Multi-site obs. of WASP-12 b transit (Maciejewski+, 2013)

Bibcode
2013yCat..35519108M
Maciejewski, G.; Dimitrov, D.; Seeliger, M.; Raetz, St.; Bukowiecki, L.; Kitze, M.; Errmann, R.; Nowak, G.; Niedzielski, A.; Popov, V.; Marka, C.; Gozdziewski, K.; Neuhaeuser, R.; Ohlert, J.; Hinse, T. C.; Lee, J. W.; Lee, C.-U.; Yoon, J.-N.; Berndt, A.; Gilbert, H.; Ginski, C.; Hohle, M. M.; Mugrauer, M.; Roll, T.; Schmidt, T. O. B.; Tetzlaff, N.; Mancini, L.; Southworth, J.; Dall'Ora, M.; Ciceri, S.; Zambelli, R.; Corfini, G.; Takahashi, H.; Tachihara, K.; Benko, J. M.; Sarneczky, K.; Szabo, Gy. M.; Varga, T. N.; Vanko, M.; Joshi, Y. C.; Chen, W. P.
Referencia bibliográfica

VizieR On-line Data Catalog: J/A+A/551/A108. Originally published in: 2013A&A...551A.108M

Fecha de publicación:
2
2013
Número de autores
41
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
Light curves for sixty WASP-12 b's transits observed in 2010-2012 are given. Data were collected with 0.5-2.6-m telescopes located in thirteen observatories distributed around the world. Details on observations, data reduction, and analysis are given in the source paper. (1 data file).
Tipo
Sin árbitro
Fotometría

Te puede interesar

  • Sin árbitro
    HARMONI at ELT: HIPOTEC electronics and control system
    HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 470nm to 2450nm with resolving powers from 3300 to 18000 and spatial sampling from 60 mas to 4 mas. It can operate in two Adaptive Optics modes - SCAO (including a High Contrast capability) and LTAO - or with NOAO. The
    Menéndez Mendoza, Saúl et al.

    Fecha de publicación:

    7
    2024
    Bibcode
    2024SPIE13096E..4ZM
    Número de citas
    0
  • Sin árbitro
    GTCAO low-frequency tip-tilt offload to M2
    GTCAO is the instrument that implements Adaptive Optics on GTC. For atmospheric turbulence correction, GTCAO uses a deformable mirror. Unlike other AO systems, GTCAO does not include a dedicated mirror for low-frequency tip-tilt (TT) correction. In the absence of dedicated correction, the TT components of atmospheric turbulence are corrected by the
    Marco de la Rosa, J. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13097E..7SM
    Número de citas
    0