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2. Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy

Author

Mousis, O., Hueso, R., Beaulieu, J. -P., Bouley, S., Carry, B., Colas, F., Klotz, A., Pellier, C., Petit, J. -M., Rousselot, P., Dib, M. Ali, Beisker, W., Birlan, M., Buil, C., Delsanti, A., Frappa, E., Hammel, H. B., Levasseur-Regourd, A. -C., Orton, G. S., Sanchez-Lavega, A., Santerne, A., Tanga, P., Vaubaillon, J., Zanda, B., Baratoux, D., Boehm, T., Boudon, V., Bouquet, A., Buzzi, L., Dauvergne, J. -L., Decock, A., Delcroix, M., Drossart, P., Esseiva, N., Fischer, G., Fletcher, L. N., Foglia, S., Gomez-Forrellad, J. M., Guarro-Flo, J., Herald, D., Jehin, E., Kugel, F., Lebreton, J. -P., Lecacheux, J., Leroy, A., Maquet, L., Masi, G., Maury, A., Meyer, F., Pérez-Hoyos, S., Rajpurohit, A. S., Rinner, C., Rogers, J. H., Roques, F., Schmude, Jr., R. W., Sicardy, B., Tregon, B., Vanhuysse, M., Wesley, A., and Widemann, T.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics
Abstract

Amateur contributions to professional publications have increased exponentially over the last decades in the field of Planetary Astronomy. Here we review the different domains of the field in which collaborations between professional and amateur astronomers are effective and regularly lead to scientific publications. We discuss the instruments, detectors, softwares and methodologies typically used by amateur astronomers to collect the scientific data in the different domains of interest. Amateur contributions to the monitoring of planets and interplanetary matter, characterization of asteroids and comets, as well as the determination of the physical properties of Kuiper Belt Objects and exoplanets are discussed., Comment: 123 pages, Accepted for publication in Experimental Astronomy

Published
2013
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6. Instrumental methods for professional and amateur collaborations in planetary astronomy

Author

Mousis, O., Hueso, R., Beaulieu, J.-P., Bouley, S., Carry, B., Colas, F., Klotz, A., Pellier, C., Petit, J.-M., Rousselot, P., Ali-Dib, M., Beisker, W., Birlan, M., Buil, C., Delsanti, A., Frappa, E., Hammel, H. B., Levasseur-Regourd, A. C., Orton, G. S., Sánchez-Lavega, A., Santerne, A., Tanga, P., Vaubaillon, J., Zanda, B., Baratoux, D., Böhm, T., Boudon, V., Bouquet, A., Buzzi, L., Dauvergne, J. -L., Decock, A., Delcroix, M., Drossart, P., Esseiva, N., Fischer, G., Fletcher, L. N., Foglia, S., M. Gómez-Forrellad, J., Guarro-Fló, J., Herald, D., Jehin, E., Kugel, F., Lebreton, J. -P., Lecacheux, J., Leroy, A., Maquet, L., Masi, G., Maury, A., Meyer, F., Pérez-Hoyos, S., Rajpurohit, A. S., Rinner, C., Rogers, J. H., Roques, F., Schmude, Jr., R.W., Sicardy, B., Tregon, B., Vanhuysse, M., Wesley, A., and Widemann, T.

Published
2014
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8. Tumbling asteroids

Author

Pravec, P., Harris, A.W., Scheirich, P., Kusnirak, P., Sarounova L., Hergenrother, C.W., Mottola, S., Hicks, M.D., Masi, G., Krugly Yu.N., Shevchenko, V.G., Nolan, M.C., Howel, E.S., Kaasalainen, M., Galad, A., Brown, P., DeGraff, D.R., Lambert, J.V., Cooney, W.R., Jr., and Foglia, S.

Subjects
Asteroids -- Observations, Asteroids -- Properties, Astronomy, Earth sciences
Abstract

We present both a review of earlier data and new results on non-principal axis rotators (tumblers) among asteroids. Among new tumblers found, the best data we have are for 2002 T[D.sub.60], 2000 W[L.sub.107], and (54789) 2001 M[Z.sub.7]--each of them shows a lightcurve with two frequencies (full terms with linear combinations of the two frequencies are present in the lightcurve). For 2002 TD60, we have constructed a physical model of the NPA rotation. Other recent objects which have been found to be likely tumblers based on their lightcurves that do not fit with a single periodicity are 2002 N[Y.sub.40], (16067) 1999 R[H.sub.27], and (5645) 1990 SP. We have done a statistical analysis of the present sample of the population of NPA rotators. It appears that most asteroids larger than ~ 0.4 km with estimated damping timescales (Harris, 1994, Icarus 107, 209) of 4.5 byr and longer are NPA rotators. The statistic of two short-period tumblers (D = 0.04 and 0.4 km) with non-zero tensile strength suggests that for them the quantity [micro] Q/T, where [micro] is the mechanical rigidity, Q is the elastic dissipation factor, and T is a spin excitation age (i.e., a time elapsed since the last significant spin excitation event), is greater by two to four orders of magnitude than the larger, likely rubble-pile tumblers. Among observational conditions and selection effects affecting detections of NPA rotations, there is a bias against detection of low-amplitude (small elongation) tumblers. Keywords: Asteroids; Excited rotation; Photometry

Published
2005

10. Unconventional magnetic behavior of iron-oxide nanoparticles in polymeric matrices

Author

Testa, A.M., Foglia, S., Suber, L., Fiorani, D., Casas, Ll., Roig, A., Molins, E., Greneche, J.M., and Tejada, J.

