Zobrazeno 1 - 10
of 107
pro vyhledávání: '"Bachschmidt, A."'
Autor:
Kokori, A., Tsiaras, A., Edwards, B., Jones, A., Pantelidou, G., Tinetti, G., Bewersdorff, L., Iliadou, A., Jongen, Y., Lekkas, G., Nastasi, A., Poultourtzidis, E., Sidiropoulos, C., Walter, F., Wünsche, A., Abraham, R., Agnihotri, V. K., Albanesi, R., Arce-Mansego, E., Arnot, D., Audejean, M., Aumasson, C., Bachschmidt, M., Baj, G., Barroy, P. R., Belinski, A. A., Bennett, D., Benni, P., Bernacki, K., Betti, L., Biagini, A., Bosch, P., Brandebourg, P., Brát, L., Bretton, M., Brincat, S. M., Brouillard, S., Bruzas, A., Bruzzone, A., Buckland, R. A., Caló, M., Campos, F., Carreno, A., Rodrigo, J. -A. Carrion, Casali, R., Casalnuovo, G., Cataneo, M., Chang, C. -M., Changeat, L., Chowdhury, V., Ciantini, R., Cilluffo, M., Coliac, J. -F., Conzo, G., Correa, M., Coulon, G., Crouzet, N., Crow, M. V., Curtis, I., Daniel, D., Dawes, S., Dauchet, B., Deldem, M., Deligeorgopoulos, D., Dransfield, G., Dymock, R., Eenmäe, T., Evans, P., Esseiva, N., Falco, C., Farfán, R. G., Fernández-Lajús, E., Ferratfiat, S., Ferreira, S. L., Ferretti, A., Fiołka, J., Fowler, M., Futcher, S. R., Gabellini, D., Gainey, T., Gaitan, J., Gajdoš, P., García-Sánchez, A., Garlitz, J., Gillier, C., Gison, C., Horta, F. Grau, Grivas, G., Gonzales, J., Gorshanov, D., Guerra, P., Guillot, T., Haswell, C. A., Haymes, T., Hentunen, V. -P., Hills, K., Hose, K., Humbert, T., Hurter, F., Hynek, T., Irzyk, M., Jacobsen, J., Jannetta, A. L., Johnson, K., Jóźwik-Wabik, P., Kaeouach, A. E., Kang, W., Kiiskinen, H., Kim, T., Kivila, Ü., Koch, B., Kolb, U., Kučáková, H., Lai, S. -P., Laloum, D., Lasota, S., Lewis, L. A., Liakos, G. -I., Libotte, F., Lopresti, C., Lomoz, F., Majewski, R., Malcher, A., Mallonn, M., Mannucci, M., Marchini, A., Mari, J. -M., Marino, A., Marino, G., Mario, J. -C., Marquette, J. -B., Martínez-Bravo, F. A., Mašek, M., Matassa, P., Michel, P., Michelet, J., Miller, M., Miny, E., Mollier, T., Molina, D., Monteleone, B., Montigiani, N., Morales-Aimar, M., Mortari, F., Morvan, M., Mugnai, L. V., Murawski, G., Naponiello, L., Naves, R., Naudin, J. -L., Néel, D., Neito, R., Neveu, S., Noschese, A., Öğmen, Y., Ohshima, O., Orbanic, Z., Pace, E. P., Pantacchini, C., Paschalis, N. I., Pereira, C., Peretto, I., Perroud, V., Phillips, M., Pintr, P., Pioppa, J. -B., Plazas, J., Poelarends, A. J., Popowicz, A., Purcell, J., Quinn, N., Raetz, M., Rees, D., Regembal, F., Rocchetto, M., Rocci, P. -F., Rockenbauer, M., Roth, R., Rousselot, L., Rubia, X., Ruocco, N., Russo, E., Salisbury, M., Salvaggio, F., Santos, A., Savage, J., Scaggiante, F., Sedita, D., Shadick, S., Silva, A. F., Sioulas, N., Školník, V., Smith, M., Smolka, M., Solmaz, A., Stanbury, N., Stouraitis, D., Tan, T. -G., Theusner, M., Thurston, G., Tifner, F. -P., Tomacelli, A., Tomatis, A., Trnka, J., Tylšar, M., Valeau, P., Vignes, J. -P., Villa, A., Sureda, A. Vives, Vora, K., Vrašťák, M., Walliang, D., Wenzel, B., Wright, D. E., Zambelli, R., Zhang, M., Zíbar, M.
