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Reply to: Explaining bright radar reflections below the south pole of Mars without liquid water

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The Original Article was published on 26 September 2022

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Fig. 1: Attenuation as a function of frequency in the SPLD.
Fig. 2: Simulation results for scenario 3.

Data availability

MARSIS data are available through the Zenodo research data repository at https://doi.org/10.5281/zenodo.1285179.

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Authors and Affiliations

  1. Dipartimento di Matematica e Fisica, Università degli studi Roma Tre, Rome, Italy

    Sebastian Emanuel Lauro, Elena Pettinelli, Elisabetta Mattei, Barbara Cosciotti & F. Di Paolo

  2. Centre for Astrophysics, University of Southern Queensland, Toowomba, Queensland, Australia

    Graziella Caprarelli

  3. Istituto di Radioastronomia (IRA), Istituto Nazionale di Astrofisica (INAF), Bologna, Italy

    Luca Guallini

  4. Department of Physics and Earth Sciences, Jacobs University Bremen, Bremen, Germany

    Angelo Pio Rossi

  5. Istituto di Astrofisica e Planetologia Spaziali (IAPS), Istituto Nazionale di Astrofisica (INAF), Rome, Italy

    Andrea Cicchetti, M. Cartacci & R. Noschese

  6. Istituto per il Rilevamento Elettromagnetico dell’Ambiente, Consiglio Nazionale delle Ricerche, Naples, Italy

    Francesco Soldovieri & R. Orosei

Authors
  1. Sebastian Emanuel Lauro
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  2. Elena Pettinelli
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  3. Graziella Caprarelli
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  4. Luca Guallini
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  6. Elisabetta Mattei
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  7. Barbara Cosciotti
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  8. Andrea Cicchetti
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  9. Francesco Soldovieri
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  11. F. Di Paolo
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  12. R. Noschese
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  13. R. Orosei
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Contributions

All authors equally contributed to the discussion and the data analysis; S.E.L., E.P., G.C., E.M., B.C., F.S. and R.O. wrote and revised the manuscript.

Corresponding author

Correspondence to Elena Pettinelli.

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Lauro, S.E., Pettinelli, E., Caprarelli, G. et al. Reply to: Explaining bright radar reflections below the south pole of Mars without liquid water. Nat Astron 7, 259–261 (2023). https://doi.org/10.1038/s41550-022-01871-0

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