Search Results - "BENZ, W"

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  1. 1

    Tectonic collision and uplift of Wallacea triggered the global songbird radiation by Moyle, Robert G., Oliveros, Carl H., Andersen, Michael J., Hosner, Peter A., Benz, Brett W., Manthey, Joseph D., Travers, Scott L., Brown, Rafe M., Faircloth, Brant C.

    Published in Nature communications (30-08-2016)
    “…Songbirds (oscine passerines) are the most species-rich and cosmopolitan bird group, comprising almost half of global avian diversity. Songbirds originated in…”
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    Journal Article
  2. 2

    The CHEOPS mission by Benz, W., Broeg, C., Fortier, A., Rando, N., Beck, T., Beck, M., Queloz, D., Ehrenreich, D., Maxted, P. F. L., Isaak, K. G., Billot, N., Alonso, R., António, C., Asquier, J., Bandy, T., Bárczy, T., Barrado, D., Barros, S. C. C., Baumjohann, W., Bekkelien, A., Bergomi, M., Biondi, F., Bonfils, X., Borsato, L., Brandeker, A., Busch, M.-D., Cabrera, J., Cessa, V., Charnoz, S., Chazelas, B., Collier Cameron, A., Corral Van Damme, C., Cortes, D., Davies, M. B., Deleuil, M., Deline, A., Delrez, L., Demangeon, O., Demory, B. O., Erikson, A., Farinato, J., Fossati, L., Fridlund, M., Futyan, D., Gandolfi, D., Garcia Munoz, A., Gillon, M., Guterman, P., Gutierrez, A., Hasiba, J., Hoyer, S., Kiss, L. L., Kuntzer, T., Laskar, J., Lecavelier des Etangs, A., Lendl, M., López, A., Lora, I., Lovis, C., Lüftinger, T., Magrin, D., Malvasio, L., Marafatto, L., Michaelis, H., de Miguel, D., Modrego, D., Munari, M., Nascimbeni, V., Ottacher, H., Ottensamer, R., Pagano, I., Palacios, R., Pallé, E., Peter, G., Piotto, G., Pizarro, A., Pollaco, D., Ragazzoni, R., Rauer, H., Rieder, M., Rohlfs, R., Safa, F., Salatti, M., Santos, N. C., Ségransan, D., Simon, A. E., Smith, A. M. S., Sordet, M., Sousa, S. G., Szabó, G. M., Szoke, J., Thomas, N., Tschentscher, M., Udry, S., Van Grootel, V., Viotto, V., Walter, I., Walton, N. A., Wildi, F., Wolter, D.

    Published in Experimental astronomy (2021)
    “…The CHaracterising ExOPlanet Satellite (CHEOPS) was selected on October 19, 2012, as the first small mission (S-mission) in the ESA Science Programme and…”
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  3. 3

    The structure of the asteroid 4 Vesta as revealed by models of planet-scale collisions by Jutzi, M., Asphaug, E., Gillet, P., Barrat, J.-A., Benz, W.

    Published in Nature (London) (14-02-2013)
    “…Three-dimensional simulations of the global evolution of asteroid 4 Vesta under two overlapping planet-scale collisions closely reproduce its observed shape;…”
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    CHEOPS: A transit photometry mission for ESA's small mission programme by Broeg, C., Fortier, A., Ehrenreich, D., Alibert, Y., Baumjohann, W., Benz, W., Deleuil, M., Gillon, M., Ivanov, A., Liseau, R., Meyer, M., Oloffson, G., Pagano, I., Piotto, G., Pollacco, D., Queloz, D., Ragazzoni, R., Renotte, E., Steller, M., Thomas, N.