Subjects
Magnetic materials -- Research, Nanotechnology -- Research, Physics
Abstract

Research into the magnetic properties of composite iron-oxide nanoparticles contained in matrices based on commercial ion-exchange type polystyrene is presented. This work supported the existence of a fraction of particles capable of rotating freely in response to an applied field.

Published
2001

14. The PHEMU15 catalogue and astrometric results of the Jupiter's Galilean satellite mutual occultation and eclipse observations made in 2014-2015

Author

Saquet, E. Emelyanov, N. Robert, V. Arlot, J.-E. Anbazhagan, P. Baillié, K. Bardecker, J. Berezhnoy, A.A. Bretton, M. Campos, F. Capannoli, L. Carry, B. Castet, M. Charbonnier, Y. Chernikov, M.M. Christou, A. Colas, F. Coliac, J.-F. Dangl, G. Dechambre, O. Delcroix, M. Dias-Oliveira, A. Drillaud, C. Duchemin, Y. Dunford, R. Dupouy, P. Ellington, C. Fabre, P. Filippov, V.A. Finnegan, J. Foglia, S. Font, D. Gaillard, B. Galli, G. Garlitz, J. Gasmi, A. Gaspar, H.S. Gault, D. Gazeas, K. George, T. Gorda, S.Y. Gorshanov, D.L. Gualdoni, C. Guhl, K. Halir, K. Hanna, W. Henry, X. Herald, D. Houdin, G. Ito, Y. Izmailov, I.S. Jacobsen, J. Jones, A. Kamoun, S. Kardasis, E. Karimov, A.M. Khovritchev, M.Y. Kulikova, A.M. Laborde, J. Lainey, V. Lavayssiere, M. Le Guen, P. Leroy, A. Loader, B. Lopez, O.C. Lyashenko, A.Y. Lyssenko, P.G. Machado, D.I. Maigurova, N. Manek, J. Marchini, A. Midavaine, T. Montier, J. Morgado, B.E. Naumov, K.N. Nedelcu, A. Newman, J. Ohlert, J.M. Oksanen, A. Pavlov, H. Petrescu, E. Pomazan, A. Popescu, M. Pratt, A. Raskhozhev, V.N. Resch, J.-M. Robilliard, D. Roschina, E. Rothenberg, E. Rottenborn, M. Rusov, S.A. Saby, F. Saya, L.F. Selvakumar, G. Signoret, F. Slesarenko, V.Y. Sokov, E.N. Soldateschi, J. Sonka, A. Soulie, G. Talbot, J. Tejfel, V.G. Thuillot, W. Timerson, B. Toma, R. Torsellini, S. Trabuco, L.L. Traverse, P. Tsamis, V. Unwin, M. Van Den Abbeel, F. Vandenbruaene, H. Vasundhara, R. Velikodsky, Y.I. Vienne, A. Vilar, J. Vugnon, J.-M. Wuensche, N. Zeleny, P.

Subjects
Physics::Space Physics, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics
Abstract

During the 2014-2015 mutual events season, the Institut de Mécanique Céleste et de Calcul des Éphémérides (IMCCE), Paris, France, and the Sternberg Astronomical Institute (SAI), Moscow, Russia, led an international observation campaign to record ground-based photometric observations of Galilean moon mutual occultations and eclipses.We focused on processing the complete photometric observations data base to compute new accurate astrometric positions. We used our method to derive astrometric positions from the light curves of the events. We developed an accurate photometric model of mutual occultations and eclipses, while correcting for the satellite albedos, Hapke's light scattering law, the phase effect, and the limb darkening. We processed 609 light curves, and we compared the observed positions of the satellites with the theoretical positions from IMCCE NOE-5-2010-GAL satellite ephemerides and INPOP13c planetary ephemeris. The standard deviation after fitting the light curve in equatorial positions is ±24 mas, or 75 km at Jupiter. The rms (O-C) in equatorial positions is ±50 mas, or 150 km at Jupiter. © 2017 The Author(s).

