F-VIPGI: A new adapted version of VIPGI for FORS2 spectroscopy: Application to a sample of 16 X-ray selected galaxy clusters at 0.6 ≤ z ≤ 1.2

Astronomy and Astrophysics

Volumn 550, Issue , 2013, Pages

  Nastasi, A ^a   Scodeggio, M ^b   Fassbender, R ^a   Bohringer H ^a   Pierini, D ^d   Verdugo, M ^c   Garilli, B M ^b   Franzetti, P ^b  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b INAF IASF MILANO   (Italy)

^c UNIVERSITY OF VIENNA   (Austria)

^d NONE

Author keywords

Galaxies: clusters: general; Instrumentation: spectrographs; Methods: data analysis; Techniques: spectroscopic

Indexed keywords

CORE FUNCTIONS; ELECTRONIC FORMS; GALAXIES: CLUSTERS: GENERAL; GALAXY CLUSTERS; GALAXY EVOLUTION; GRAPHICAL INTERFACE; HIGH QUALITY; HIGH SIGNAL-TO-NOISE RATIO; HIGH-REDSHIFT; INSTRUMENTATION: SPECTROGRAPHS; LOCAL CLUSTER; LUMINOUS GALAXIES; METHODS:DATA ANALYSIS; OPTICAL SPECTRA; PHOTOMETRIC PROPERTIES; RED SHIFT; SPECTRAL INDICES; SPECTROSCOPIC DATA; STAR FORMING GALAXY; TECHNICAL INFORMATION; TECHNIQUES: SPECTROSCOPIC; XMM-NEWTON;

COMMUNICATION CHANNELS (INFORMATION THEORY); DATA REDUCTION; FADING (RADIO); LUMINANCE; PHOTOMETRY; PIPELINES; SPECTROSCOPIC ANALYSIS; X RAYS;

GALAXIES;

EID: 84872544109     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219862     Document Type: Article

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