The statistic shows the market share of smartphones in use in Europe, by device, from the second quarter of 2015 to the second quarter of 2018. The Apple iPhone X model had a market share of 1.9 percent in the second quarter of 2018.

Restart files for CLM-FATES version 2.0.1 for CLM-FATES EMERALD version 2.0.1.

CTSM_FATES-EMERALD_on_inputdata_version2.0.0_ALP1.tar_(restart_info):
- ALP1_refcase.datm.r.2300-01-01-00000.nc
- ALP1_refcase.datm.rs1.2300-01-01-00000.bin
- ALP1_refcase.cpl.r.2300-01-01-00000.nc
- ALP1_refcase.clm2.r.2300-01-01-00000.nc

This dataset is being used in the Galaxy Training tutorial on CLM-FATES.

This work has been done in in collaboration with Galaxy Europe and EOSC-Life:
- Within the 1st EOSC-Life Training Open Call, two out of four proposals have been awarded to the European Galaxy team to develop climate science e-learning material and mentoring and training opportunities for our communities.

CLM-FATES documentation can be found here.

The statistic shows the market share of tablets in use in Europe, by device, from the second quarter of 2015 to the second quarter of 2018. The Apple iPad Air model had a market share of 8.14 percent in the second quarter of 2018.

This repository contains datasets required for the online training "Data analysis and interpretation for clinical genomics" available at https://sigu-training.github.io/clinical_genomics/.

Tools used in the training are available at the European Galaxy instance running at https://usegalaxy.eu, which also includes a copy of this repository in the Shared Data Libraries. BAM files in this dataset are based on the hg38 reference genome.

This is part of a 4 dataset submission. Refer to this dataset for details.

This repository contains datasets required for the online training "Data analysis and interpretation for clinical genomics" available at https://sigu-training.github.io/clinical_genomics/.

Tools used in the training are available at the European Galaxy instance running at https://usegalaxy.eu, which also includes a copy of this repository in the Shared Data Libraries. BAM files in this dataset are based on the hg38 reference genome.

This is part of a 4 dataset submission. Refer to this dataset for details.

Europe Black Granite market size is USD 206742.66 million in 2024 and will expand at a compound annual growth rate (CAGR) of 1.0% from 2024 to 2031.

In years 2018-2019, we organized on behalf of the Italian Society of Human Genetics (SIGU) an itinerant Galaxy-based “hands-on-computer” training activity entitled “Data analysis and interpretation for clinical genomics”. This one-day course was offered to participants including clinical doctors, biologists, laboratory technicians and bioinformaticians. Topics covered by the course were NGS data quality check, detection of variants, copy number alterations and runs of homozygosity, annotation and filtering and clinical interpretation of sequencing results.

To meet the constant need for training on basic NGS analysis and interpretation of sequencing data in the clinical setting, we designed an on-line Galaxy-based training resource dedicated to this topic, articulated in presentations and practical assignments by which students will learn how to approach NGS data processing at the level of FASTQ, BAM and VCF files and clinically-oriented examination of variants emerging from sequencing experiments such as whole exomes.

This repository contains datasets required for the online training "Data analysis and interpretation for clinical genomics" available at https://sigu-training.github.io/clinical_genomics/.

Tools used in the training are available at the European Galaxy instance running at https://usegalaxy.eu, which also includes a copy of this repository in the Shared Data Libraries. Files named Fam_*.bam are based on hg38 reference genome; all the other files refer to hg19.

This is part of a 4 dataset submission.

The effect of environment is an essential, but poorly understood ingredient ingalaxy formation. We propose to measure the gas and dark matter in the clumpsand filaments around two massive distant galaxy clusters. By combining highquality XMM data with our existing widefield opticalNIR imaging andspectroscopy we will perform a census of the baryons in the large scalestructure around these clusters and measure the effects of environment on thefundamental physical properties of the member galaxies. Combined with a stackedweak lensing analysis, the Xray data will be used to perform the first test ofthe galaxy group massobservable scaling relations in an LSS environment,thereby probing the role of environment on preheating in groups. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]

SDSSC4 3028 is a cluster of galaxies identified in the Sloan Digital SkySurvey. It stands out as a nearby cluster containing a surprisingly largefraction of star forming galaxies, which is not fully understood in the standardmodel of galaxy evolution. It is also very unusual that the brightest galaxy ofthis cluster is a passive red spiral galaxy. We propose an XMM pointing thatcovers the entire cluster to determine its dynamical state and to obtain a morerobust cluster mass measurement. We will also verify whether this passive redspiral galaxy is the brightest cluster galaxy residing at the the bottom of thegravitational potential of this cluster. SDSSC4 3028 provides a valuableopportunity to study the evolutionary link between galaxies and clusters. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]

We propose a 100 ksec XMM observation of the isolated elliptical galaxy NGC2325,a fairly typical galaxy in terms of its Xray and optical luminosity. Studies ofisolated galaxies allow us to investigate the intrinsic properties of the hotgas halos in earlytype galaxies without the complicating effects of a clusteror group environment, and we will study in detail the metallicity, entropy, andtemperature profiles in this galaxy as indications of the effectiveness ofenrichment and feedback processes. In addition, we will shed light on the debateover the dark matter density profiles of ellipticals by uniquely determining themass profile of the same isolated galaxy using both deep Xray and opticaldynamical measurements. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]

Galaxy groups are ideal systems to study baryon physics, which is important forboth using clusters for precision cosmology and understanding galaxy formationand evolution. Over the last decade, our understanding on the ICM properties ofgalaxy groups has been greatly improved. However, there is no a representativegroup sample with Chandra or XMM that allows full coverage to r_500. We definedsuch a sample of 13 galaxy groups that are Xray luminosity selected from the400 deg^2 survey (REGOS4). The lowL_X bin was approved in the last XMM cycle.Complete Chandra coverage (mostly short exposures) and other supporting datahave also been obtained. We now propose to observe the highL_X bin with XMM tofinish REGOS4 and ensure a continuous L_X coverage from REXCESS to REGOS4. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]

Powerful radio galaxies have played a central role in our understanding of active galaxies over the past five decades. CygnusA, the brightest and most nearby FRII source, has been a Rosetta Stone in this study.It appears to have the outward characteristics of a normal radio galaxybut its proximity allows us to identify the more subtle properties ofan obscured quasar. The energy provided by this very active galaxyis sufficient to launch the energetic jets we observe but the transportof the energy to the hotspots is poorly constrained and understood.The growing realisation that AGN directly affect their host galaxythrough a direct feedback mechanism throughout the lifetime of thegalaxy makes it especially important for the most nearby obscured quasar to be observed with the widest possible spectral coverage.We propose to use Herschel to reveal the heating of the central region and the energetics of the hotspots. We request observations of theatomic cooling lines OI, OIII and CII that will allow us to compare theenergetics of the ISM in Cygnus A with other local and more distantgalaxies. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]

We propose to observe a newly discovered galaxy cluster around the radio galaxy3C 210 at z1.17. We intend to obtain a 20 Ksec ACIS exposure to identify pointsources, which can severely bias measurements of extended emission in highzclusters, and to study the radio galaxy itself. We also ask to obtain a 100 ksEPIC exposure to measure the properties of the intracluster medium including itsXray temperature and morphology. These observations will help to understand theway that galaxy clusters create an ICM as they evolve from the protoclustersrecently discovered at 2<z<4, and to act as a pathfinder for the futureexploitation of high redshift galaxy clusters in understanding dark energy. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]