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Integral Field Spectroscopy of Planetary Nebulae with MUSE
J. R. Walsh, A. Monreal-Ibero
The Multi-Unit Spectroscopic Explorer (MUSE) is a large integral field unit mounted on the ESO Very Large Telescope. Its spatial (60 arcsecond field) and wavelength (4800-9300A) co…
An Imaging Spectroscopic Survey of the Planetary Nebula NGC 7009 with MUSE
J. R. Walsh, A. Monreal-Ibero, M. J. Barlow +6
The spatial structure of the emission lines and continuum over the 50 arcsecond extent of the nearby, O-rich, planetary nebula NGC 7009 (Saturn Nebula) have been observed with the…
A Two-Dimensional Spectroscopic Study of Emission Line Galaxies in the Faint Infrared Grism Survey (FIGS) I: Detection Method and Catalog
Norbert Pirzkal, Barry Rothberg, Russell E. Ryan +31
We present the results from the application of a two-dimensional emission line detection method, EMission-line two-Dimensional (EM2D), to the near-infrared G102 grism observations…
FIGS -- Faint Infrared Grism Survey: Description and Data Reduction
Norbert Pirzkal, Sangeeta Malhotra, Russell E. Ryan +26
The Faint Infrared Grism Survey (FIGS) is a deep Hubble Space Telescope (HST) WFC3/IR (Wide Field Camera 3 Infrared) slitless spectroscopic survey of four deep fields. Two fields a…
The Wolf-Rayet star population in the dwarf galaxy NGC 625
Ana Monreal-Ibero, Jeremy R. Walsh, Jorge Iglesias-Paramo +4
ABRIGED: Quantifying the number, type and distribution of W-R stars is a key component in the context of galaxy evolution, since they put constraints on the age of the star formati…
First results from Faint Infrared Grism Survey (FIGS): first simultaneous detection of Lyman-alpha emission and Lyman break from a galaxy at z=7.51
V. Tilvi, N. Pirzkal, S. Malhotra +22
Galaxies at high redshifts provide a valuable tool to study cosmic dawn, and therefore it is crucial to reliably identify these galaxies. Here, we present an unambiguous and first…