Published
2018

15. Observations and Orbits of Comets

Author

Kulichenko, N., Pomazan, A. V., Maigurova, N. V., Bodryagin, D. V., Bacci, P., Maestripieri, M., Tesi, L., Fagioli, G., Bonomi, R., Facchini, M., Coffano, A., Marinello, W., Micheli, M., Pizzetti, G., Soffiantini, A., Cernis, K., Haver, R., Gorelli, R., Piazzolla, L. M., Jaeger, M., Prosperi, E., Prosperi, S., Vollmann, W., Wiebe, Y., Kaiser, G., Puccini, S., Buriev, A. M., Ibrohimov, A. A., Safarov, A. G., Ayubov, D. K., Asoev, H. G., Foglia, S., Galli, G., Naves, R., Campas, M., Hasubick, W., Scotti, J. V., Altieri, B., Bouy, H., Verdoes-Kleijn, G., Carry, B., Kadota, K., Abe, H., Seki, T., Sato, H., Rodríguez, D., Ionescu, D., Christie, G. W., Natusch, T., Gilmore, A. C., Kilmartin, P. M., Meech, K. J., Kleyna, J., Woodworth, D., Kashuba, V., Troianskyi, V., Kashuba, S., Baransky, A., Tochonyy, V., Gunko, N., Pogrebtsov, N., Radomskiy, V., Ruban, E., Pavluk, Y., Kurginian, E., Ershov, D., Zadorozhny, O., Kasyanchuk, A., Bakaieva, O., Shevchuk, D., Bondar, D., Pais, T., Smolynec, V., Balam, D. D., Tubbiolo, A. F., Leonard, G. J., Matheny, R. G., Kowalski, R. A., Fuls, D. C., Johnson, J. A., Christensen, E. J., Gibbs, A. R., Grauer, A. D., Larson, S. M., Seaman, R. L., Shelly, F. C., Moritz, N., Childs, W., Ikari, Y., Masi, G., Schwartz, M., Holvorcem, P., Dupouy, P., de Vanssay, J. B., James, N., Soulier, J.-F., Aymami, J. M., Camarasa, J., Linder, J., Montoro, L., Bosch, J. M., Bryssinck, E., Diepvens, A., Shurpakov, S., Gao, X. Liao X., Liao, X., Lindner, P., Dangl, G., Mainzer, A. K., Bauer, J. M., Grav, T., Masiero, J. R., Dailey, J. W., Cutri, R. M., Wright, E. L., Nugent, C., Sonnett, S., Kramer, E., Gaitan, J., Tremosa, L., Zhao, H. B., Li, B., Zhaori, G., Hong, R. Q., Hu, L. F., Lu, H., Tan, H. J., Ohshima, Y., Barona Felgosa, L., Belli, L., Bilhaj, M., Bosse, M., Schmidt, M., Breitenstein, P., Mccormick, J., Carstens, R., Drummond, J., Bulger, J., Goggia, T., Lowe, T., Schultz, A., Willman, M., Chambers, K., Chastel, S., Denneau, L., Flewelling, H., Huber, M., Lilly, E., Magnier, E., Wainscoat, R., Waters, C., Weryk, R., Pei, W., Hambsch, F.-J., Hambsch, J., Lutkenhoner, B., Paul, N., Gasparovic, G., Chen, Y., Cox, P., Betzler, A. S., Sherrod, P. C., Sherrod, L. P., Bell, C., Peterson, H., Chapman, A., Sparrenberger, M., Gonzalez, J., Hills, K., Benavides, R., Carson, P., Morales, M., Gerhard, C., Fichtl, R., Haeusler, B., Ditz, P., Hudin, L., Sugawara, K., Nohara, H., Buzzi, L., Concari, P., Cremaschini, C., Tombelli, M., Tilley, S. M., van Buitenen, G., Dymock, R., Camilleri, P., Williams, H., Heinze, A., Weiland, H., Stalder, B., Tonry, J., Sherstyuk, A., Rowe, B., Wilde, D., Flynn, R. L., Allen, L., Trilling, D., James, D., Herrera, D., Fuentes, C., Rajagopal, J., Axelrod, T., Valdes, F., Lipunov, V., Podesta, R., Gorbovskoy, E., Tiurina, N., Balanutsa, P., Kuznetsov, A., Kornilov, V., Chazov, V., Lopez, C., Podesta, F., Levato, H., Saffe, C., Maury, A., Vanssay, J. B., Noël, T., Sandness, B., Maur, A., Jacques, C., Pimentel, E., Barros, J., Acosta, A., Sofia, A., Silvia, A., Jackson, F., Limon, F., Farf, R., Wells, G., Bamberger, D., Williams, G. V., and Pomies, Marie-Paule

Subjects
[SDU.ASTR.IM] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
Abstract

Available from the Minor Planet Center.

Published
2017

16. Controlled filling and external cleaning of multi-wall carbon nanotubes using a wet chemical method

Author

Capobianchi, A, Foglia, S, Imperatori, P, Notargiacomo, A, Giammatteo, M, Del, Buono, T, Palange, Elia, Notargiacomo, Andrea, Capobianchi, A., Foglia, S., Imperatori, P., Giammatteo, M., DEL BUONO, T., and Palange, E.

Subjects
Chemical procedure, Materials science, chemistry.chemical_element, General Chemistry, Carbon nanotube, HIGH RESOLUTION TEM, Condensed Matter::Mesoscopic Systems and Quantum Hall Effect, law.invention, Crystal, Condensed Matter::Materials Science, Potential applications of carbon nanotubes, chemistry, law, Frit compression, General Materials Science, Carbon nanotube supported catalyst, CHEMICAL FILLING, Composite material, CARBON NANOTUBE, Carbon
Abstract

A controlled, material-independent and adaptable cold wet chemical procedure is described. It allows organic and inorganic compounds to be confined inside multi-wall carbon nanotubes. The procedure mainly consists of a lyophilization process to fill multi-wall carbon nanotubes (MWCNTs), and a washing method to clean their outer surface without removing the encapsulated material. The technique was tested by synthesizing CdS crystals inside the nanotubes. Morphological and structural studies of the CdS crystals demonstrated a complete control of the synthesis process, and the possibility of maximizing the crystal size and the filling efficiency that approached 70% of open-ended nanotubes.

Published
2007
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18. 2016 RU

Author

Bressi, T. H., Sarneczky, K., Bikie, E., Bouquillon, Sébastien, Thuillot, William, Leonard, G. J., Christensen, E. J., Fuls, D. C., Gibbs, A. R., Grauer, A. D., Johnson, Jennifer A., Kowalski, R. A., Larson, S. M., Matheny, R. G., Seaman, R. L., Shelly, F. C., Holmes, Richard C., Foglia, S., Buzzi, L., Linder, T., Systèmes de Référence Temps Espace (SYRTE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Centre National de la Recherche Scientifique (CNRS), Planetology and Environments from Ground Astrometry and Space Exploration (PEGASE), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience; Available from the Minor Planet Center.

