MASTER Follow-up Observations of LIGO GW170104 Event

Bibcode
2020RNAAS...4..211L
DOI
10.3847/2515-5172/abccc2
Lipunov, V.; Kornilov, V.; Gorbovskoy, E.; Vlasenko, D.; Tiurina, N.; Gress, O.; Gorbunov, I.; Balanutsa, P.; Pozdnyakov, A.; Buckley, D.; Podesta, R.; Rebolo, R.; Serra, M.; Balakin, F.; Chasovnikov, A.; Topolev, V.; Zhirkov, K.; Kuznetsov, A.; Vladimirov, V.; Senik, V.; Cheryasov, D.; Gabovich, A.; Zimnukhov, D.; Kuvshinov, D.; Podesta, F.; Francile, C.; Budnev, N.; Sergienko, Yu.; Tlatov, A.; Grinshpun, V.; Pogrosheva, T.; Shumkov, V.; Minkina, E.; Yurkov, V.
Referencia bibliográfica

Research Notes of the American Astronomical Society

Fecha de publicación:
11
2020
Número de autores
34
Número de autores del IAC
2
Número de citas
1
Número de citas referidas
1
Descripción
We present the results of MASTER Global Robotic Net optical observations of the LIGO GW170104 error-box during the LIGO/Virgo O2 run. We observed 3421 square degrees inside 3σ error-field. Dozens of optical transients unrelated to gravitational waves were discovered as the result of MASTER observation strategy, that we presented, including short very bright MASTER optical transients J133017.28+780951.8.
Tipo
Sin árbitro
Astronomía de ondas gravitacionales
Cartografiados del cielo
Telescopio automáticos de patrulla
LIGO

Te puede interesar

  • Sin árbitro
    Massive characterisation of subgiants and red giants with TESS (Kepler and Gaia)
    TESS serves as a formidable tool for investigating stellar variability. Nonetheless, the adaptation of methodologies employed in other space missions, such as Kepler, to deduce long stellar rotation periods or solar-like stellar pulsations has been a challenge. The advent of multiple sectors of data for most stars every two years with the extended
    García, Rafael A. et al.

    Fecha de publicación:

    9
    2024
    Bibcode
    2024tkas.confE.123G
    Número de citas
    0
  • Sin árbitro
    Calibrating the color-redshift relation for an optimum exploitation of Euclid data
    Euclid's three dimensional reconstruction of the matter distribution in the Universe heavily relies on a proper calibration of the color-redshift relation. Getting such calibration was the motivation of the project Complete Calibration of the Color-Redshift Relation (C3R2) survey (Masters et al. 2017), with the goal of mapping the empirical
    Gutierrez, Carlos

    Fecha de publicación:

    8
    2024
    Bibcode
    2024IAUGA..32P2796G
    Número de citas
    0
  • Sin árbitro
    Gas Flows in the Central Region of NGC 4593 with Muse
    Understanding how gas flows into galactic centers, fuels the AGN and in turn is expelled back through feedback processes is of great importance to appreciate the role AGN play in the growth and evolution of galaxies. We use MUSE-AO optical spectra of the inner 7''. 5 × 7''. 5 of the nearby Seyfert 1 galaxy NGC 4593 to understand how gas flows in
    Mulumba, Dorcus et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024IAUGA..32P.367M
    Número de citas
    0