activity
19982026
most citedThe Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission

395 citations · 4.4k across the 78 of their papers we have counts for

collaborators
Showing 2016Show all

7 papers · 1 filter

astro-ph.GA2016★ 1 cited

Measuring Diffuse Interstellar Bands with cool stars. An improved line list to model the background stellar spectra

A. Monreal-Ibero, R. Lallement

DIBs are ubiquitous in stellar spectra. Traditionally, they have been studied through their extraction from hot stars, because of their smooth continuum. In an era where there are…

astro-ph.SR2016★ 14 cited

Stability of the interstellar hydrogen inflow longitude from 20 years of SOHO/SWAN observations

Dimitra Koutroumpa, Eric Quémerais, Olga Katushkina +3

Aims. A recent debate on the decade-long stability of the interstellar He flow vector, and in particular the flow longitude, has prompted us to check for any variability in the int…

astro-ph.HE2016★ 88 cited

The Structure of the Local Hot Bubble

W. Liu, M. Chiao, M. R. Collier +14

DXL (Diffuse X-rays from the Local Galaxy) is a sounding rocket mission designed to quantify and characterize the contribution of Solar Wind Charge eXchange (SWCX) to the Diffuse X…

astro-ph.GA2016★ 29 cited

On the distance to the North Polar Spur and the local CO-H2 factor

R. Lallement, S. Snowden, K. D. Kuntz +4

Most models identify the X-ray bright North Polar Spur (NPS) with a hot interstellar (IS) bubble in the Sco-Cen star-forming region at 130 pc. An opposite view considers th…

astro-ph.GA2016★ 25 cited

A catalog of 1.5273 micron diffuse interstellar bands based on APOGEE hot telluric calibrators

Meriem Elyajouri, Ana Monreal-Ibero, Quentin Remy +1

High resolution stellar spectroscopic surveys provide massive amounts of diffuse interstellar bands (DIBs) measurements. Data can be used to study the distribution of the DIB carri…

astro-ph.IM2016★ 31 cited

The Detailed Science Case for the Maunakea Spectroscopic Explorer: the Composition and Dynamics of the Faint Universe

Alan McConnachie, Carine Babusiaux, Michael Balogh +173

MSE is an 11.25m aperture observatory with a 1.5 square degree field of view that will be fully dedicated to multi-object spectroscopy. More than 3200 fibres will feed spectrograph…