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201by Wagner, J., Ansmann, A., Wandinger, U., Seifert, P., Schwarz, A., Tesche, Matthias, Chaikovsky, A., Dubovik, O.“... photometry and allows us to retrieve vertical profiles of particle optical and microphysical properties...”
Published in Atmospheric Measurement Techniques (2013)
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202by Mékarnia, D., Chapellier, E., Guillot, T., Abe, L., Agabi, A., de Pra, Y., Schmider, F. -X., Zwintz, K., Stevenson, K. B., Wang, J. J., Lagrange, A. -M., Bigot, L., Crouzet, N., Fanteï-Caujolle, Y., Christille, J. -M., Kalas, P.“... photometric data were obtained using aperture photometry by telescope defocussing. The 66 418 data points were...”
Published in Astronomy & Astrophysics (2017)
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203by Mékarnia, D., Chapellier, E., Guillot, T., Abe, L., Agabi, A., de Pra, Y., Schmider, F. -X., Zwintz, K., Stevenson, K. B., Wang, J. J., Lagrange, A. -M., Bigot, L., Crouzet, N., Fanteï-Caujolle, Y., Christille, J. -M., Kalas, P.“... photometric data were obtained using aperture photometry by telescope defocussing. The 66 418 data points were...”
Published in Astronomy & Astrophysics (2017)
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204by Aurière, M., Konstantinova-Antova, R., Petit, P., Roudier, T., Donati, J.-F., Charbonnel, Corinne, Dintrans, B., Lignières, F., Wade, G. A., Morgenthaler, A., Tsvetkova, S.“... timescale compatible with the rotational period inferred from photometry (308.8 d), however large deviations...”
Published in Astronomy & Astrophysics (2011)
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205by Aurière, M., Konstantinova-Antova, R., Petit, P., Roudier, T., Donati, J.-F., Charbonnel, Corinne, Dintrans, B., Lignières, F., Wade, G. A., Morgenthaler, A., Tsvetkova, S.“... timescale compatible with the rotational period inferred from photometry (308.8 d), however large deviations...”
Published in Astronomy & Astrophysics (2011)
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206by Aurière, M., Konstantinova-Antova, R., Petit, P., Roudier, T., Donati, J.-F., Charbonnel, Corinne, Dintrans, B., Lignières, F., Wade, G. A., Morgenthaler, A., Tsvetkova, S.“... timescale compatible with the rotational period inferred from photometry (308.8 d), however large deviations...”
Published in Astronomy & Astrophysics (2011)
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207by Strandet, M. L., Weiss, Axel, de Breuck, C., Marrone, Daniel P., Vieira, J. D., Aravena, Manuel, Ashby, M. L. N., Béthermin, M., Bothwell, M. S., Bradford, C. M., Carlstrom, J. E., Chapman, S. C., Cunningham, D. J. M., Chen, Chian-Chou, Fassnacht, C. D., Gonzalez, Anthony H., Greve, T. R., Gullberg, B., Hayward, C. C., Hezaveh, Y., Litke, Katrina C., Ma, J., Malkan, M., Menten, Karl M., Miller, T., Murphy, Eric J., Narayanan, D., Phadke, K. A., Rotermund, K. M., Spilker, Justin S., Sreevani, J.“... transfer analysis of the dust continuum photometry and the CO and [C I] line emission. This allows us...”
Published in The Astrophysical Journal (2017)
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208by Petit, P., Folsom, C. P., Donati, J.-F., Yu, L., do Nascimento Jr., J.-D., Jeffers, S. V., Marsden, S. C., Morin, J., Vidotto, A. A.“... and broadband photometry display clear signs of non-rotational evolution over the course of data collection...”
Published in Astronomy & Astrophysics (2021)
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209by Lemasle, Bertrand, François, Patrick, Piersimoni, A. M., Pedicelli, S., Bono, G., Laney, C. D., Primas, Francesca, Romaniello, M.“...-infrared photometry are adopted to constrain the Galactic iron gradient beyond 10 kpc. Methods: Iron...”
Published 2008
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210by Tubiana, C., Snodgrass, Colin, Bertini, I., Mottola, S., Vincent, J.-B., Lara, L., Fornasier, S., Knollenberg, J., Thomas, N., Fulle, M., Agarwal, J., Bodewits, D., Ferri, F., Güttler, C., Gutierrez, P. J., La Forgia, F., Lowry, S., Magrin, S., Oklay, N., Pajola, M., Rodrigo, R., Sierks, H., A’Hearn, M. F., Angrilli, F., Barbieri, C., Barucci, M. A., Bertaux, J.-L., Cremonese, G., Da Deppo, V., Davidsson, B., De Cecco, M., Debei, S., Groussin, O., Hviid, S. F., Ip, W., Jorda, L., Keller, H. U., Koschny, D., Kramm, R., Kührt, E., Küppers, M., Lazzarin, M., Lamy, P. L., Lopez Moreno, J. J., Marzari, F., Michalik, H., Naletto, G., Rickman, H., Sabau, L., Wenzel, K.-P.“... photometry, we investigated how the comet brightness varies with heliocentric distance. 67P was likely...”
Published in Astronomy & Astrophysics (2015)
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211by Lemasle, Bertrand, François, Patrick, Piersimoni, A. M., Pedicelli, S., Bono, G., Laney, C. D., Primas, Francesca, Romaniello, M.“...-infrared photometry are adopted to constrain the Galactic iron gradient beyond 10 kpc. Methods: Iron...”
Published 2008
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212by Lemasle, Bertrand, François, Patrick, Piersimoni, A. M., Pedicelli, S., Bono, G., Laney, C. D., Primas, Francesca, Romaniello, M.“...-infrared photometry are adopted to constrain the Galactic iron gradient beyond 10 kpc. Methods: Iron...”