The ExoClock project has been created with the aim of increasing the efficiency of the Ariel mission. It will achieve this by continuously monitoring and updating the ephemerides of Ariel candidates over an extended period, in order to produce a cons
Externí odkaz:
http://arxiv.org/abs/2209.09673
Autor:
Kokori, A., Tsiaras, A., Edwards, B., Rocchetto, M., Tinetti, G., Bewersdorff, L., Jongen, Y., Lekkas, G., Pantelidou, G., Poultourtzidis, E., Wünsche, A., Aggelis, C., Agnihotri, V. K., Arena, C., Bachschmidt, M., Bennett, D., Benni, P., Bernacki, K., Besson, E., Betti, L., Biagini, A., Brandebourg, P., Bretton, M., Brincat, S. M., Caló, M., Campos, F., Casali, R., Ciantini, R., Crow, M. V., Dauchet, B., Dawes, S., Deldem, M., Deligeorgopoulos, D., Dymock, R., Eenmäe, T., Evans, P., Esseiva, N., Falco, C., Ferratfiat, S., Fowler, M., Futcher, S. R., Gaitan, J., Horta, F. Grau, Guerra, P., Hurter, F., Jones, A., Kang, W., Kiiskinen, H., Kim, T., Laloum, D., Lee, R., Lomoz, F., Lopresti, C., Mallonn, M., Mannucci, M., Marino, A., Mario, J. -C., Marquette, J. -B., Michelet, J., Miller, M., Mollier, T., Molina, D., Montigiani, N., Mortari, F., Morvan, M., Mugnai, L. V., Naponiello, L., Nastasi, A., Neito, R., Pace, E., Papadeas, P., Paschalis, N., Pereira, C., Perroud, V., Phillips, M., Pintr, P., Pioppa, J. -B., Popowicz, A., Raetz, M., Regembal, F., Rickard, K., Roberts, M., Rousselot, L., Rubia, X., Savage, J., Sedita, D., Shave-Wall, D., Sioulas, N., Školník, V., Smith, M., St-Gelais, D., Stouraitis, D., Strikis, I., Thurston, G., Tomacelli, A., Tomatis, A., Trevan, B., Valeau, P., Vignes, J. -P., Vora, K., Vrašťák, M., Walter, F., Wenzel, B., Wright, D. E., Zíbar, M.
The ExoClock project is an inclusive, integrated, and interactive platform that was developed to monitor the ephemerides of the Ariel targets to increase the mission efficiency. The project makes the best use of all available resources, i.e., observa
Externí odkaz:
http://arxiv.org/abs/2110.13863
Autor:
Kokori, Anastasia, Tsiaras, Angelos, Edwards, Billy, Rocchetto, Marco, Tinetti, Giovanna, Wünsche, Anaël, Paschalis, Nikolaos, Agnihotri, Vikrant Kumar, Bachschmidt, Matthieu, Bretton, Marc, Caines, Hamish, Caló, Mauro, Casali, Roland, Crow, Martin, Dawes, Simon, Deldem, Marc, Deligeorgopoulos, Dimitrios, Dymock, Roger, Evans, Phil, Falco, Carmelo, Ferratfiat, Stephane, Fowler, Martin, Futcher, Stephen, Guerra, Pere, Hurter, Francois, Jones, Adrian, Kang, Wonseok, Kim, Taewoo, Lee, Richard, Lopresti, Claudio, Marino, Antonio, Mallonn, Matthias, Mortari, Fabio, Morvan, Mario, Mugnai, Lorenzo V., Nastasi, Alessandro, Perroud, Valère, Pereira, Cédric, Phillips, Mark, Pintr, Pavel, Raetz, Manfred, Regembal, Francois, Savage, John, Sedita, Danilo, Sioulas, Nick, Strikis, Iakovos, Thurston, Geoffrey, Tomacelli, Andrea, Tomatis, Alberto
The Ariel mission will observe spectroscopically around 1000 exoplanets to further characterise their atmospheres. For the mission to be as efficient as possible, a good knowledge of the planets' ephemerides is needed before its launch in 2028. While
Externí odkaz:
http://arxiv.org/abs/2012.07478
Autor:
