OGLE 2008--BLG--290: An accurate measurement of the limb darkening of a Galactic Bulge K Giant spatially resolved by microlensing

Autor: Fouque, P., Heyrovsky, D., Dong, S., Gould, A., Udalski, A., Albrow, M. D., Batista, V., Beaulieu, J. -P., Bennett, D. P., Bond, I. A., Bramich, D. M., Novati, S. Calchi, Cassan, A., Coutures, C., Dieters, S., Dominik, M., Prester, D. Dominis, Greenhill, J., Horne, K., Jorgensen, U. G., Kozlowski, S., Kubas, D., Lee, C. -H., Marquette, J. -B., Mathiasen, M., Menzies, J., Monard, L. A. G., Nishiyama, S., Papadakis, I., Street, R., Sumi, T., Williams, A., Yee, J. C., Brillant, S., Caldwell, J. A. R., Cole, A., Cook, K. H., Donatowicz, J., Kains, N., Kane, S. R., Martin, R., Pollard, K. R., Sahu, K. C., Tsapras, Y., Wambsganss, J., Zub, M., DePoy, D. L., Gaudi, B. S., Han, C., Lee, C. -U., Park, B. -G., Pogge, R. W., Kubiak, M., Szymanski, M. K., Pietrzynski, G., Soszynski, I., Szewczyk, O., Ulaczyk, K., Wyrzykowski, L., Abe, F., Fukui, A., Furusawa, K., Gilmore, A. C., Hearnshaw, J. B., Itow, Y., Kamiya, K., Kilmartin, P. M., Korpela, A. V., Lin, W., Ling, C. H., Masuda, K., Matsubara, Y., Miyake, N., Muraki, Y., Nagaya, M., Ohnishi, K., Okumura, T., Perrott, Y., Rattenbury, N. J., Saito, To., Sako, T., Sato, S., Skuljan, L., Sullivan, D., Sweatman, W., Tristram, P. J., Yock, P. C. M., Allan, A., Bode, M. F., Burgdorf, M. J., Clay, N., Fraser, S. N., Hawkins, E., Kerins, E., Lister, T. A., Mottram, C. J., Saunders, E. S., Snodgrass, C., Steele, I. A., Wheatley, P. J., Anguita, T., Bozza, V., Harpsoe, K., Hinse, T. C., Hundertmark, M., Kjaergaard, P., Liebig, C., Mancini, L., Masi, G., Rahvar, S., Ricci, D., Scarpetta, G., Southworth, J., Surdej, J., Thone, C. C., Riffeser, A., Seitz, S., Bender, R.

Gravitational microlensing is not only a successful tool for discovering distant exoplanets, but it also enables characterization of the lens and source stars involved in the lensing event. In high magnification events, the lens caustic may cross ove

Externí odkaz: http://arxiv.org/abs/1005.0966

The Automatic Real-Time GRB Pipeline of the 2-m Liverpool Telescope

Autor: Guidorzi, C., Monfardini, A., Gomboc, A., Mottram, C. J., Mundell, C. G., Steele, I. A., Carter, D., Bode, M. F., Smith, R. J., Fraser, S. N., Burgdorf, M. J., Newsam, A. M.

The 2-m Liverpool Telescope (LT), owned by Liverpool John Moores University, is located in La Palma (Canary Islands) and operates in fully robotic mode. In 2005, the LT began conducting an automatic GRB follow-up program. On receiving an automatic GR

Externí odkaz: http://arxiv.org/abs/astro-ph/0511032

Early GRB Optical and Infrared Afterglow Observations with the 2-m Robotic Liverpool Telescope

Autor: Gomboc, A., Mundell, C. G., Guidorzi, C., Monfardini, A., Mottram, C. J., Priddey, R., Smith, R. J., Pak, S., Steele, I. A., Tanvir, N., Carter, D., Fraser, S. N., Bode, M. F., Newsam, A. M., Hughes, M.

Publikováno v: Nuovo Cim.C28:723-726,2005

We present the first optical observations of a Gamma Ray Burst (GRB) afterglow using the 2-m robotic Liverpool Telescope (LT), which is owned and operated by Liverpool John Moores University and situated on La Palma. We briefly discuss the capabiliti

Externí odkaz: http://arxiv.org/abs/astro-ph/0502505

THE EXTREME MICROLENSING EVENT OGLE-2007-BLG-224: TERRESTRIAL PARALLAX OBSERVATION OF A THICK-DISK BROWN DWARF

Autor: Gould, A., Udalski, A., Monard, B., Horne, K., Dong, Subo, Miyake, N., Sahu, K., Bennett, D. P., Wyrzykowski, Ł., Soszyński, I., Szymański, M. K., Kubiak, M., Pietrzyński, G., Szewczyk, O., Ulaczyk, K., Allen, W., Christie, G. W., Depoy, D. L., Gaudi, B. S., Han, C., Lee, C.-U., Mccormick, J., Natusch, T., Park, B.-G., Pogge, R. W., Allan, A., Bode, M. F., Bramich, D. M., Burgdorf, M. J., Dominik, M., Fraser, S. N., Kerins, E., Mottram, C., Snodgrass, C., Steele, I. A., Street, R., Tsapras, Y., Abe, F., Bond, I. A., Botzler, C. S., Fukui, A., Furusawa, K., Hearnshaw, J. B., Itow, Y., Kamiya, K., Kilmartin, P. M., Korpela, A., Lin, W., Ling, C. H., Masuda, K., Matsubara, Y., Muraki, Y., Nagaya, M., Ohnishi, K., Okumura, T., Perrott, Y. C., Rattenbury, N., Saito, To., Sako, T., Skuljan, L., Sullivan, D. J., Sumi, T., Sweatman, W. L., Tristram, P. J., Yock, P. C. M., Albrow, M., Beaulieu, J. P., Coutures, C., Calitz, H., Caldwell, J., Fouqué, P., Martin, Roland, Williams, A.

Publikováno v: The Astrophysical journal letters
The Astrophysical journal letters, 2009, 698, pp.L147-L151. ⟨10.1088/0004-637X/698/2/L147⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2009, 698, pp.L147-L151. ⟨10.1088/0004-637X/698/2/L147⟩

Parallax is the most fundamental technique to measure distances to astronomical objects. Although terrestrial parallax was pioneered over 2000 years ago by Hipparchus (ca. 140 BCE) to measure the distance to the Moon, the baseline of the Earth is so

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e4b8b46e5aa0318a7d83c2fec9ae638c
https://doi.org/10.1088/0004-637x/698/2/l147

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