415 citations
- Spanish National ObservatoryES25 papers
- Yebes ObservatoryES14 papers
- Max Planck Institute for Radio AstronomyDE13 papers
- Consejo Superior de Investigaciones CientíficasES12 papers
- Institut de Radioastronomie MillimétriqueFR9 papers
- Centre National de la Recherche ScientifiqueFR8 papers
- Centro de AstrobiologíaES8 papers
- Chalmers University of TechnologySE8 papers
- Arcetri Astrophysical ObservatoryIT7 papers
- Center for Astrophysics Harvard & SmithsonianUS6 papers
- Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et AtmosphèresFR6 papers
- Observatoire de ParisFR6 papers
51 papers
XRISM Resolves the Circum-nuclear Environment of NGC 4945
Peter G. Boorman, Poshak Gandhi, Yoshihiro Ueda +31
Compton-thick Active Galactic Nuclei (AGN) represent one of the most elusive phases of massive black hole growth, yet are expected to contribute substantially to the Cosmic X-ray B…
How reliable are remote sensing maps calibrated over large areas? A matter of scale?
Andrey Ramirez Luigui, Jean-Pierre Renaud, Cédric Vega
Remote sensing data are increasingly available and frequently used to produce forest attributes maps. The sampling strategy of the calibration plots may directly affect predictions…
Linking the dust and chemical evolution: Taurus and Perseus -- New collisional rates for HCN, HNC, and their C, N, and H isotopologues
D. Navarro-Almaida, C. T. Bop, F. Lique +18
HCN, HNC, and their isotopologues are ubiquitous molecules that can serve as chemical thermometers and evolutionary tracers to characterize star-forming regions. Despite their impo…
The Canfranc Axion Detection Experiment (CADEx): Search for axions at 90 GHz with Kinetic Inductance Detectors
Beatriz Aja, Sergio Arguedas Cuendis, Ivan Arregui +33
We propose a novel experiment, the Canfranc Axion Detection Experiment (CADEx), to probe dark matter axions with masses in the range 330-460 eV, within the W-band (80-110 GHz),…
Ultra-deep 31.0-50.3 GHz spectral survey of IRC+10216
J. R. Pardo, J. Cernicharo, B. Tercero +8
Context. IRC+10216, the carbon-rich envelope of the asymptotic giant branch (AGB) star CW Leo, is one of the richest molecular sources in the sky. Available spectral surveys below…
Magnesium radicals MgCN and MgCH in IRC+10216
J. R. Pardo, C. Cabezas, J. P. Fonfría +5
After the previous discovery of MgCN and MgCH in IRC+10216, a deeper Q-band (31.0-50.3 GHz) integration on this source had revealed two additional series of harmonically re…