Edwards, Billy, Changeat, Quentin, Yip, Kai Hou, Tsiaras, Angelos, Taylor, Jake, Akhtar, Bilal, AlDaghir, Josef, Bhattarai, Pranup, Bhudia, Tushar, Chapagai, Aashish, Huang, Michael, Kabir, Danyaal, Khag, Vieran, Khaliq, Summyyah, Khatri, Kush, Kneth, Jaidev, Kothari, Manisha, Najmudin, Ibrahim, Panchalingam, Lobanaa, Patel, Manthan, Premachandran, Luxshan, Qayyum, Adam, Rana, Prasen, Shaikh, Zain, Syed, Sheryar, Theti, Harnam, Zaidani, Mahmoud, Saraf, Manasvee, de Mijolla, Damien, Caines, Hamish, Kokori, Anatasia, Rocchetto, Marco, Mallonn, Matthias, Bachschmidt, Matthieu, Bosch, Josep M., Bretton, Marc, Chatelain, Philippe, Deldem, Marc, Di Sisto, Romina, Evans, Phil, Fernandez-Lajus, Eduardo, Guerra, Pere, Horta, Ferran Grau, Kang, Wonseok, Kim, Taewoo, Leroy, Arnaud, Lomoz, Frantivsek, de Haro, Juan Lozano, Hentunen, Veli-Pekka, Jongen, Yves, Molina, David, Montaigut, Romain, Naves, Ramon, Raetz, Manfred, Sauer, Thomas, Watkins, Americo, Wunsche, Anael, Zibar, Martin, Dunn, William, Tessenyi, Marcell, Savini, Giorgio, Tinetti, Giovanna, Tennyson, Jonathan
We report follow-up observations of transiting exoplanets that have either large uncertainties (>10 minutes) in their transit times or have not been observed for over three years. A fully robotic ground-based telescope network, observations from citi
Externí odkaz:
http://arxiv.org/abs/2005.01684
Publikováno v:
In Annales médico-psychologiques April 2022 180(4):301-306
Autor:
Hanuš, J., Delbo', M., Alí-Lagoa, V., Bolin, B., Jedicke, R., Ďurech, J., Cibulková, H., Pravec, P., Kušnirák, P., Behrend, R., Marchis, F., Antonini, P., Arnold, L., Audejean, M., Bachschmidt, M., Bernasconi, L., Brunetto, L., Casulli, S., Dymock, R., Esseiva, N., Esteban, M., Gerteis, O., de Groot, H., Gully, H., Hamanowa, H., Krafft, P., Lehký, M., Manzini, F., Michelet, J., Morelle, E., Oey, J., Pilcher, F., Reignier, F., Roy, R., Salom, P. A., Warner, B. D.
Eos family was created during a catastrophic impact about 1.3 Gyr ago. Rotation states of individual family members contain information about the history of the whole population. We aim to increase the number of asteroid shape models and rotation sta
Externí odkaz:
http://arxiv.org/abs/1707.05507
Autor:
Santerne, A., Hébrard, G., Lillo-Box, J., Armstrong, D. J., Barros, S. C. C., Demangeon, O., Barrado, D., Debackere, A., Deleuil, M., Mena, E. Delgado, Montalto, M., Pollacco, D., Osborn, H. P., Sousa, S. G., Abe, L., Adibekyan, V., Almenara, J. -M., André, P., Arlic, G., Barthe, G., Bendjoya, P., Behrend, R., Boisse, I., Bouchy, F., Boussier, H., Bretton, M., Brown, D. J. A., Carry, B., Cailleau, A., Conseil, E., Courcol, B., Dauchet, B., Dalouzy, J. -C., Deldem, M., Dubreuil, P., Fehrenbach, J. -M., Ferratfiat, S., Girelli, R., Gregorio, J., Jaecques, S., Kugel, F., Kirk, J., Labrevoir, O., Lachurié, J. -C., Lam, K. W. F., Guen, P. Le, Martinez, P., Maurin, L., McCormac, J., Pioppa, J-B., Quadri, U., Rajpurohit, A., Rey, J., Rivet, J. -P., Roy, R., Santos, N. C., Signoret, F., Strabla, L., Suarez, O., Toublanc, D., Tsantaki, M., Wilson, P. A., Bachschmidt, M., Colas, F., Gerteis, O., Louis, P., Mario, J. -C., Marlot, C., Montier, J., Perroud, V., Pic, V., Romeuf, D., Ubaud, S., Verilhac, D.
