Red noise versus planetary interpretations in the microlensing event OGLE-2013-BLG-446

Autor: Bachelet, E., Bramich, D. M., Han, C., Greenhill, J., Street, R. A., Gould, A., Ago, G. D, AlSubai, K., Dominik, M., Jaimes, R. Figuera, Horne, K., Hundertmark, M., Kains, N., Snodgrass, C., Steele, I. A., Tsapras, Y., Albrow, M. D., Batista, V., Beaulieu, J. -P., Bennett, D. P., Brillant, S., Caldwell, J. A. R., Cassan, A., Cole, A., Coutures, C., Dieters, S., Prester, D. Dominis, Donatowicz, J., Fouque, P., Hill, K., Marquette, J. -B., Menzies, J., Pere, C., Ranc, C., Wambsganss, J., Warren, D., de Almeida, L. Andrade, Choi, J. -Y., DePoy, D. L., Dong, Subo, Hung, L. -W., Hwang, K. H., Jablonski, F., Jung, Y. K., Kaspi, S., Klein, N., Lee, C. -U., Maoz, D., Munoz, J. A., Nataf, D., Park, H., Pogge, R. W., Polishook, D., Shin, I. -G., Shporer, A., Abe, J. C. Yee F., Bhattacharya, A., Bond, I. A., Botzler, C. S., Freeman, M., Fukui, A., Itow, Y., Koshimoto, N., Ling, C. H., Masuda, K., Matsubara, Y., Muraki, Y., Ohnishi, K., Philpott, L. C., Rattenbury, N., Saito, To., Sullivan, D. J., Sumi, T., Suzuki, D., Tristram, J., Yonehara, A., Bozza, V., Novati, S. Calchi, Ciceri, S., Galianni, P., Gu, S. H., Harpsoe, K., Hinse, T. C., Jorgensen, U. G., Juncher, D., Korhonen, H., Mancini, L., Melchiorre, C., Popovas, A., Postiglione, A., Rabus, M., Rahvar, S., Schmidt, R. W., Scarpetta, G., Skottfelt, J., Southworth, John, Stabile, An., Surdej, J., Wang, X. -B., Wertz, O.

For all exoplanet candidates, the reliability of a claimed detection needs to be assessed through a careful study of systematic errors in the data to minimize the false positives rate. We present a method to investigate such systematics in microlensi

Externí odkaz: http://arxiv.org/abs/1510.02724

Variability of the Brunt–Väisälä frequency at the OH∗-airglow layer height at low and midlatitudes

Autor: S. Wüst, M. Bittner, J.-H. Yee, M. G. Mlynczak, J. M. Russell III

Publikováno v: Atmospheric Measurement Techniques, Vol 13, Pp 6067-6093 (2020)

Airglow spectrometers, as they are operated within the Network for the Detection of Mesospheric Change (NDMC; https://ndmc.dlr.de, last access: 1 November 2020), for example, allow the derivation of rotational temperatures which are equivalent to the

Externí odkaz: https://doaj.org/article/a2b130568bf64f00a5cdc798d86375d6

Radiometric Stability of the SABER Instrument

Autor: Martin G. Mlynczak, Taumi Daniels, Linda A. Hunt, Jia Yue, B. Thomas Marshall, James M. Russell III, Ellis E. Remsberg, Joseph Tansock, Roy Esplin, Mark Jensen, Andrew Shumway, Larry Gordley, J.‐H. Yee

Publikováno v: Earth and Space Science, Vol 7, Iss 2, Pp n/a-n/a (2020)

Abstract The SABER instrument on the National Aeronautics and Space Administration Thermosphere‐Ionosphere‐Mesosphere Energetics and Dynamics satellite continues to provide a long‐term record of Earth's stratosphere, mesosphere, and lower therm

Externí odkaz: https://doaj.org/article/74db548441584da99a473d8dd1dd974f

Variability of the Brunt–Väisälä frequency at the OH* layer height

Autor: S. Wüst, M. Bittner, J.-H. Yee, M. G. Mlynczak, J. M. Russell III

Publikováno v: Atmospheric Measurement Techniques, Vol 10, Pp 4895-4903 (2017)

In and near the Alpine region, the most dense subnetwork of identical NDMC (Network for the Detection of Mesospheric Change, https://www.wdc.dlr.de/ndmc/) instruments can be found: five stations are equipped with OH* spectrometers which deliver a

Externí odkaz: https://doaj.org/article/7f5ae57a018b49cf97855d86ed21dd55

Mesosphere and lower thermosphere temperature anomalies during the 2002 Antarctic stratospheric warming event

Autor: S. M. I. Azeem, E. R. Talaat, G. G. Sivjee, J.-H. Yee

Publikováno v: Annales Geophysicae, Vol 28, Pp 267-276 (2010)

We present kinetic temperatures at ~87 km and ~94 km altitudes inferred from OH (6,2) and O2 At(0,1) airglow observations, respectively, at South Pole (90° S), Antarctica in the austral winter of 2002. These OH and O2 rotational temperatures meas

Externí odkaz: https://doaj.org/article/95420da7d801469bb19ae665c5405789