    Published in EPJ Web of Conferences (01-01-2013)
    “…Ground based radial velocity (RV) searches continue to discover exoplanets below Neptune mass down to Earth mass. Furthermore, ground based transit searches…”
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    Journal Article Conference Proceeding
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    The PLATO 2.0 mission by Rauer, H., Catala, C., Benz, W., Christensen-Dalsgaard, J., Deleuil, M., Goupil, M.-J., Janot-Pacheco, E., Santos, Ċ., Smith, A., Suárez, J.-C., Adibekyan, V., Alibert, Y., Almenara, J.-M., Barnes, S., Baudin, F., Bergemann, M., Bihain, G., Birch, A. C., Bonfils, X., Boisse, I., Bonomo, A. S., Borsa, F., Brandão, I. M., Brun, S., Burleigh, M., Cabrera, J., Charpinet, S., Church, R. P., Csizmadia, Sz, Cunha, M., Davies, M. B., Deeg, H. J., Díaz, R. F., Dreizler, S., Dreyer, C., Eggenberger, P., Eigmüller, P., Erikson, A., Farmer, R., Figueira, P., Fridlund, M., Giuffrida, G., da Silva, J. Gomes, Granzer, T., Grenfell, J. L., Günther, E., Haswell, C. A., Hébrard, G., Hekker, S., Heng, K., Johansen, A., Kislyakova, K. G., Kupka, F., Lammer, H., Marcos-Arenal, P., Marrese, P. M., Marques, J. P., Martins, J., Mathis, S., Mathur, S., Miglio, A., Montalban, J., Montalto, M., Moravveji, E., Morel, T., Mortier, A., Nascimbeni, V., Nelson, R. P., Nielsen, M. B., Noack, L., Norton, A. J., Ofir, A., Pápics, P., Quirrenbach, A., Raimondo, G., Rainer, M., Reese, D. R., Redmer, R., Reffert, S., Rojas-Ayala, B., Roxburgh, I. W., Salmon, S., Santerne, A., Schneider, J., Schou, J., Schuh, S., Schunker, H., Silva-Valio, A., Skillen, I., Snellen, I., Sozzetti, A., Strassmeier, K. G., Švanda, M., Tkachenko, A., Van Grootel, V., Vauclair, S. D., Ventura, P., Wagner, F. W., Wheatley, P. J., Zwintz, K.

    Published in Experimental astronomy (01-11-2014)
    “…PLATO 2.0 has recently been selected for ESA’s M3 launch opportunity (2022/24). Providing accurate key planet parameters (radius, mass, density and age) in…”
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    Investigating the architecture and internal structure of the TOI-561 system planets with CHEOPS, HARPS-N, and TESS by Lacedelli, G, Wilson, T G, Malavolta, L, Hooton, M J, Collier Cameron, A, Alibert, Y, Mortier, A, Bonfanti, A, Haywood, R D, Hoyer, S, Piotto, G, Bekkelien, A, Vanderburg, A M, Benz, W, Dumusque, X, Deline, A, López-Morales, M, Borsato, L, Rice, K, Fossati, L, Latham, D W, Brandeker, A, Poretti, E, Sousa, S G, Sozzetti, A, Salmon, S, Burke, C J, Van Grootel, V, Fausnaugh, M M, Adibekyan, V, Huang, C X, Osborn, H P, Mustill, A J, Pallé, E, Bourrier, V, Nascimbeni, V, Alonso, R, Anglada, G, Bárczy, T, Barrado y Navascues, D, Barros, S C C, Baumjohann, W, Beck, M, Beck, T, Billot, N, Bonfils, X, Broeg, C, Buchhave, L A, Cabrera, J, Charnoz, S, Cosentino, R, Csizmadia, Sz, Davies, M B, Deleuil, M, Delrez, L, Demangeon, O, Demory, B -O, Ehrenreich, D, Erikson, A, Esparza-Borges, E, Florén, H G, Fortier, A, Fridlund, M, Futyan, D, Gandolfi, D, Ghedina, A, Gillon, M, Güdel, M, Guterman, P, Harutyunyan, A, Heng, K, Isaak, K G, Jenkins, J M, Kiss, L, Laskar, J, Lecavelier des Etangs, A, Lendl, M, Lovis, C, Magrin, D, Marafatto, L, Martinez Fiorenzano, A F, Maxted, P F L, Mayor, M, Micela, G, Molinari, E, Murgas, F, Narita, N, Olofsson, G, Ottensamer, R, Pagano, I, Pasetti, A, Pedani, M, Pepe, F A, Peter, G, Phillips, D F, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Ratti, F