Publikováno v:
2016, ApJ, 825, 55
In the present paper we report the discovery of a new hot Jupiter, EPIC211089792 b, first detected by the Super-WASP observatory and then by the K2 space mission during its campaign 4. The planet has a period of 3.25d, a mass of 0.73 +/- 0.04 Mjup, a
Externí odkaz:
http://arxiv.org/abs/1601.07680
Autor:
Hanuš, J., Ďurech, J., Oszkiewicz, D. A., Behrend, R., Carry, B., Delbo', M., Adam, O., Afonina, V., Anquetin, R., Antonini, P., Arnold, L., Audejean, M., Aurard, P., Bachschmidt, M., Badue, B., Barbotin, E., Barroy, P., Baudouin, P., Berard, L., Berger, N., Bernasconi, L., Bosch, J-G., Bouley, S., Bozhinova, I., Brinsfield, J., Brunetto, L., Canaud, G., Caron, J., Carrier, F., Casalnuovo, G., Casulli, S., Cerda, M., Chalamet, L., Charbonnel, S., Chinaglia, B., Cikota, A., Colas, F., Coliac, J-F., Collet, A., Coloma, J., Conjat, M., Conseil, E., Costa, R., Crippa, R., Cristofanelli, M., Damerdji, Y., Debackere, A., Decock, A., Déhais, Q., Déléage, T., Delmelle, S., Demeautis, C., Dróżdż, M., Dubos, G., Dulcamara, T., Dumont, M., Durkee, R., Dymock, R., del Valle, A. Escalante, Esseiva, N., Esseiva, R., Esteban, M., Fauchez, T., Fauerbach, M., Fauvaud, M., Fauvaud, S., Forné, E., Fournel, C., Fradet, D., Garlitz, J., Gerteis, O., Gillier, C., Gillon, M., Giraud, R., Godard, J-P., Goncalves, R., Hamanowa, H., Hay, K., Hellmich, S., Heterier, S., Higgins, D., Hirsch, R., Hodosan, G., Hren, M., Hygate, A., Innocent, N., Jacquinot, H., Jawahar, S., Jehin, E., Jerosimic, L., Klotz, A., Koff, W., Korlevic, P., Kosturkiewicz, E., Krafft, P., Krugly, Y., Kugel, F., Labrevoir, O., Lecacheux, J., Lehký, M., Leroy, A., Lesquerbault, B., Lopez-Gonzales, M. J., Lutz, M., Mallecot, B., Manfroid, J., Manzini, F., Marciniak, A., Martin, A., Modave, B., Montaigut, R., Montier, J., Morelle, E., Morton, B., Mottola, S., Naves, R., Nomen, J., Oey, J., Ogłoza, W., Paiella, M., Pallares, H., Peyrot, A., Pilcher, F., Pirenne, J-F., Piron, P., Polinska, M., Polotto, M., Poncy, R., Previt, J. P., Reignier, F., Renauld, D., Ricci, D., Richard, F., Rinner, C., Risoldi, V., Robilliard, D., Romeuf, D., Rousseau, G., Roy, R., Ruthroff, J., Salom, P. A., Salvador, L., Sanchez, S., Santana-Ros, T., Scholz, A., Séné, G., Skiff, B., Sobkowiak, K., Sogorb, P., Soldán, F., Spiridakis, A., Splanska, E., Sposetti, S., Starkey, D., Stephens, R., Stiepen, A., Stoss, R., Strajnic, J., Teng, J-P., Tumolo, G., Vagnozzi, A., Vanoutryve, B., Vugnon, J. M., Warner, B. D., Waucomont, M., Wertz, O., Winiarski, M., Wolf, M.