Published
2016

19. The PHEMU15 catalogue and astrometric results of the Jupiter's Galilean satellite mutual occultation and eclipse observations made in 2014–2015

Author

Saquet, E, primary, Emelyanov, N, additional, Robert, V, additional, Arlot, J-E, additional, Anbazhagan, P, additional, Baillié, K, additional, Bardecker, J, additional, Berezhnoy, A A, additional, Bretton, M, additional, Campos, F, additional, Capannoli, L, additional, Carry, B, additional, Castet, M, additional, Charbonnier, Y, additional, Chernikov, M M, additional, Christou, A, additional, Colas, F, additional, Coliac, J-F, additional, Dangl, G, additional, Dechambre, O, additional, Delcroix, M, additional, Dias-Oliveira, A, additional, Drillaud, C, additional, Duchemin, Y, additional, Dunford, R, additional, Dupouy, P, additional, Ellington, C, additional, Fabre, P, additional, Filippov, V A, additional, Finnegan, J, additional, Foglia, S, additional, Font, D, additional, Gaillard, B, additional, Galli, G, additional, Garlitz, J, additional, Gasmi, A, additional, Gaspar, H S, additional, Gault, D, additional, Gazeas, K, additional, George, T, additional, Gorda, S Y, additional, Gorshanov, D L, additional, Gualdoni, C, additional, Guhl, K, additional, Halir, K, additional, Hanna, W, additional, Henry, X, additional, Herald, D, additional, Houdin, G, additional, Ito, Y, additional, Izmailov, I S, additional, Jacobsen, J, additional, Jones, A, additional, Kamoun, S, additional, Kardasis, E, additional, Karimov, A M, additional, Khovritchev, M Y, additional, Kulikova, A M, additional, Laborde, J, additional, Lainey, V, additional, Lavayssiere, M, additional, Le Guen, P, additional, Leroy, A, additional, Loader, B, additional, Lopez, O C, additional, Lyashenko, A Y, additional, Lyssenko, P G, additional, Machado, D I, additional, Maigurova, N, additional, Manek, J, additional, Marchini, A, additional, Midavaine, T, additional, Montier, J, additional, Morgado, B E, additional, Naumov, K N, additional, Nedelcu, A, additional, Newman, J, additional, Ohlert, J M, additional, Oksanen, A, additional, Pavlov, H, additional, Petrescu, E, additional, Pomazan, A, additional, Popescu, M, additional, Pratt, A, additional, Raskhozhev, V N, additional, Resch, J-M, additional, Robilliard, D, additional, Roschina, E, additional, Rothenberg, E, additional, Rottenborn, M, additional, Rusov, S A, additional, Saby, F, additional, Saya, L F, additional, Selvakumar, G, additional, Signoret, F, additional, Slesarenko, V Y, additional, Sokov, E N, additional, Soldateschi, J, additional, Sonka, A, additional, Soulie, G, additional, Talbot, J, additional, Tejfel, V G, additional, Thuillot, W, additional, Timerson, B, additional, Toma, R, additional, Torsellini, S, additional, Trabuco, L L, additional, Traverse, P, additional, Tsamis, V, additional, Unwin, M, additional, Abbeel, F Van Den, additional, Vandenbruaene, H, additional, Vasundhara, R, additional, Velikodsky, Y I, additional, Vienne, A, additional, Vilar, J, additional, Vugnon, J-M, additional, Wuensche, N, additional, and Zeleny, P, additional

Published
2017
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21. P1.01-058 Real World Data with Nivolumab: Experience in Argentina

Author

Martin, C., primary, Lupinacci, L., additional, Perazzo, F., additional, Bas, C., additional, Carranza, O., additional, Puparelli, C., additional, Kowalyzyn, R., additional, Magri, I., additional, Varela, M., additional, Richardet, E., additional, Vera, K., additional, Foglia, S., additional, Jerez, I., additional, Aman, E., additional, Martinengo, G., additional, Batagel, E., additional, Dri, A., additional, Pilnik, N., additional, Roa, M., additional, Mando, P., additional, Tsou, F., additional, Recondo, G., additional, Cayol, F., additional, Marcos, F., additional, Sena, S., additional, Bagnes, C., additional, Minatta, J., additional, and Rizzo, M., additional

Published
2017
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22. 2015 OH22

Author

Gilmore, A. C., Kilmartin, P. M., Dennefeld, Michel, Bouquillon, Sébastien, Taris, François, Thuillot, William, Carry, Benoît, Jorda, Laurent, Tanga, Paolo, Eggl, Siegfried, David, Pedro, Carlucci, Teddy, Barache, Christophe, Pettarin, E., Linder, T., Holmes, Richard C., Serra-Ricart, Miquel, Rodríguez, M., Bosch, J. M., Haeusler, B., Dangl, G., Mantero, A., Banks, L., Blythe, M., Brungard, R., Festler, P., Mcvey, T., Paige, J., Robertson, W., Spitz, G., Byun, C., Cornell, M., Goldberg, M., Klein, A., Ruprecht, J., Ushomirsky, G., Varey, J., Viggh, H., Woods, D., Foglia, S., Buzzi, L., Baj, G., Moravec, Z., Schmalz, S., Tungalag, N., Systèmes de Référence Temps Espace (SYRTE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Systèmes de référence célestes, Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience; Available from the Minor Planet Center.

