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100 simulated line of sights up to z=1
100 column data up to z=1 from an MHD cosmological simulation run using ENZO (Bryan+14). All dataset are written in a formatted way. Each column contains: redshift, electron... -
Simulated cluster with MHD, resolution 220kpc
Innermost (7.04 Mpc)^3 for a simulated cluster at z=0 using ENZO and MHD, as in http://arxiv.org/abs/1409.2640. The hdf5 datasets contains 32^3 distribution of cells for... -
Simulated cluster with MHD, resolution 22kpc
Innermost (7.04 Mpc)^3 for a simulated cluster at z=0 using ENZO and MHD, as in http://arxiv.org/abs/1409.2640. The hdf5 datasets contains 320^3 distribution of cells for... -
Simulated cluster with MHD, resolution 22kpc (TRUE ONE!)
Innermost (7.04 Mpc)^3 for a simulated cluster at z=0 using ENZO and MHD, as in http://arxiv.org/abs/1409.2640. The hdf5 datasets contains 256^3 distribution of cells for... -
Simulated cluster with MHD, resolution 27pc
Innermost (7.04 Mpc)^3 for a simulated cluster at z=0 using ENZO and MHD, as in http://arxiv.org/abs/1409.2640. The hdf5 datasets contains 256^3 distribution of cells for... -
Simulated cluster with MHD, resolution 55kpc
Innermost (7.04 Mpc)^3 for a simulated cluster at z=0 using ENZO and MHD, as in http://arxiv.org/abs/1409.2640. The hdf5 datasets contains 128^3 distribution of cells for... -
SPIRE (f250um>17.4mJy) GOODS-N galaxies
For the first time, we investigate the X-ray/infrared (IR) correlation for star-forming galaxies (SFGs) at z~1, using SPIRE submm data from the recently launched Herschel Space... -
Supernovae in the Subaru Deep Field
The Type Ia supernova (SN Ia) rate, when compared to the cosmic star formation history (SFH), can be used to derive the delay-time distribution (DTD; the hypothetical SN Ia rate... -
New brown dwarfs in upper Sco
This paper presents the results of a search for brown dwarfs in the Upper Scorpius Association using data from the UKIRT Infrared Deep Sky Survey (UKIDSS) Galactic Cluster...
