Publication type: Non-refereed

  • Publication
    Retrieving the Transmission Spectrum of HD209458b using CHOCOLATE: a new Chromatic Line-Profile Technique
    Multi-band photometric transit observations or low resolution spectroscopy (spectro-photometry) are normally used to retrieve the broadband transmission spectra...
  • Publication
    Revealing Low Luminosity Active Galactic Nuclei (ReveaLLAGN)
    JWST will be the most sensitive tool ever built for studying the accretion onto supermassive black holes (SMBHs) at the centers of galaxies. While quasars and...
  • Publication
    Revealing the Brown Dwarf Population in the Pleiades Open Cluster
    Not Available
  • Publication
    Revealing the origin of the cold ISM in massive early-type galaxies
    Recently, massive early-type galaxies have shed their red-and-dead moniker, thanks to the discovery that many host residual star formation. As part of the ATLAS...
  • Publication
    Reverberation lags in black hole X-ray binaries
    Reprocessing of the primary X-ray continuum in the accretion disc is expected to cause reverberation lags which are powerful diagnostics of the geometry of the...
  • Publication
    Reversal-free Ca II H Profiles: a Challenge for Solar Chromosphere Modeling in Quiet Inter-Network
    There is no agreement on the thermal structure of the solar chromosphere. While results of the CO observations and 3D MHD simulations suggest very cool...
  • Publication
    Review of J.A. Hill, P. Jones and A.J. Morales (eds.), Experiencing Power, Generating Authority: Cosmos, Politics, and the Ideology of Kingship in Ancient Egypt and Mesopotamia; Penn Museum International Research Conferences 6, University of Pennsylvania
  • Publication
    Reviews of Publications/Critiques d'ouvrages- Instrumentation for Large Telescopes, edited
    Not Available
  • Publication
    Revised chemistry of HD209458 b
    We characterize the atmosphere of the iconic giant planet HD209458 b based on a joint modeling effort of the available observations. HD 209458 b is the first...