Search results for "SPECTRA"

showing 10 items of 3542 documents

Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of LGRBs

2015

Aims: Long gamma-ray bursts (LGRBs) are associated with massive stars and are therefore linked to star formation. However, the conditions needed for the progenitor stars to produce LGRBs can affect the relation between the LGRB rate and star formation. By using the power of a complete LGRB sample, our long-term aim is to understand whether such a bias exists and, if it does, what its origin is. Methods: To reach our goal we use the Swift/BAT6 complete sample of LGRBs. In this first paper, we build the spectral energy distribution (SED) of the 14 z ⋆) from SED fitting. To investigate the presence of a bias in the LGRB-star formation relation we compare the stellar mass distribution of the LG…

Stellar massMetallicityAstrophysics::High Energy Astrophysical PhenomenaPopulationgamma-ray burst: generalAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicseducation010303 astronomy & astrophysicsQCAstrophysics::Galaxy AstrophysicsQBPhysicseducation.field_of_study010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsGalaxyStarsgalaxies: photometrySpace and Planetary Sciencegalaxies: star formationSpectral energy distributionAstrophysics::Earth and Planetary AstrophysicsGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Lyman break and ultraviolet-selected galaxies at z ~ 1 - II. PACS 100μm/160μm FIR detections

2013

In this work, we report the Photodetector Array Camera and Spectrometer (PACS) 100 μm/160 μm detections of a sample of 42 GALEX-selected and far-infrared (FIR)-detected Lyman break galaxies (LBGs) at z ~ 1 located in the Cosmic Evolution Survey (COSMOS) field and analyse their ultraviolet (UV) to FIR properties. The detection of these LBGs in the FIR indicates that they have a dust content high enough so that its emission can be directly detected. According to a spectral energy distribution (SED) fitting with stellar population templates to their UV-to-near-IR observed photometry, PACS-detected LBGs tend to be bigger (Reff ~ 4.1 kpc), more massive [log (M*/M⊙) ~ 10.7], dustier [Es(B - V) ~ …

Stellar populationAstrophysicsgalaxies [Radio continuum]medicine.disease_causestar formation [Galaxies]Physical cosmologyhigh-redshift [Galaxies]galaxies [Infrared]galaxies: high-redshiftmedicineLuminous infrared galaxyPhysicsStar formationinfrared: galaxieAstronomyAstronomy and Astrophysicsevolution [Galaxies]RedshiftGalaxygalaxies [Ultraviolet]Space and Planetary Sciencegalaxies: star formationultraviolet: galaxiesSpectral energy distributionradio continuum: galaxiegalaxies: evolutionUltraviolet
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The ALHAMBRA survey: 2D analysis of the stellar populations in massive early-type galaxies atz< 0.3

2017

Reproduced with permission from Astronomy & Astrophysics

Stellar populationMetallicityAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicselliptical and lenticular cD [Galaxies]01 natural sciencescDPhotometry (optics)0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsgalaxies: formationgalaxies: elliptical and lenticularSpectroscopy010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics[PHYS]Physics [physics]Physics010308 nuclear & particles physicsphotometry [Galaxies]FísicaAstronomy and Astrophysicsevolution [Galaxies]Astrophysics - Astrophysics of Galaxiesformation [Galaxies]Galaxy2d analysisEarly typeGalaxies: elliptical and lenticular cDgalaxies: photometrySpace and Planetary ScienceSpectral energy distributionAstrophysics::Earth and Planetary Astrophysicsgalaxies: evolution[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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<b>ANTIMICROBIAL DITERPENOID ALKALOIDS FROM <i>ERYTHROPHLEUM SUAVEOLENS</i> (GUILL. & PERR.) BRENAN</b>

2005

An investigation of the stem bark of Erythrophleum suaveolens (Guill. & Perr.) Brenan yielded the known amide norcassaide ( 1 ) and a new diterpenoid alkaloid named norerythrosuaveolide ( 2 ) which was characterized as 7β-hydroxy-7-deoxo-6-oxonorcassaide. The structures were established on the basis of one and two-dimensional 1 H and 13 C NMR spectral data. The compounds showed potent antimicrobial activities against bacteria and yeasts. KEY WORDS: Erythrophleum suaveolens (Guill. & Perr.) Brenan, Norcassaide, Diterpenoid alkaloid, Norerythrosuaveolide, Antimicrobial activities, Bacteria, Yeasts Bull. Chem. Soc. Ethiop. 2005, 19(2), 221-226.