    “…We present a precise characterization of the TOI-561 planetary system obtained by combining previously published data with TESS and CHEOPS photometry, and a…”
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  10. 10

    The Origin of Mercury by Benz, W, Anic, A, Horner, J, Whitby, JA

    Published in Space science reviews (01-10-2007)
    “…Issue Title: Mercury Mercury's unusually high mean density has always been attributed to special circumstances that occurred during the formation of the planet…”
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    Journal Article
  11. 11

    The EBLM project – VIII. First results for M-dwarf mass, radius, and effective temperature measurements using CHEOPS light curves by Swayne, M I, Maxted, P F L, Triaud, A H M J, Sousa, S G, Broeg, C, Florén, H-G, Guterman, P, Simon, A E, Boisse, I, Bonfanti, A, Martin, D, Santerne, A, Salmon, S, Standing, M R, Van Grootel, V, Wilson, T G, Alibert, Y, Alonso, R, Anglada Escudé, G, Asquier, J, Bárczy, T, Barrado, D, Barros, S C C, Battley, M, Baumjohann, W, Beck, M, Beck, T, Bekkelien, A, Benz, W, Billot, N, Bonfils, X, Brandeker, A, Busch, M-D, Cabrera, J, Charnoz, S, Collier Cameron, A, Csizmadia, Sz, Davies, M B, Deleuil, M, Deline, A, Delrez, L, Demangeon, O D S, Demory, B-O, Dransfield, G, Ehrenreich, D, Erikson, A, Fortier, A, Fossati, L, Fridlund, M, Futyan, D, Gandolfi, D, Gillon, M, Guedel, M, Hébrard, G, Heidari, N, Hellier, C, Heng, K, Hobson, M, Hoyer, S, Isaak, K G, Kiss, L, Kunovac Hodžić, V, Lalitha, S, Laskar, J, Lecavelier des Etangs, A, Lendl, M, Lovis, C, Magrin, D, Marafatto, L, McCormac, J, Miller, N, Nascimbeni, V, Olofsson, G, Ottensamer, R, Pagano, I, Pallé, E, Peter, G, Piotto, G, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Rauer, H, Ribas, I, Santos, N C, Scandariato, G, Ségransan, D, Smith, A M S, Steinberger, M, Steller, M, Szabó, Gy M, Thomas, N, Udry, S, Walter, I, Walton, N A, Willett, E

    “…The accuracy of theoretical mass, radius, and effective temperature values for M-dwarf stars is an active topic of debate. Differences between observed and…”
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    Journal Article
  12. 12

    Two warm Neptunes transiting HIP 9618 revealed by TESS and Cheops by Masseron, T, Lillo-Box, J, Pallé, E, Bekkelien, A, Florén, H-G, Guterman, P, Adibekyan, V, Bieryla, A, Borsato, L, Brandeker, A, Ciardi, D R, Collier Cameron, A, Collins, K A, Egger, J A, Gandolfi, D, Hooton, M J, Latham, D W, Lendl, M, Matthews, E C, Ulmer-Moll, S, Vanderburg, A, Wilson, T G, Ziegler, C, Alibert, Y, Anglada, G, Asquier, J, Barrado y Navascues, D, Baumjohann, W, Belinski, A A, Benz, W, Biondi, F, Boisse, I, Bonfils, X, Broeg, C, Bárczy, T, Barros, S C C, Cabrera, J, Cardona Guillen, C, Carleo, I, Charnoz, S, Cortes-Zuleta, P, Davies, M B, Deleuil, M, Delfosse, X, Ehrenreich, D, Erikson, A, Fernandes, R B, Fortier, A, Fridlund, M, Gillon, M, Goliguzova, M V, Gonzales, E J, Günther, M N, Heidari, N, Henze, C E, Hoyer, S, Isaak, K G, Jenkins, J M, Kiefer, F, Kiss, L, Korth, J, Maxted, P F L, Laskar, J, Lecavelier des Etangs, A, Lovis, C, Lund, M B, Luque, R, Magrin, D, Almenara, J M, Martioli, E, Mecina, M, Moldovan, D, Morales-Calderón, M, Morello, G, Jensen, E L N, Olofsson, G, Ottensamer, R, Pagano, I, Peter, G, Piotto, G, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Rauer, H, Ribas, I, Ricker, G, Demangeon, O D S, Smith, A M S, Santos, N, Scandariato, G, Seager, S, Sousa, S G, Szabó, G M, Ségransan, D, Udry, S, Van Grootel, V, Vanderspek, R, Walton, N, Winn, J N