Published
2015

24. 2014 UK57 = 2004 RL341

Author

Bouquillon, Sébastien, Thuillot, William, Holmes, Richard C., Buzzi, L., Foglia, S., Vorobjov, T., Linder, T., Williams, G. V., Systèmes de Référence Temps Espace (SYRTE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Systèmes de référence célestes, Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience; Not Available

Published
2014

25. Affinity immobilization of aptamers on graphene oxide for biosensor applications

Author

Foglia S., Lamberti I., Berzina T.S., Cerchia L., Ranzieri P., Quagliano L.G., Tanzarella C., Tarabella G., Iannotta S., and De Franciscis V.

Subjects
Aptamer, graphene
Abstract

The preparation of biorecognition layers on the surface of a sensing platform is a very crucial step for the development of sensitive and selective biosensor. The incredibly large specific surface area, the abundant surface functionalities and the high water solubility indicate graphene oxide (GO) sheets as ideal substrate for such application. The immobilization of aptamers as the recognition element on GO allows the formation of a nanocomplex, usable as biosensing platform in an aptasensors. In this work, we investigate the immobilization of the biotin-thrombin-aptamer on GO, exploiting the high affinity of avidin for biotin. Avidin was directly immobilized on GO without any chemical functionalization, following a simple incubation procedure, performed in PBS. The ability of Avidin-GO substrate to bind biotinylated aptamers could lead an oriented immobilization of the recognition element (i.e. aptamer), avoiding unwanted interaction between aptamer and GO and keeping intact the exposed binding sites for the thrombin assay. The immobilization was observed directly using atomic force microscopy (AFM) and the modification of the GO functional groups was verified by UV-vis and Fourier transform infrared (FT-IR) spectroscopy.

Published
2014

28. 2013 QF11

Author

Boattini, A., Christensen, E. J., Gibbs, A. R., Grauer, A. D., Hill, R. E., Johnson, J. A., Kowalski, R. A., Larson, S. M., Mcnaught, R. H., Shelly, F. C., Fratev, F., Minkov, M., Hume, C., Twer, A., Klein, M., Mantero, A., Holmes, R., Foglia, S., Buzzi, L., Devore, H., Kostin, A., Linder, T., Lister, T., Vorobjov, T., Hug, G., Losse, F., Cavalié, T., D'Anna, W., Birtwhistle, P., Università degli Studi di Roma Tor Vergata [Roma], Laboratoire d'Ingénierie des Matériaux (LIM), Centre National de la Recherche Scientifique (CNRS), SSE 2013, Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux (L3AB), Université Sciences et Technologies - Bordeaux 1-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Observatoire aquitain des sciences de l'univers (OASU), Université Sciences et Technologies - Bordeaux 1-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS)-Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB), Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Bordeaux (UB), and FORMATION STELLAIRE 2013

Subjects
[PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], Astrophysics::Earth and Planetary Astrophysics
Abstract

Available from the Minor Planet Center.

Published
2013

29. Minor Planet Observations [W85 Cerro Tololo-LCOGT A]

Author

Lister, Tim A., Christensen, E. J., Larson, S. M., Buzzi, L., Vorobjov, T., Foglia, S., Miller, P., Altmann, Martin, Brown, T., Bouquillon, Sébastien, Taris, François, Carlucci, Teddy, Barache, Christophe, Systèmes de Référence Temps Espace (SYRTE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Systèmes de référence célestes, Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience; Not Available

Published
2013

30. Aptamer based SERS sensing surface for direct detection of proteins

Author

Lamberti I, Antoccia A., Battocchio C., Quagliano L.G., Tanzarella C., Iucci g., and Foglia S.

Subjects
SERS, Aptamers
Abstract

Aptamers, specific nucleic acid selected from random sequence pools, are a valid alternative to antibodies or other biomimetic receptors. Aptamer-based biosystems are still immature compared to immunoassays, which reflects the limited availability of aptamer types and for this purpose an optical aptamer-based detection systems label free appear as highly efficient devices with enormous potential. [Ellington, A.D., Szostak, J.W., 1990. Nature 346,818-822; Song S., Wanga L., Lia J., Fana C., Zhaob J., 2008 TrAC 27(2), 108-117] We approach the development of an affinity based detection system for analytes unlimited by size and tossicity, designing a nanoaptasensor sensing surface for microfluidic device, coupled with Surface Enhanced Raman Spectroscopy (SERS). Among the optical detection methods, SERS distinguishes itself with several advantages: the spectrum change brought by a single molecules, is induced by the specific interaction between aptamers and their own proteins and the spectral probe specificity is excellent in comparison to the fluorescence methods. The thrombin aptamer is the first example of ssDNA oligonucleotides that bind a target protein with unknown specificity for nucleic acids. [Bock, L.C., et al., 1992. Nature 355, 564-566] A Thrombin SERS aptasensor is usually realized by a sandwich structure, formed between the immobilized aptamer, the protein target and a secondary aptamer bound to a Raman probe (i.e. gold nanoparticles ), which requires a consuming and inconvenient handling step. [Sassolas A, Blum L. J., Leca-Bouvier B. D. 2011 Biosens Bioelectron., on line] In attempt to over come this drawback we report the preparation of a aptamer terminated sensing surface, allowing a faster and cheaper system and suitable for an analytical label free measurements, in order to perform a direct analisys of biological samples. We develop a multi-step depositional sequence: firstly was prepared a mixed self assembled monolayer (SAM) on a gold thin film, containing a binary mixture of biotinylated alkylthiol (BAT) with the capacity to graft neutravidin proteins and diluent methyl-terminated alkylthiol. The composition depth profile of the mixed SAMs was examined by angle-resolved XPS. Insight in to the order of the SAM system was provided by NEXAFS characterization [Nelson K.E., Gamble L., et al. 2001, Langmuir, 17, 2807-2816]. BAT was produced by a solid-phase synthesis, based on a resin, which protects the thiol group and prevents the formation of non-desired compounds [Prats-Alfonso E. et al. 2006 Tetrahedron 62, 6876-6881]. In a second step, the bioconjugation with an avidin-gold sol is performed. Monodispersed 5 nm gold particles were prepared in aqueous medium and covered with neutravidin, overcoming possible non-specific bindings, which are usually attribuited to the isolectric point (~ 6) of neutravidin [Grabar, K.C et al. 1995 Anal. Chem. 67, 735-743; Morris R.E. and Saelinger C.B. 1984 The journal of Histochemistry and Cytochemistry 32, 124-128]. Gold colloid was prepared by reducing tetrachloroauric(III) acid with sodium citrate controlling growth kinetics and temporal size/shape evolution of gold nanocrystal. The citrate plays a dual role as reducing agent and protection capping group and temperature and pH values of the citrate reaction drastically affect the size and quality of the particles. The morphologies was observed by atom force microscopy (AFM) and the concentration of gold species in the colloid was monitored by UV-vis spectra.[Kimling J. et al.2006 J.Phys.Chem B 110, 15700-15707; Ji X. et al. 2007 J.Am.Chem.Soc. 129, 13939-13948] In the ending step, the Aptamer is bond to the surface thought the avidin-biotin linkage. In this strategy aptamer against thrombin [5'GGT TGG TGT GGT TGG T(15)3'Biotin], marked by a guanine quadruplex (G-quadruplex), is used. The resulting SERS changes involved was observed when the target molecule (Thrombin) interacts with its own aptamer [Nie S.; and Emory S. R. 1997 Science 275, 1102].