Publikováno v:
A&A 586, A108 (2016)
Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almost 400 convex shape models and their rotation states. This amount already provided a deep insight into physical properties of main-belt asteroids or large collisi
Externí odkaz:
http://arxiv.org/abs/1510.07422
Autor:
A. Kokori, A. Tsiaras, B. Edwards, A. Jones, G. Pantelidou, G. Tinetti, L. Bewersdorff, A. Iliadou, Y. Jongen, G. Lekkas, A. Nastasi, E. Poultourtzidis, C. Sidiropoulos, F. Walter, A. Wünsche, R. Abraham, V. K. Agnihotri, R. Albanesi, E. Arce-Mansego, D. Arnot, M. Audejean, C. Aumasson, M. Bachschmidt, G. Baj, P. R. Barroy, A. A. Belinski, D. Bennett, P. Benni, K. Bernacki, L. Betti, A. Biagini, P. Bosch, P. Brandebourg, L. Brát, M. Bretton, S. M. Brincat, S. Brouillard, A. Bruzas, A. Bruzzone, R. A. Buckland, M. Caló, F. Campos, A. Carreño, J. A. Carrion Rodrigo, R. Casali, G. Casalnuovo, M. Cataneo, C.-M. Chang, L. Changeat, V. Chowdhury, R. Ciantini, M. Cilluffo, J.-F. Coliac, G. Conzo, M. Correa, G. Coulon, N. Crouzet, M. V. Crow, I. A. Curtis, D. Daniel, B. Dauchet, S. Dawes, M. Deldem, D. Deligeorgopoulos, G. Dransfield, R. Dymock, T. Eenmäe, N. Esseiva, P. Evans, C. Falco, R. G. Farfán, E. Fernández-Lajús, S. Ferratfiat, S. L. Ferreira, A. Ferretti, J. Fiołka, M. Fowler, S. R. Futcher, D. Gabellini, T. Gainey, J. Gaitan, P. Gajdoš, A. García-Sánchez, J. Garlitz, C. Gillier, C. Gison, J. Gonzales, D. Gorshanov, F. Grau Horta, G. Grivas, P. Guerra, T. Guillot, C. A. Haswell, T. Haymes, V.-P. Hentunen, K. Hills, K. Hose, T. Humbert, F. Hurter, T. Hynek, M. Irzyk, J. Jacobsen, A. L. Jannetta, K. Johnson, P. Jóźwik-Wabik, A. E. Kaeouach, W. Kang, H. Kiiskinen, T. Kim, Ü. Kivila, B. Koch, U. Kolb, H. Kučáková, S.-P. Lai, D. Laloum, S. Lasota, L. A. Lewis, G.-I. Liakos, F. Libotte, F. Lomoz, C. Lopresti, R. Majewski, A. Malcher, M. Mallonn, M. Mannucci, A. Marchini, J.-M. Mari, A. Marino, G. Marino, J.-C. Mario, J.-B. Marquette, F. A. Martínez-Bravo, M. Mašek, P. Matassa, P. Michel, J. Michelet, M. Miller, E. Miny, D. Molina, T. Mollier, B. Monteleone, N. Montigiani, M. Morales-Aimar, F. Mortari, M. Morvan, L. V. Mugnai, G. Murawski, L. Naponiello, J.-L. Naudin, R. Naves, D. Néel, R. Neito, S. Neveu, A. Noschese, Y. Öğmen, O. Ohshima, Z. Orbanic, E. P. Pace, C. Pantacchini, N. I. Paschalis, C. Pereira, I. Peretto, V. Perroud, M. Phillips, P. Pintr, J.-B. Pioppa, J. Plazas, A. J. Poelarends, A. Popowicz, J. Purcell, N. Quinn, M. Raetz, D. Rees, F. Regembal, M. Rocchetto, P.-F. Rocci, M. Rockenbauer, R. Roth, L. Rousselot, X. Rubia, N. Ruocco, E. Russo, M. Salisbury, F. Salvaggio, A. Santos, J. Savage, F. Scaggiante, D. Sedita, S. Shadick, A. F. Silva, N. Sioulas, V. Školník, M. Smith, M. Smolka, A. Solmaz, N. Stanbury, D. Stouraitis, T.-G. Tan, M. Theusner, G. Thurston, F. P. Tifner, A. Tomacelli, A. Tomatis, J. Trnka, M. Tylšar, P. Valeau, J.-P. Vignes, A. Villa, A. Vives Sureda, K. Vora, M. Vrašt’ák, D. Walliang, B. Wenzel, D. E. Wright, R. Zambelli, M. Zhang, M. Zíbar
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 265, Iss 1, p 4 (2023)
The ExoClock project has been created to increase the efficiency of the Ariel mission. It will achieve this by continuously monitoring and updating the ephemerides of Ariel candidates, in order to produce a consistent catalog of reliable and precise
Externí odkaz:
https://doaj.org/article/82020958eddb4304949cd6fc6e4a1e0d
Autor:
Keren, Amit, Shafir, Oren, Shimshoni, Efrat, Marvaud, Valerie, Bachschmidt, Anne, Long, Jerome
Publikováno v:
Phys. Rev. Lett. 98, 257204 (2007)
Muon spin relaxation measurements in isotropic molecular magnets (MM) with a spin value S ranging from 7/2 to 27/2 are used to determine the magnitude and origin of dephasing time $\tau_\phi$ of molecular magnets. It is found that $\tau_\phi$ ~ 10 ns
Externí odkaz:
http://arxiv.org/abs/0706.3506