Amelia Bayo

Paranal Observatory., FLAMES@UT2, Several Gaia-ESO runs


La Silla Observatory., EFOSC@NTT. Low resolution optical spec.


Support Astronomer at UT4 and UT3 (VLT/Paranal)., More than 230 nights experience.

Paranal Observatory., The nature of Subaru Planetary Mass Candidates in the 5 Myr
Col 69 cluster., VLT/UT1 with FORS2, an optical spectrograph and imaging camera, in
its multi-object spectroscopic mode.

Mauna Kea Observatory., The nature of Subaru Planetary Mass Candidates in the 5
Myr Col 69 cluster., 8.2m SUBARU telescope with IRCS, an infrared spectrograph and
imaging camera, in its spectroscopic mode.

Mauna Kea Observatory., The nature of Subaru Planetary Mass Candidates in the 5
Myr Col 69 cluster., 8.2m SUBARU telescope with IRCS, an infrared spectrograph and
imaging camera, in its spectroscopic mode.

La Silla Observatory., Dust settling: the luminosity function gap at M7M8., 3.6m NTT
telescope with SOFI, an infrared spectrograph and imaging camera, in its spectroscopic
mode.

CAHA., Lambda Orionis SFR: Membership & properties of SPITZER & BUSCA candiates.,
3.5m Telescope with TWIN, an optical spectrograph in its low resolution mode.

La Silla Observatory., Dust settling: the luminosity function gap at M7M8., 3.6m NTT
telescope with SOFI, an infrared spectrograph and imaging camera, in its spectroscopic
mode.

Observatorio del Roque de Los Muchachos (La Palma Canary Islands, Spain).,
Dust settling: the luminosity function gap at M7M8., Telescopio Nazionale Galileo
(3.6m) with NICS, a Near Infrared Camera Spectrometer, in its low resolution spectroscopic
mode.

Observatorio del Roque de Los Muchachos (La Palma Canary Islands, Spain).,
Exploring the differential IMF in the LOri SFR, Isaac Newton 2.5m Telescope with WFC,
an optical mosaic camera.

Calar Alto Observatory (CAHA)., Exploring the differential Initial Mass Functions in
the LOri SFR, 2.2m Telescope with BUSCA, a CCD camera system of simultaneous
direct imaging in 4 colors.