Spectroscopic survey
The WFI Halpha spectroscopic survey
... our spectroscopic survey of Hα emitters in galactic and SMC open clusters with the ESO Wide Field Imager in its slitless spectroscopic ...slitless spectroscopic mode, we performed a Hα ...
3
Spectroscopic Survey of X-type Asteroids
... ing to the mysterious X group, we have carried out a spectroscopic survey of these bodies in the visible and near infrared range at the 3.5m Telescopio Nazionale Galileo (TNG), in La Palma, Spain, at the ...
58
The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant
... producing spectroscopic target catalogues for massive spectroscopic surveys for cos- ...Oscillation Spectroscopic Survey (eBOSS), which will use ∼200 000 emission line galaxies (ELGs) at ...
20
The SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: final Emission Line Galaxy Target Selection
... Oscillation Spectroscopic Survey (eBOSS, 2014–2020, Dawson et ...Sky Survey (SDSS, York et ...Redshift Survey ( Colless et ...Oscillation Spectroscopic Survey (BOSS, 2008– 2014, ...
19
ARCS: the Asiago Red Clump Spectroscopic Survey
... Clump Spectroscopic survey derives from high resolution optical spectra accurate multi-epoch radial velocities and atmospheric parameters (T eff , log g, [M/H], V rot sin i, [α/Fe], ξ) for a well selected ...
2
A spectroscopic survey of faint, high-Galactic-latitude red clump stars. I. The high resolution sample
... this survey The afore mentioned, high-resolution spectroscopic surveys of RC stars generally focused only on atmospheric parameters or radial velocities, but not on both simultaneously, with the ex- ception ...
12
Spectroscopic survey of M-type asteroids
... scopic survey in the visible and near infrared wavelength range (0.4-2.5 µm) of 30 as- teroids chosen from the population of asteroids initially classified as Tholen M-types, aiming to investigate their surface ...
65
Spectroscopic survey of Kepler stars. I. HERMES/Mercator observations of A- and F-type stars
... ABSTRACT The Kepler space mission provided near-continuous and high-precision photometry of about 207,000 stars, which can be used for asteroseismology. However, for successful seismic modelling it is equally important ...
42
A spectroscopic survey of the WNL stars in the large magellanic cloud : general properties and binary status
... After summarizing the general importance of massive stars, we describe the spectroscopic observations of our program stars. We then detail the data analysis process, which encompasses ca[r] ...
234
A slitless spectroscopic survey for Halpha emission-line objects in SMC clusters
... 4.1.1. Astrometry and correlation with OGLE The ASTROM package (Wallace & Gray 2003) was ap- plied to the extracted spectra of the -1st order. Per WFI image, 30 to 80 astrometric reference stars from the GSC2.2 ...
58
The extended Baryon Oscillation Spectroscopic Survey: Variability selection and quasar luminosity function
... Key words. quasars: general – large-scale structure of Universe – surveys 1. Introduction Quasars have become a key ingredient in our understanding of cosmology and galaxy evolution. Since they are among the most ...
15
Chemical behavior of tungstate solutions. Part 1. A spectroscopic survey of the species involved
... decrease could be considered in aqueous solution: starting from the WO 4 2− ion (O/W = 4), the appearance of ions of the type W 2 O 7 2− (O/W = 3.5) could be thus expected in acidic conditions. Moreover, it should be ...
11
The XXL Survey
... 3. Methodology 3.1. Spatial density of optical galaxies Any excess of X-ray AGNs in the area of galaxy clusters can be due to the obvious abundance of galaxies with respect to the field (e.g. Koulouridis & Plionis ...
11
Sensing ruthenium tetroxide Emissions : a spectroscopic study
... Diagnostic tool of nuclear core degradation state Online quantification of released fission gas.. Improve the evaluation of environmental releases[r] ...
16
The XMM-LSS survey. Survey design and first results
... X-ray survey to systematically address LSS with clusters in the nearby universe (450 clusters with z ≤ ...a survey to yield some 800 clusters in two redshift bins with 0 < z < 1: the XMM Large Scale ...
35
Deriving biomedical diagnostics from NMR spectroscopic data
... / La version de cette publication peut être l’une des suivantes : la version prépublication de l’auteur, la version acceptée du manuscrit ou la version de l’éditeur. For the publisher’[r] ...
12
Bipolar Jets Produced By A Spectroscopic Binary
... Subject headings: binaries: spectroscopic – circumstellar matter – ISM: jets and outflows – stars: individual (KH 15D) 1. INTRODUCTION The models proposed for driving jets and outflows from young stars can be ...
7
The XXL Survey
... area. Such luminosities are missed by deep radio surveys such as COSMOS /VIDEO which usually cover much smaller areas. In Fig. 9 we compared our values and the literature 1.4 GHz luminosity functions for radio AGN with ...
12
Detecting cervical dysplasia with quantitative spectroscopic imaging
... Figure 6.1 shows spectroscopy parameters measured from HSIL and non-HSIL sites (determined by pathology) in the transformation zones of the LEEP patients. The medians of the [r] ...
150
The XXL Survey
... [0.5–2] keV band for point sources. This study is focussed on computing the fraction of star- forming and blue galaxies and the SFR–M ? relation, in the field versus clusters, also distinguishing between structures ...
23