercropping with closely-related Brassica cultivars could negatively influence whitefly population build-up. At the second step, we characterized the defensive mechanisms whiteflies use to detoxify GSs and other plant toxins. We identified five detoxification genes, which can be considered as putative "key" general induced detoxifiers because their expression-levels responded to several unrelated plant toxic compounds. This knowledge is currently used (using new funding) to develop a new technology that will allow the production of pestresistant crops capable of protecting themselves from whiteflies by silencing insect detoxification genes without which successful host utilization can not occur. Finally, we made an effort to identify defense genes that deter whitefly performance, by infesting with whiteflies, wild-type and defense mutated Arabidopsis plants. The infested plants were used to construct deep-sequencing expression libraries. The 30- 50 million sequence reads per library, provide an unbiased and quantitative assessment of gene expression and contain sequences from both Arabidopsis and whiteflies. Therefore, the libraries give us sequence data that can be mined for both the plant and insect gene expression responses. An intensive analysis of these datasets is underway. We also conducted electrical penetration graph (EPG) recordings of whiteflies feeding on Arabidopsis wild-type and defense mutant plants in order to determine the time-point and feeding behavior in which plant-defense genes are expressed. We are in the process of analyzing the recordings and calculating 125 feeding behavior parameters for each whitefly. From the analyses conducted so far we conclude that the Arabidopsis defense mutants do not affect adult feeding behavior in the same manner that they affect immatures development. Analysis of the immatures feeding behavior is not yet completed, but if it shows the same disconnect between feeding behavior data and developmental rate data, we would conclude that the differences in the defense mutants are due to a qualitative effect based on the chemical constituency of the phloem sap.
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Bishop, Bradley Wade. Data from Data Management Plan Compliance. University of Tennessee, Knoxville Libraries, January 2020. http://dx.doi.org/10.7290/pebuwhcq7l.

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Simmons, Trey. Data quality standards for monitoring stream ecosystems in the Central Alaska Network. National Park Service, 2017. http://dx.doi.org/10.36967/2244207.

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The purpose of this report is to document the standards used by the Central Alaska Inventory and Monitoring Network (CAKN) for activities related to the collection, processing, storage, analysis, and publication of monitoring data as described in the CAKN Stream Monitoring Protocol (Simmons 2017a). The policies and procedures documented in this quality-assurance plan for activities complement the quality-assurance plans for other monitoring activities conducted by the CAKN. The plan also serves as a guide for all CAKN personnel who are involved in protocol/program activities and as a resource for identifying memoranda, publications, and other literature that describe associated techniques and requirements in more detail.
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Ron, Eliora, and Eugene Eugene Nester. Global functional genomics of plant cell transformation by agrobacterium. United States Department of Agriculture, March 2009. http://dx.doi.org/10.32747/2009.7695860.bard.