Stem barkbiologyTraditional medicineChemistryStereochemistryErythrophleum suaveolensGeneral ChemistryAntimicrobialbiology.organism_classificationSpectral dataTerpenoidBulletin of the Chemical Society of Ethiopia
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Multinuclear magnetic resonance and x-ray diffraction studies of aminonitropyridines

1992

The 15N NMR spectra for 21 aminonitropyridines were measured and their chemical shifts assigned. The 1H and 13C NMR chemical shifts and spin–spin coupling constants were also determined for 16 compounds of this series. In order to relate the structural properties of nitramino groups and their 15N NMR chemical shifts in 2- and 4-nitramino-3-nitropyridines, which differ remarkably from all other amino groups studied, low-temperature 1H NMR, 17O NMR, comparative INEPT and IR spectroscopic studies were carried out. In addition, the x-ray crystal structure of 2-nitramino-3-nitropyridine was determined. Comparative spectroscopic studies showed that the nitramino derivatives exhibit different char…

StereochemistryCarbon-13 NMR satelliteChemical shiftGeneral ChemistryNuclear magnetic resonance spectroscopyCarbon-13 NMRTautomerNMR spectra databasechemistry.chemical_compoundCrystallographychemistryProton NMRGeneral Materials SciencePyridiniumMagnetic Resonance in Chemistry
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1H,13C and15N NMR spectroscopic, x-ray structural andab initio/HF studies on nitramino andN-alkylamino-4-nitro derivatives of pyridineN-oxides and py…

2003

The 1H, 13C and 15N NMR spectra in DMSO-d6 were measured for eight nitraminopyridine N-oxides, ten 4-nitropyridine N-oxides, four 2-nitraminopyridines and five 4-nitropyridines. Their chemical shift assignments are based on PFG 1H,X (X = 13C and 15N) HMQC and HMBC experiments. The relative energies for the tautomers of two nitraminopyridine N-oxides were determined by ab initio HF/6–311G** calculations. A single-crystal x-ray structural analysis was made for 4-methyl-2-nitraminopyridine: C6H7O2N3, M = 153.15, triclinic, space group P-1 (No. 2), a = 7.0275(4), b = 6.8034(3), c = 8.6086(5) A, α = 103.620(2), β = 90.309(2), γ = 122.215(3)°, V = 334.11(3) A3, Z = 2. Copyright © 2003 John Wiley …

StereochemistryChemical shiftAb initioGeneral ChemistryCarbon-13 NMRTriclinic crystal systemTautomerNMR spectra databasechemistry.chemical_compoundCrystallographychemistryPyridineProton NMRGeneral Materials ScienceMagnetic Resonance in Chemistry
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Nitramino, NRNO2 (R = H, CH3), as a substituent.13C and15N NMR spectroscopic study of nitraminobenzenes and -pyridines

1993

In order to clarify the special properties of the aryl-bound nitramino substituent NRNO 2 (R=H, CH 3 ), 13 C and 15 N NMR spectra of six nitraminobenzenes and nine nitraminopyridines were measured in DMSO-d 6 and their chemical shifts assigned. 1 H NMr chemical shifts and spin-spin coupling constants of all the compounds were also determined. In contrast to the behaviour of nitropyridines or -benzenes studied previously, most of the present compounds gave very broad 17 O NMR lines even at elevated temperatures and their 17 O NMR data were not useful for any reliable conclusions

