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Learning mid-IR emission spectra of polycyclic aromatic hydrocarbon populations from observations
Sacha Foschino, Olivier Berné, Christine Joblin
The JWST will deliver large data sets of high-quality spectral data over the 0.6-28 m range. It will combine sensitivity, spectral and spatial resolution. Specific tools are req…
Faint end of the luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE
G. de La Vieuville, D. Bina, R. Pello +21
We present the results obtained with VLT/MUSE on the faint-end of the Lyman-alpha luminosity function (LF) based on deep observations of four lensing clusters. The precise aim of t…
Accretion in Stellar-Mass Black Holes at High X-ray Spectral Resolution
J. M. Miller, D. Barret, E. Cackett +9
Accretion disks around stellar-mass black holes offer unique opportunities to study the fundamental physics of standard thin disks, super-Eddington disks, and structure that may be…
Consistent dust and gas models for protoplanetary disks IV. A panchromatic view of protoplanetary disks
O. Dionatos, P. Woitke, M. Guedel +17
Consistent modeling of protoplanetary disks requires the simultaneous solution of both continuum and line radiative transfer, heating/cooling balance between dust and gas and, of c…