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The aim of this study was to carry out a global functional genomics analysis of plant cell transformation by Agrobacterium in order to define and characterize the physiology of Agrobacterium in the acidic environment of a wounded plant. We planed to study the proteome and transcriptome of Agrobacterium in response to a change in pH, from 7.2 to 5.5 and identify genes and circuits directly involved in this change. Bacteria-plant interactions involve a large number of global regulatory systems, which are essential for protection against new stressful conditions. The interaction of bacteria with their hosts has been previously studied by genetic-physiological methods. We wanted to make use of the new capabilities to study these interactions on a global scale, using transcription analysis (transcriptomics, microarrays) and proteomics (2D gel electrophoresis and mass spectrometry). The results provided extensive data on the functional genomics under conditions that partially mimic plant infection and – in addition - revealed some surprising and significant data. Thus, we identified the genes whose expression is modulated when Agrobacterium is grown under the acidic conditions found in the rhizosphere (pH 5.5), an essential environmental factor in Agrobacterium – plant interactions essential for induction of the virulence program by plant signal molecules. Among the 45 genes whose expression was significantly elevated, of special interest is the two-component chromosomally encoded system, ChvG/I which is involved in regulating acid inducible genes. A second exciting system under acid and ChvG/Icontrol is a secretion system for proteins, T6SS, encoded by 14 genes which appears to be important for Rhizobium leguminosarum nodule formation and nitrogen fixation and for virulence of Agrobacterium. The proteome analysis revealed that gamma aminobutyric acid (GABA), a metabolite secreted by wounded plants, induces the synthesis of an Agrobacterium lactonase which degrades the quorum sensing signal, N-acyl homoserine lactone (AHL), resulting in attenuation of virulence. In addition, through a transcriptomic analysis of Agrobacterium growing at the pH of the rhizosphere (pH=5.5), we demonstrated that salicylic acid (SA) a well-studied plant signal molecule important in plant defense, attenuates Agrobacterium virulence in two distinct ways - by down regulating the synthesis of the virulence (vir) genes required for the processing and transfer of the T-DNA and by inducing the same lactonase, which in turn degrades the AHL. Thus, GABA and SA with different molecular structures, induce the expression of these same genes. The identification of genes whose expression is modulated by conditions that mimic plant infection, as well as the identification of regulatory molecules that help control the early stages of infection, advance our understanding of this complex bacterial-plant interaction and has immediate potential applications to modify it. We expect that the data generated by our research will be used to develop novel strategies for the control of crown gall disease. Moreover, these results will also provide the basis for future biotechnological approaches that will use genetic manipulations to improve bacterial-plant interactions, leading to more efficient DNA transfer to recalcitrant plants and robust symbiosis. These advances will, in turn, contribute to plant protection by introducing genes for resistance against other bacteria, pests and environmental stress.
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García-Espinosa, J., and C. Soriano. Data management plan. Scipedia, 2021. http://dx.doi.org/10.23967/prodphd.2021.9.003.

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Анотація:
This document presents the deliverable D8.1 – the Data Management Plan (DMP) of work package 8 of the prodPhD project. It aims to present the plan for the management, generation, collection, security, preservation and sharing of data generated through the prodPhD project. The DMP is a key element for organizing the project’s data. It provides an analysis of the data, which will be collected, processed and published by the prodPhD consortium. The project embraces the initiatives of the European Commission to promote the open access to research data, aiming to improve and maximize access to and reuse of research data generated by Horizon 2020 projects. In this sense prodPhD will adhere to the Open Research Data Pilot (ORD Pilot) fostered by the European Commission, and this DMP will be developed following the standards of data storage, access and management. This plan will detail what data will be generated through the project, whether and how it will be made accessible for the verification and reuse and how it will be curated and preserved. In this context, the term data applies to the information generated during the different experimental campaigns carried out in the project, and specifically to the data, including associated metadata, to be used to validate the computational models and the technical solutions to be developed in the project. This document is the first version of the DMP and may be updated throughout the project, if significant changes (new data, changes in consortium policies, changes in consortium composition, etc.) arise.
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8

Paglialonga, Lisa, and Carsten Schirnick. Data management plan. OceanNETs, June 2022. http://dx.doi.org/10.3289/oceannets_d8.1.

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Анотація:
This is the data management plan for the research project OceanNETs. It compiles OceanNETs research data output and describes the data handling during and after the projects duration with the aim to make OceanNETs research data FAIR – sustainably available for the scientific community. This data management plan is a living document; it will be continuously developed in close cooperation with the consortium members throughout the project duration
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9

Papke, Leslie. Participation in and Contributions to 401(k) Pension Plans: Evidence om Plan Data. Cambridge, MA: National Bureau of Economic Research, October 1992. http://dx.doi.org/10.3386/w4199.

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10

Fan, Jianhua, Zhiyong Tian, Simon Furbo, Weiqiang Kong, and Daniel Tschopp. Simulation and design of collector array units within large systems. IEA SHC Task 55, October 2019. http://dx.doi.org/10.18777/ieashc-task55-2019-0004.

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Анотація:
Solar radiation data is necessary for the design of solar heating systems and used to estimate the thermal performance of solar heating plants. Compared to global irradiance, the direct beam component shows much more variability in space and time. The global radiation split into beam and diffuse radiation on collector plane is important for the evaluation of the performance of different collector types and collector field designs.
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