Published
2011

33. L10 FePt-filled Carbon Nanotubes by Wet Chemical Synthesis

Author

Capobianchi A., Foglia S., Palange E., Arrizza L., Veroli C., Vasquez Mansilla M., and Fiorani D.

Subjects
Condensed Matter::Materials Science
Abstract

This paper reports on the synthesis of iron-platinum (FePt) alloy clusters within Multi Wall Carbon Nanotubes using a novel wet chemical method that allows the filling of the nanotube cavity keeping clear their external wall. In the present case, the procedure permits the filling of the nanotubes with precursor salts of Pt and Fe and, by direct heating at 700°C of the Fe and Pt mixed salts, magnetic hard, face-centred-tetragonal (fct) crystallographic (L10) phase FePt alloy nanoparticles are obtained without the need to pass through the formation of the magnetic soft, face-centred-cubic (fcc) FePt alloy phase. By a suitable choice of the concentration of the starting material solution, we obtained particles of two different sizes into the nanotubes with magnetic blocked and super-paramagnetic states at room temperature. Morphological, structural and magnetic properties of the filled nanotubes have been performed by magnetic measurements, X-ray diffraction and transmission electron microscopy in normal and high resolution mode

Published
2009

34. Searching for V-type and Q-type Main-Belt Asteroids Based on SDSS Colors

Author

Binzel, Richard P., Masi, G., Foglia, S., Vernazza, Pierre, Burbine, T. H., Thomas, Cristina A., Demeo, Francesca E., Nesvorny, David, Birlan, Mirel, Fulchignoni, Marcello, Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Ingénieurs, Techniciens et Administratifs, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience

Published
2007

35. Thermal behavior of Zn and Cd complexes intercalated into gamma-zirconium phosphate - Synthesis and physical-chemical characterization

Author

Ferragina C., Di Rocco R., Foglia S., and Petrilli L.

Abstract

Intercalation compounds such as zinc and cadmium diamines complexes intercalated into the inorganic layered ion-exchanger gamma-zirconium phosphate have been synthesized and characterized. The diamine content intercalated inside the host matrix depends on the ligand size; the complexes "in situ" formed depend on the metal ion exchanged. Only in the case of the 2,2'-bipyridyl amine, after cation exchange with Zn and Cd, is an increase of the interlayer distance observed and an energy variations from the IR measurements. All the prepared materials maintained thermal stability up to about 400 degrees C. At a higher temperature combustion of the complexes occurs depending on the ligand size.

Published
2007
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39. Free Rotor ?Like Behaviour of Magnetite Nanoparticles in Polymeric Matrices

Author

Testa A.M. 1, Foglia S. 1, Suber L. 1, Fiorani D. 1, Roig A.2, Ll Casas 2, Molins E.2, Grenèche J.M. 3, and Tejada J. 4

Subjects
Condensed Matter::Materials Science, nanocompositi, sintesi chimica, magnetismo
Abstract

We report the results of magnetization and 57Fe Mossbauer spectroscopy measurements performed at 5-300K on composites containg Fe3O4 nanoparticles encased in polystyrene-type resins. After carrying out a suitable field treatment to decouple the particles from the matrix, a fraction of the particles freely rotate in response to an applied magnetic field.

