DOI,IST REx ID,Title of publication
10.1086/321567,17829,Extended Lyα emission around young quasars: A constraint on galaxy formation
10.1086/320586,17831,What is the highest plausible redshift of luminous quasars?
10.1086/322393,17832,Constraints on warm dark matter from cosmological reionization
10.1086/319732,17840,"Probing early structure formation with far‐infrared background correlations"
10.1086/324309,17846,"Constraints on Ωm, ΩΛ, and σ8 from galaxy cluster redshift distributions"
10.1086/320232,17847,Photon consumption in minihalos during cosmological reionization
10.1086/320939,17849,Constraints on cosmological parameters from future galaxy cluster surveys
10.1109/icip.2004.1421428,18397,Optimal sparse representations for blind source separation and blind deconvolution: A learning approach
10.1063/1.1434627,18736,Probing the cosmic dark age in X-rays
10.1063/1.1419569,18743,Clusters in the precision cosmology era
10.1063/1.1419543,18747,"Warm Dark Matter, small scale crisis, and the high redshift universe"
10.1038/ncb1201-1086,11125,Distinct AAA-ATPase p97 complexes function in discrete steps of nuclear assembly
10.1007/978-3-0348-8231-6,2340,Bosons in a trap: Asymptotic exactness of the Gross-Pitaevskii ground state energy formula
10.1007/PL00001032,2341,Atoms with bosonic &quot;electrons&quot; in strong magnetic fields
10.1088/0305-4470/34/9/311,2345,On the maximal ionization of atoms in strong magnetic fields
10.1023/A:1010951905548,2346,Bounds on one-dimensional exchange energies with application to lowest Landau band quantum mechanics
10.1007/s002200100533,2347,A rigorous derivation of the Gross-Pitaevskii energy functional for a two-dimensional Bose gas
10.1007/s002200100373,2348,A discrete density matrix theory for atoms in strong magnetic fields
10.1007/s00454-001-0028-9,2419,A continuous analogue of the Upper Bound Theorem
10.1002/cne.1114,2604,Light and electron microscopic study of the distribution of substance P-immunoreactive fibers and neurokinin-1 receptors in the skin of the rat lower lip
