Zobrazeno 1 - 10
of 171
pro vyhledávání: '"Hines, D. C."'
Autor:
Libralato, M., Argyriou, I., Dicken, D., Marín, M. García, Guillard, P., Hines, D. C., Kavanagh, P. J., Kendrew, S., Law, D. R., Noriega-Crespo, A., Álvarez-Márquez, J.
Astrometry is one of the main pillars of astronomy, and one of its oldest branches. Over the years, an increasing number of astrometric works by means of Hubble Space Telescope (HST) data have revolutionized our understanding of various phenomena. Wi
Externí odkaz:
http://arxiv.org/abs/2311.12145
Autor:
Emery, J. P., Wong, I., Brunetto, R., Cook, J. C., Pinilla-Alonso, N., Stansberry, J. A., Holler, B. J., Grundy, W. M., Protopapa, S., Souza-Feliciano, A. C., Fernández-Valenzuela, E., Lunine, J. I., Hines, D. C.
We observed Sedna, Gonggong, and Quaoar with the NIRSpec instrument on the James Webb Space Telescope (JWST). All three bodies were observed in the low-resolution prism mode at wavelengths spanning 0.7 to 5.2 $\mu$m. Quaoar was also observed at 10x h
Externí odkaz:
http://arxiv.org/abs/2309.15230
Autor:
Choquet, É., Bryden, G., Perrin, M. D., Soummer, R., Augereau, J.-C., Chen, C. H., Debes, J. H., Gofas-Salas, E., Hagan, J. B., Hines, D. C., Mawet, D., Morales, F., Pueyo, L., Rajan, A., Ren, B., Schneider, G., Stark, C. C., Wolff, S.
We present the first scattered-light images of two debris disks around the F8 star HD. 104860 and the F0V star HD. 192758, respectively similar to 45 and similar to 67. pc away. We detected these systems in the F110W and F160W filters through our rea
Externí odkaz:
http://hdl.handle.net/10150/627098
http://arizona.openrepository.com/arizona/handle/10150/627098
http://arizona.openrepository.com/arizona/handle/10150/627098
Autor:
Boccaletti, A., Cossou, C., Baudoz, P., Lagage, P. O., Dicken, D., Glasse, A., Hines, D. C., Aguilar, J., Detre, O., Nickson, B., Noriega-Crespo, A., Gáspár, A., Labiano, A., Stark, C., Rouan, D., Reess, J. M., Wright, G. S., Rieke, G., Marin, M. Garcia
Publikováno v:
A&A 667, A165 (2022)
Characterization of directly imaged exoplanets is one of the most eagerly anticipated science functions of the James Webb Space Telescope. MIRI, the mid-IR instrument has the capability to provide unique spatially resolved photometric data points in
Externí odkaz:
http://arxiv.org/abs/2207.11080
Autor:
Zubko, E., Chornaya, E., Zheltobryukhov, M., Matkin, A., Ivanova, O. V., Bodewits, D., Kochergin, A., Kornienko, G., Luk'yanyk, I., Hines, D. C., Videen, G.
We measured the degree of linear polarization P of comet C/2018 V1 (Machholz-Fujikawa-Iwamoto) with the broadband Johnson V filter in mid-November of 2018. Within a radius of \r{ho}=17,000 km of the inner coma, we detected an extremely low linear pol
Externí odkaz:
http://arxiv.org/abs/2012.10724
Autor:
Stevance, H. F., Baade, D., Bruten, J. R., Cikota, A., Clocchiatti, A., Hines, D. C., Höflich, P., Maund, J. R., Patat, F., Vallely, P. J., Wheeler, J. C.
SN 1993J is one of the best studied Type IIb supernovae. Spectropolarimetric data analyses were published over two decades ago at a time when the field of supernova spectropolarimetry was in its infancy. Here we present a new analysis of the spectrop
Externí odkaz:
http://arxiv.org/abs/2003.06032
Akademický článek
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Autor:
Choquet, É., Bryden, G., Perrin, M. D., Soummer, R., Augereau, J. -C., Chen, C. H., Debes, J. H., Gofas-Salas, E., Hagan, J. B., Hines, D. C., Mawet, D., Morales, F., Pueyo, L., Rajan, A., Ren, B., Schneider, G., Stark, C. C., Wolff, S.
We present the first scattered-light images of two debris disks around the F8 star HD 104860 and the F0V star HD 192758, respectively $\sim45$ and $\sim67$ pc away. We detected these systems in the F110W and F160W filters through our re-analysis of a
Externí odkaz:
http://arxiv.org/abs/1801.05424
Autor:
Choquet, É., Milli, J., Wahhaj, Z., Soummer, R., Roberge, A., Augereau, J. -C., Booth, M., Absil, O., Boccaletti, A., Chen, C. H., Debes, J. H., del Burgo, C., Dent, W. R. F., Ertel, S., Girard, J. H., Gofas-Salas, E., Golimowski, D. A., González, C. A. Gómez, Hagan, J. B., Hibon, P., Hines, D. C., Kennedy, G. M., Lagrange, A. -M., Matrà, L., Mawet, D., Mouillet, D., N'Diaye, M., Perrin, M. D., Pinte, C., Pueyo, L., Rajan, A., Schneider, G., Wolff, S., Wyatt, M.
We present the first scattered-light images of the debris disk around 49 ceti, a ~40 Myr A1 main sequence star at 59 pc, famous for hosting two massive dust belts as well as large quantities of atomic and molecular gas. The outer disk is revealed in
Externí odkaz:
http://arxiv.org/abs/1612.07320
Akademický článek
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