activity
20152019
most citedOxygen, α-element and iron abundance distributions in the inner part of the Galactic thin disc

50 citations · 69 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2019

O CAESAR: The Optical CAtalogue of Extragalactic SupernovA Remnants

I. Moumen, C. Robert, D. Devost +6

We present O CAESAR, the Optical CAtalogue of Extragalactic SupernovA Remnants. O CAESAR will provide the largest homogeneous optical survey of extragalactic SNR candidates taken b…

astro-ph.GA2019

Elemental abundances in the center of the Galactic Nuclear Disc

V. V. Kovtyukh, S. M. Andrievsky, R. P. Martin +5

We have made the first attempt to derive the chemical properties of the Galactic disc at its very central part using high-resolution infrared spectroscopic observations of four cla…

astro-ph.GA2019

SIGNALS: I. Survey Description

L. Rousseau-Nepton, R. P. Martin, C. Robert +60

SIGNALS, the Star formation, Ionized Gas, and Nebular Abundances Legacy Survey, is a large observing program designed to investigate massive star formation and HII regions in a sam…

astro-ph.GA201919 cited

3D Optical Spectroscopic Study of NGC3344 with SITELLE: I. Identification and Confirmation of Supernova Remnants

Ismael Moumen, Carmelle Robert, Daniel Devost +4

We present the first optical identification and confirmation of a sample of supernova remnants (SNRs) in the nearby galaxy NGC3344. Using high spectral and spatial resolution data,…

astro-ph.IM2018

SITELLE: An Imaging Fourier Transform Spectrometer for the Canada-France-Hawaii Telescope

Laurent Drissen, Thomas Martin, Laurie Rousseau-Nepton +11

We present an overview of SITELLE, an Imaging Fourier Transform Spectrometer (iFTS) available at the 3.6-meter Canada-France-Hawaii Telescope. SITELLE is a Michelson-type interfero…

astro-ph.GA201550 cited

Oxygen, α-element and iron abundance distributions in the inner part of the Galactic thin disc

R. P. Martin, S. M. Andrievsky, V. V. Kovtyukh +3

We derived elemental abundances in 27 Cepheids, the great majority situated within a zone of Galactocentric distances ranging from 5 to 7 kpc. One star of our sample, SU Sct, has a…