    “…ABSTRACT HIP 9618 (HD 12572, TOI-1471, TIC 306263608) is a bright (G = 9.0 mag) solar analogue. TESS photometry revealed the star to have two candidate planets…”
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  13. 13

    A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067 by Luque, R., Osborn, H. P., Pallé, E., Bonfanti, A., Wilson, T. G., Cameron, A. Collier, Lendl, M., Maxted, P. F. L., Alibert, Y., Gandolfi, D., Egger, J. A., Morales, J. C., Carleo, I., Orell-Miquel, J., Adibekyan, V., Alonso, R., Anderson, D. R., Bandy, T., Bárczy, T., Barrado Navascues, D., Barros, S. C. C., Baumjohann, W., Bean, J. L., Beck, M., Benz, W., Billot, N., Borsato, L., Brandeker, A., Carrazco-Gaxiola, S., Charbonneau, D., Charnoz, S., Ciardi, D. R., Cochran, W. D., Collins, K. A., Crossfield, I. J. M., Csizmadia, Sz, Cubillos, P. E., Davies, M. B., Deeg, H. J., Deline, A., Delrez, L., Demangeon, O. D. S., Demory, B.-O., Ehrenreich, D., Erikson, A., Esparza-Borges, E., Falk, B., Fossati, L., Fridlund, M., Fukui, A., Garcia-Mejia, J., Gillon, M., Goffo, E., Guenther, E. W., Günther, M. N., Hatzes, A. P., Helling, Ch, Howell, S. B., Hoyer, S., Ikuta, K., Jenkins, J. M., Kagetani, T., Kiss, L. L., Korth, J., Lam, K. W. F., Laskar, J., Latham, D. W., Lecavelier des Etangs, A., Leon, J. P. D., Livingston, J. H., Matthews, E. C., Mordasini, C., Narita, N., Nascimbeni, V., Osborne, H. L. M., Ottensamer, R., Pagano, I., Parviainen, H., Quinn, S. N., Quirrenbach, A., Ragazzoni, R., Rando, N., Ratti, F., Rauer, H., Redfield, S., Ricker, G. R., Sabin, L., Salmon, S., Santos, N. C., Scandariato, G., Schlieder, J. E., Seager, S., Shporer, A., Simon, A. E., Stalport, M., Szabó, Gy. M., Van Eylen, V., Van Grootel, V., Watanabe, N., Zingales, T.

    Published in Nature (London) (30-11-2023)
    “…Planets with radii between that of the Earth and Neptune (hereafter referred to as ‘sub-Neptunes’) are found in close-in orbits around more than half of all…”
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    The EBLM project – IX. Five fully convective M-dwarfs, precisely measured with CHEOPS and TESS light curves by Sebastian, D, Swayne, M I, Maxted, P F L, Triaud, A H M J, Sousa, S G, Olofsson, G, Beck, M, Billot, N, Hoyer, S, Gill, S, Heidari, N, Martin, D V, Persson, C M, Standing, M R, Alibert, Y, Alonso, R, Anglada, G, Asquier, J, Bárczy, T, Barrado, D, Barros, S C C, Battley, M P, Baumjohann, W, Beck, T, Benz, W, Bergomi, M, Boisse, I, Bonfils, X, Brandeker, A, Broeg, C, Cabrera, J, Charnoz, S, Collier Cameron, A, Csizmadia, Sz, Davies, M B, Deleuil, M, Delrez, L, Demangeon, O D S, Demory, B-O, Dransfield, G, Ehrenreich, D, Erikson, A, Fortier, A, Fossati, L, Fridlund, M, Gandolfi, D, Gillon, M, Güdel, M, Hasiba, J, Hébrard, G, Heng, K, Isaak, K G, Kiss, L L, Kopp, E, Kunovac, V, Laskar, J, Lecavelier des Etangs, A, Lendl, M, Lovis, C, Magrin, D, McCormac, J, Miller, N J, Nascimbeni, V, Ottensamer, R, Pagano, I, Pallé, E, Pepe, F A, Peter, G, Piotto, G, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Rauer, H, Ribas, I, Lalitha, S, Santerne, A, Santos, N C, Scandariato, G, Ségransan, D, Simon, A E, Smith, A M S, Steller, M, Szabó, Gy M, Thomas, N, Udry, S, Van Grootel, V, Walton, N A

