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.
Bibliographical reference

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

Advertised on:
2
2013
Number of authors
41
IAC number of authors
0
Citations
0
Refereed citations
0
Description
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).
Type
Non-refereed
Photometry

It may interest you

  • Non-refereed
    A Systematic Search for and Characterization of White Dwarf Binaries Across the H-R Diagram
    White dwarfs (WDs) are the endpoint of evolution for 97% of stars. Most of these stars are in multiple systems, and a significant fraction of those are compact enough to exchange mass, altering the structures and subsequent evolution of both stars. The physical mechanisms that facilitate these mass exchanges include common envelope evolution, Roche
    Anguiano, Borja et al.

    Advertised on:

    6
    2024
    Bibcode
    2024AAS...24410807A
    Citations
    0
  • Non-refereed
    ROSALIA: ROman Sky Analyst for Low surface brightness Imaging & Astronomy
    Diffuse emission in the outskirts of galaxies, such as stellar tidal streams, galaxy stellar halos and intracluster light, provides important constraints on the structure and evolution of the Universe. However, such low surface brightness diffuse emission can be up to thousands of times dimmer (>29 AB mag/[square arcseconds]) than the sky
    Laine, Seppo et al.

    Advertised on:

    6
    2024
    Bibcode
    2024AAS...24412902L
    Citations
    0
  • Non-refereed
    Deep HST Imaging Favors the Bulgeless Edge-on Galaxy Explanation for the Hypothetical Stellar Wake Created by a Runaway Supermassive Black Hole
    A long linear structure recently discovered could be the stellar wake produced by the passage of a runaway supermassive black hole (SMBH) or, alternatively, a bulgeless edge-on galaxy. We report on new very deep Hubble Space Telescope imaging that seems to be in tension with the SMBH runaway scenario but is consistent with the bulgeless edge-on
    Montes, Mireia et al.

    Advertised on:

    6
    2024
    Bibcode
    2024RNAAS...8..150M
    Citations
    0