Published
2001

40. The PHEMU03 catalogue of observations of the mutual phenomena of the Galilean satellites of Jupiter

Author

Arlot, J. -E., Thuillot, W., Ruatti, C., Ahmad, A., Amosse, A., Anbazhagan, P., Andreyev, M., Antov, A., Appakutty, M., Asher, D., Aubry, S., Baron, N., Bassiere, N., Berthe, M., Bogdanovski, R., Bosq, F., Bredner, E., Buettner, D., Buromsky, M., Cammarata, S., Casas, R., Chis, G. D., Christou, A. A., Coquerel, J. -P., Corlan, R., Cremaschini, C., Crussaire, D., Cuypers, J., Dennefeld, M., Descamps, P., Devyatkin, A., Dimitrov, D., Dorokhova, T. N., Dorokhov, N. I., Dourneau, G., Duenas, M., Dumitrescu, A., Emelianov, N., Ferrara, D., Fiel, D., Fienga, A., Flatres, T., Foglia, S., Garlitz, J., Gerbos, J., Gilbert, R., Goncalves, R. M. D., Gonzales, D., Gorda, S. Yu., Gorshanov, D. L., Hansen, M. W., Harrington, M., Irsmambetova, T. R., Ito, Y., Ivanova, V., Izmailov, I. S., Khovritchev, M. Yu., Khrutskaya, E. V., Kieken, J., Kiseleva, T. P., Kuppuswamy, K., Lainey, V., Lavayssiere, M., Lazzarotti, P., Le Campion, J. -F., Lellouch, E., Li, Z. L., Lo Savio, E., Lou, M., Magny, E., Manek, J., Marinello, W., Marino, G., McAuliffe, J. P., Michelli, M., Moldovan, D., Montagnac, S., Moorthy, V., Nickel, O., Nier, J. M., Noel, T., Noyelles, B., Oksanen, A., Parrat, D., Pauwels, T., Peng, Q. Y., Pizzetti, G., Priban, V., Ramachandran, B., Rambaux, N., Rapaport, M., Rapavy, P., Rau, G., Sacre, J. -J., Sada, P. V., Salvaggio, F., Sarlin, P., Sciuto, C., Selvakumar, G., Sergeyev, A., Sidorov, M., Sorescu, S., Spampinato, S. A., Stellmacher, I., Trunkovsky, E., Tejfel, V., Tudose, V., Turcu, V., Ugarte, I., Vantyghem, P., Vasundhara, R., Vaubaillon, J., Velu, C., Venkataramana, A. K., Vidal-Sainz, J., Vienne, A., Vilar, J., Vingerhoets, P., Vollman, W., Arlot, J. -E., Thuillot, W., Ruatti, C., Ahmad, A., Amosse, A., Anbazhagan, P., Andreyev, M., Antov, A., Appakutty, M., Asher, D., Aubry, S., Baron, N., Bassiere, N., Berthe, M., Bogdanovski, R., Bosq, F., Bredner, E., Buettner, D., Buromsky, M., Cammarata, S., Casas, R., Chis, G. D., Christou, A. A., Coquerel, J. -P., Corlan, R., Cremaschini, C., Crussaire, D., Cuypers, J., Dennefeld, M., Descamps, P., Devyatkin, A., Dimitrov, D., Dorokhova, T. N., Dorokhov, N. I., Dourneau, G., Duenas, M., Dumitrescu, A., Emelianov, N., Ferrara, D., Fiel, D., Fienga, A., Flatres, T., Foglia, S., Garlitz, J., Gerbos, J., Gilbert, R., Goncalves, R. M. D., Gonzales, D., Gorda, S. Yu., Gorshanov, D. L., Hansen, M. W., Harrington, M., Irsmambetova, T. R., Ito, Y., Ivanova, V., Izmailov, I. S., Khovritchev, M. Yu., Khrutskaya, E. V., Kieken, J., Kiseleva, T. P., Kuppuswamy, K., Lainey, V., Lavayssiere, M., Lazzarotti, P., Le Campion, J. -F., Lellouch, E., Li, Z. L., Lo Savio, E., Lou, M., Magny, E., Manek, J., Marinello, W., Marino, G., McAuliffe, J. P., Michelli, M., Moldovan, D., Montagnac, S., Moorthy, V., Nickel, O., Nier, J. M., Noel, T., Noyelles, B., Oksanen, A., Parrat, D., Pauwels, T., Peng, Q. Y., Pizzetti, G., Priban, V., Ramachandran, B., Rambaux, N., Rapaport, M., Rapavy, P., Rau, G., Sacre, J. -J., Sada, P. V., Salvaggio, F., Sarlin, P., Sciuto, C., Selvakumar, G., Sergeyev, A., Sidorov, M., Sorescu, S., Spampinato, S. A., Stellmacher, I., Trunkovsky, E., Tejfel, V., Tudose, V., Turcu, V., Ugarte, I., Vantyghem, P., Vasundhara, R., Vaubaillon, J., Velu, C., Venkataramana, A. K., Vidal-Sainz, J., Vienne, A., Vilar, J., Vingerhoets, P., and Vollman, W.