    “…ABSTRACT Eclipsing binaries are important benchmark objects to test and calibrate stellar structure and evolution models. This is especially true for binaries…”
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  16. 16

    Disinfection of surfaces by photocatalytic oxidation with titanium dioxide and UVA light by Kühn, Klaus P., Chaberny, Iris F., Massholder, Karl, Stickler, Manfred, Benz, Volker W., Sonntag, Hans-Günther, Erdinger, Lothar

    Published in Chemosphere (Oxford) (01-10-2003)
    “…Particularly in microbiological laboratories and areas in intensive medical use, regular and thorough disinfection of surfaces is required in order to reduce…”
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    CHEOPS Performance for Exomoons: The Detectability of Exomoons by Using Optimal Decision Algorithm by Simon, A. E., Szabó, Gy. M., Kiss, L. L., Fortier, A., Benz, W.

    “…Many attempts have already been made to detect exomoons around transiting exoplanets, but the first confirmed discovery is still pending. The experiences that…”
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    The EBLM Project– XI. Mass, radius, and effective temperature measurements for 23 M-dwarf companions to solar-type stars observed with CHEOPS by Swayne, M I, Maxted, P F L, Triaud, A H M J, Sousa, S G, Deline, A, Ehrenreich, D, Hoyer, S, Olofsson, G, Boisse, I, Duck, A, Gill, S, Martin, D, McCormac, J, Persson, C M, Sebastian, D, Standing, M R, Acuña, L, Alibert, Y, Alonso, R, Anglada, G, Bárczy, T, Barrado Navascues, D, Barros, S C C, Baumjohann, W, Baycroft, T A, Beck, M, Beck, T, Benz, W, Billot, N, Bonfils, X, Borsato, L, Bourrier, V, Brandeker, A, Broeg, C, Carmona, A, Charnoz, S, Collier Cameron, A, Cortés-Zuleta, P, Csizmadia, Sz, Cubillos, P E, Davies, M B, Deleuil, M, Delrez, L, Demangeon, O D S, Demory, B -O, Dransfield, G, Erikson, A, Fortier, A, Forveille, T, Fossati, L, Fridlund, M, Gandolfi, D, Gillon, M, Günther, M N, Hara, N, Hébrard, G, Heidari, N, Hellier, C, Helling, Ch, Isaak, K G, Kiefer, F, Kiss, L L, Kunovac, V, Lam, K W F, Laskar, J, Lecavelier des Etangs, A, Lendl, M, Magrin, D, Marafatto, L, Martioli, E, Miller, N J, Mordasini, C, Moutou, C, Nascimbeni, V, Ottensamer, R, Pagano, I, Pallé, E, Peter, G, Piotto, G, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Rauer, H, Ribas, I, Santos, N C, Scandariato, G, Ségransan, D, Smith, A M S, Southworth, R, Stalport, M, Szabó, Gy M, Thomas, N, Udry, S, Ulmer, B, Van Grootel, V, Venturini, J, Walton, N A, Willett, E, Wilson, T G

    “…ABSTRACT Observations of low-mass stars have frequently shown a disagreement between observed stellar radii and radii predicted by theoretical stellar…”
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