Published 2008
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213by Auriere, M., Konstantinova-Antova, R., Petit, P., Roudier, T., Donati, J. -F., Charbonnel, C., Dintrans, B., Lignieres, F., Wade, G. A., Morgenthaler, A., Tsvetkova, S.“... smoothly on a timescale compatible with the rotational period inferred from photometry (308.8 d.), however...”
Published 2011
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214by Petit, P., Folsom, C. P., Donati, J. -F., Yu, L., Nascimento Jr., J. -D. do, Jeffers, S., Marsden, S. C., Morin, J., Vidotto, A. A.“...-scale magnetic field geometry, chromospheric emission, and broadband photometry display clear signs...”
Published in Astronomy & Astrophysics (2021)
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215by Gandolfi, Davide, Parviainen, Hannu, Fridlund, Malcolm, Hatzes, Artie, Deeg, Hans, Frasca, A., Lanza, Antonino, Prada Moroni, Pier Giorgio, Tognelli, E., McQuillan, Amy, Aigrain, Suzanne, Alonso, Roi, Antoci, Victoria, Cabrera, Juan, Carone, Ludmila, Csizmadia, Szillard, Djupvik, A., Guenther, Eike, Jessen-Hansen, J., Ofir, Aviv, Telting, J.“...-day orbit around a metal-rich solar-like star. We combined the publicly available Kepler photometry...”
Published in Astronomy & Astrophysics (2013)
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216by Tubiana, C., Snodgrass, C., Bertini, I., Mottola, S., Vincent, J.-B., Lara López, Luisa M., Fornasier, S., Knollenberg, J., Thomas, N., Fulle, M., Agarwal, J., Bodewits, D., Ferri, F., Güttler, C., Gutierrez, P. J., La Forgia, F, Lowry, S., Magrin, S., Oklay, N., Pajola, M., Rodrigo, R., Sierks, H., A’Hearn, M. F., Angrilli, F., Barbieri, C., Barucci, M. A., Bertaux, J.-L., Cremonese, G., Da Deppo, V., Davidsson, B., De Cecco, M., Debei, S., Groussin, O., Hviid, S., Ip, W-H., Jorda, L., Keller, H. U., Koschny, D., Kramm, R., Kührt, E., Küppers, M., Lazzarin, M., Lamy, P., Lopez Moreno, J., Marzari, F., Michalik, H., Naletto, G., Rickman, H., Sabau, L., Wenzel, K. P.“... photometry, we investigated how the comet brightness varies with heliocentric distance. 67P was likely...”
Published in Astronomy & Astrophysics (2015)
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217by Lemasle, Bertrand, François, Patrick, Piersimoni, A. M., Pedicelli, S., Bono, G., Laney, C. D., Primas, Francesca, Romaniello, M.“...-infrared photometry are adopted to constrain the Galactic iron gradient beyond 10 kpc. Methods: Iron...”
Published 2008
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218by Lemasle, Bertrand, François, Patrick, Piersimoni, A. M., Pedicelli, S., Bono, G., Laney, C. D., Primas, Francesca, Romaniello, M.“...-infrared photometry are adopted to constrain the Galactic iron gradient beyond 10 kpc. Methods: Iron...”
Published 2008
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219by Tubiana, C., Snodgrass, C., Mottola, S., Vincent, J. B., Lara, L., Fornasier, S., Knollenberg, J., Thomas, N., Fulle, M., Agarwal, J., Bodewits, D., Güttler, C., Gutierrez, P. J., Lowry, S., Oklay, N., Rodrigo, R., Sierks, H., A’Hearn, M. F., Barucci, M. A., Bertaux, J. L., Cremonese, G., Da Deppo, V., Davidsson, B., De Cecco, M., Groussin, O., Hviid, S. F., Ip, W., Jorda, L., Keller, H. U., Koschny, D., Kramm, R., Kührt, E., Küppers, M., Lamy, P. L., Lopez Moreno, J. J., Michalik, H., Rickman, H., Sabau, L., Wenzel, K. P., BERTINI, IVANO, FERRI, FRANCESCA, LA FORGIA, FIORANGELA, MAGRIN, SARA, PAJOLA, MAURIZIO, ANGRILLI, FRANCESCO, BARBIERI, CESARE, DEBEI, STEFANO, LAZZARIN, MONICA, MARZARI, FRANCESCO, NALETTO, GIAMPIERO“... photometry, we investigated how the comet brightness varies with heliocentric distance. 67P was likely...”
Published in Astronomy & Astrophysics (2015)
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220by Tubiana C., Snodgrass C., Bertini I., Mottola S., Vincent J. -B., Lara L., Fornasier S., Knollenberg J., Thomas N., Fulle M., Agarwal J., Bodewits D., Ferri F., Guttler C., Gutierrez P. J., La Forgia F., Lowry S., Magrin S., Oklay N., Pajola M., Rodrigo R., Sierks H., A'hearn M. F., Angrilli F., Barbieri C., Barucci M. A., Bertaux J. -L., Cremonese G., Da Deppo V., Davidsson B., De Cecco M., Debei S., Groussin O., Hviid S. F., Ip W., Jorda L., Keller H. U., Koschny D., Kramm R., Kuhrt E., Kuppers M., Lazzarin M., Lamy P. L., Lopez Moreno J. J., Marzari F., Michalik H., Naletto G., Rickman H., Sabau L., Wenzel K. -P.“... photometry, we investigated how the comet brightness varies with heliocentric distance. 67P was likely...”
Published in Astronomy & Astrophysics (2015)
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