Published
2009

44. The PHEMU03 catalogue of observations of the mutual phenomena of the Galilean satellites of Jupiter

Author

Arlot, J.-E., primary, Thuillot, W., additional, Ruatti, C., additional, Ahmad, A., additional, Amossé, A., additional, Anbazhagan, P., additional, Andreyev, M., additional, Antov, A., additional, Appakutty, M., additional, Asher, D., additional, Aubry, S., additional, Baron, N., additional, Bassiere, N., additional, Berthe, M., additional, Bogdanovski, R., additional, Bosq, F., additional, Bredner, E., additional, Buettner, D., additional, Buromsky, M., additional, Cammarata, S., additional, Casas, R., additional, Chis, G. D., additional, Christou, A. A., additional, Coquerel, J.-P., additional, Corlan, R., additional, Cremaschini, C., additional, Crussaire, D., additional, Cuypers, J., additional, Dennefeld, M., additional, Descamps, P., additional, Devyatkin, A., additional, Dimitrov, D., additional, Dorokhova, T. N., additional, Dorokhov, N. I., additional, Dourneau, G., additional, Dueñas, M., additional, Dumitrescu, A., additional, Emelianov, N., additional, Ferrara, D., additional, Fiel, D., additional, Fienga, A., additional, Flatres, T., additional, Foglia, S., additional, Garlitz, J., additional, Gerbos, J., additional, Gilbert, R., additional, Goncalves, R. M. D., additional, Gonzãles, D., additional, Gorda, S. Yu., additional, Gorshanov, D. L., additional, Hansen, M. W., additional, Harrington, M., additional, Irsmambetova, T. R., additional, Ito, Y., additional, Ivanova, V., additional, Izmailov, I. S., additional, Khovritchev, M. Yu., additional, Khrutskaya, E. V., additional, Kieken, J., additional, Kiseleva, T. P., additional, Kuppuswamy, K., additional, Lainey, V., additional, Lavayssiére, M., additional, Lazzarotti, P., additional, Le Campion, J.-F., additional, Lellouch, E., additional, Li, Z. L., additional, Lo Savio, E., additional, Lou, M., additional, Magny, E., additional, Manek, J., additional, Marinello, W., additional, Marino, G., additional, McAuliffe, J. P., additional, Michelli, M., additional, Moldovan, D., additional, Montagnac, S., additional, Moorthy, V., additional, Nickel, O., additional, Nier, J. M., additional, Noel, T., additional, Noyelles, B., additional, Oksanen, A., additional, Parrat, D., additional, Pauwels, T., additional, Peng, Q. Y., additional, Pizzetti, G., additional, Priban, V., additional, Ramachandran, B., additional, Rambaux, N., additional, Rapaport, M., additional, Rapavy, P., additional, Rau, G., additional, Sacré, J.-J., additional, Sada, P. V., additional, Salvaggio, F., additional, Sarlin, P., additional, Sciuto, C., additional, Selvakumar, G., additional, Sergeyev, A., additional, Sidorov, M., additional, Sorescu, S., additional, Spampinato, S. A., additional, Stellmacher, I., additional, Trunkovsky, E., additional, Tejfel, V., additional, Tudose, V., additional, Turcu, V., additional, Ugarte, I., additional, Vantyghem, P., additional, Vasundhara, R., additional, Vaubaillon, J., additional, Velu, C., additional, Venkataramana, A. K., additional, Vidal-Sãinz, J., additional, Vienne, A., additional, Vilar, J., additional, Vingerhoets, P., additional, and Vollman, W., additional

Published
2008
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45. The PHEMU97 catalogue of observations of the mutual phenomena of the Galilean satellites of Jupiter

Author

Arlot, J.-E., primary, Thuillot, W., additional, Ruatti, C., additional, Akasawa, H., additional, Baroni, S., additional, Beisker, W., additional, Berthier, J., additional, Blanco, C., additional, Boonstra, J., additional, Bourgeois, J., additional, Bulder, H., additional, Casas, R., additional, Castano, J. G., additional, Colas, F., additional, Collins, D., additional, Cuypers, J., additional, Czech, W., additional, D'Ambrosio, V., additional, Denzau, H., additional, Descamps, P., additional, Dimitrescu, A., additional, Dinakarian, N., additional, Dourneau, G., additional, Emelyanov, N., additional, Enriquez, J. M., additional, Fernandez, J. M., additional, Fernandez-Barba, D., additional, Flatres, T., additional, Foglia, S., additional, Goncalves, M., additional, Guhl, K., additional, Helmer, G., additional, Hirose, T., additional, Irsmambetova, T. R., additional, Krobusek, B. A., additional, Lecacheux, J., additional, Le Campion, J.-F., additional, Lou, M., additional, Mallama, A., additional, Marchis, F., additional, Navarro, M. A. S., additional, Nelson, P., additional, Okura, N., additional, Park, J., additional, Pauwels, T., additional, Pluchino, S., additional, Priban, V., additional, Rapaport, M., additional, Sacré, J.-J., additional, Salvaggio, F., additional, Sanchez, M. A., additional, Sanchez-Bajo, F., additional, Stefanescu, G., additional, Tanga, P., additional, Tejfel, V. G., additional, Trisan, J. L., additional, Trunkovsky, E. M., additional, Van Gestel, J., additional, Vandenbulcke, G., additional, Vasundhara, R., additional, Vass, G., additional, Vingerhoets, P., additional, Vu, D. T., additional, and Wilds, R. T., additional

Published
2006
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47. The PHESAT95 catalogue of observations of the mutual events of the Saturnian satellites

Author

Thuillot, W., primary, Arlot, J.-E., additional, Ruatti, C., additional, Berthier, J., additional, Blanco, C., additional, Colas, F., additional, Czech, W., additional, Damani, M., additional, D'Ambrosio, V., additional, Descamps, P., additional, Dourneau, G., additional, Emelianov, N., additional, Foglia, S., additional, Helmer, G., additional, Irsmambetova, T. R., additional, James, N., additional, Laques, P., additional, Lecacheux, J., additional, Le Campion, J.-F., additional, Ledoux, C., additional, Le Floch, J.-C., additional, Oprescu, G., additional, Rapaport, M., additional, Riccioli, R., additional, Starosta, B., additional, Tejfel, V. G., additional, Trunkovsky, E. M., additional, Viateau, B., additional, Veiga, C. H., additional, and Vu, D. T., additional

Published
2001
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