StereochemistryChemical shiftSubstituentGeneral ChemistryNuclear magnetic resonance spectroscopyNmr dataMedicinal chemistryNMR spectra databasechemistry.chemical_compoundchemistryBenzene derivativesProton NMRNitroamineGeneral Materials ScienceMagnetic Resonance in Chemistry
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Specificity of 15N NMR chemical shifts to the nature of substituents and tautomerism in substituted pyridine N-oxides

2012

1H, 13C, and 15N NMR chemical shifts have been measured for 2-aminopyridine N-oxide (1), its eleven derivatives (2–10, 13, 14), and 3-Cl and 3-Br substituted 4-nitropyridine N-oxides (11, 12). δ(15N) of pyridine ring nitrogen in 2-acetylaminopyridine N-oxides are 5.9–11.5 ppm deshielded from those in 2-aminopyridine N-oxides. When amino and acetylamino substituents are in 4-position, δ(15N) of ring nitrogen is 21.3 ppm deshielded in the acetylated derivative. The strong resonance interaction between 2-amino and 5-nitro groups reflects in the decrease of amino nitrogen shielding about 5.3–17.9 ppm. Also, 1H and 13C NMR spectral data are in agreement with 15N NMR results reflected as deshield…

StereochemistryChemical shiftchemistry.chemical_elementCarbon-13 NMRCondensed Matter PhysicsRing (chemistry)Resonance (chemistry)NitrogenMedicinal chemistryTautomerchemistry.chemical_compoundchemistryPyridinePhysical and Theoretical ChemistrySpectral dataStructural Chemistry
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Neo-clerodane diterpenoids from Scutellaria lateriflora

1998

Abstract Three new diterpenoids, scutelaterins A-C, have been isolated from Scutellaria lateriflora and their structures established as (11S,13S,16S)-2β,6α,19-triacetoxy-4α,18;11,16;15,16-triepoxy-neo-clerod-14-ene (scutelaterin A), (11S,13S,16S)-6α,19-diacetoxy-2β-(2′-methyl)butyryloxy-4α,18;11,16;15,16-triepoxy-neo-clerod-14-ene (scutelaterin B) and (11S,13S,15R and S)-6α,19-diacetoxy-2β-(2′-methyl)butyryloxy-4α,18;11,16;15,16-triepoxy-neo-clerodan-15-ol (scutelaterin C) by chemical and spectroscopic means. In addition, the already known neo-clerodanes ajugapitin and scutecyprol A were also found in the same source.

StereochemistryChemical structurePlant ScienceGeneral MedicineNuclear magnetic resonance spectroscopyHorticultureBiologyBiochemistryTerpenoidchemistry.chemical_compoundchemistryOrganic chemistryMoleculeSpectral analysisScutellaria laterifloraDiterpeneMolecular BiologyPhytochemistry
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Synthesis and spectroscopic studies (Mo¨ssbauer, IR and NMR) of [R2SnCl2bipym] (R = butyl or phenyl) and the crystal and molecular structure of [Ph2S…

1994

Abstract The complexes [R 2 SnCl 2 bipym] (R = phenyl or butyl, bipym = 2,2′,6,6′-bipyrimidine) were synthesized and studied in solution by 1 H- and 13 C-NMR spectroscopy and in the solid state by IR and Mo¨ssbauer spectroscopy. The latter was also performed in frozen ethanolic solution. The structure of the phenyl complex was determined by single crystal diffraction methods. The value obtained for the angle C-SN-C in the phenyl compound is 169.3(2)° (X-ray) and 151° (Mo¨ssbauer), but the assignment of an octahedral configuration by Mo¨ssbauer spectroscopy is consistent with the structure determined by diffraction. The butyl complex is also octahedral and the two techniques show better agre…

StereochemistryChemistryCoordination numberOrganic ChemistryCrystal structureBiochemistryInorganic ChemistryCrystalNMR spectra databaseCrystallographyOctahedronX-ray crystallographyMaterials ChemistryMoleculePhysical and Theoretical ChemistrySpectroscopyJournal of Organometallic Chemistry
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