[PDF] Top 20 Abundant serendipitous emission line sources with JWST/NIRSpec
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Abundant serendipitous emission line sources with JWST/NIRSpec
... of line fluxes (H α and [O III ]) based on the method presented in Section ...of NIRSpec as a function of wavelength for a spectrally unresolved point source centred in a 1 × 3 ...predicted line ... See full document
17
Simulating and interpreting deep observations in the Hubble Ultra Deep Field with the JWST/NIRSpec low-resolution `prism'
... on JWST/NIRCam imaging (Near Infrared Camera, Horner & Rieke 2004), this will provide researchers with unique data to constrain the physical processes driving the evolution of galaxies at z & 4, the ... See full document
20
Uncovering the Early Stages of Galaxy Evolution: Multi-Object Spectrometry with JWST/NIRSpec
... the JWST will be a large and cold telescope optimized for the infrared (Gardner et ...the JWST, the instrument that will enable multi-object slit spectroscopy (MOS) is ...Indeed, NIRSpec will be the ... See full document
5
All NIRspec Needs is HST/WFC3 Pre-Imaging? The Use of Milky Way Stars in WFC3 Imaging to Register NIRspec MSA Observations
... plan NIRspec / MSA observations based on catalogues from WFC3 or ACS imaging is being ...for NIRspec/MSA work, considering the strict astrometric accuracy ... See full document
17
Infrared molecular hydrogen lines in GRB host galaxies
... S(1) line will be in the MIRI spectral range for the entire known GRB red- shift distribution), and the molecular gas properties in the GRB host galaxies can be studied using multiple ...space-based JWST ... See full document
8
Detection of partially coherent optical emission sources
... without emission source) is multiplied by a factor to convert it to microns and is then displayed as the phase step ...no emission being present while the upper ones have an emission and background ... See full document
15
Imaging chemical differentiation around the low-mass protostar L483-mm
... line emission that can be directly compared to interferometer observations constraining the envelope structure down to scales of a few hundred AU ...unresolved emission, possibly originating in ... See full document
13
Space Telescope and Optical Reverberation Mapping Project. V. Optical Spectroscopic Campaign and Emission-line Analysis for NGC 5548
... derive emission-line lags because it is close in wavelength to the ionizing continuum and should therefore serve as an accurate ...broad- line lag if the BLR has a characteristic radius on the order ... See full document
21
Uptake of Chlorin e6 Photosensitizer by Polystyrene Diphenyloxazole Poly(N Isopropylacrylamide) Hybrid Nanosystem Studied by Electronic Excitation Energy Transfer
... fluorescent emission of PS-PPO-PNIPAM hybrid NS, and this quenching does enhance during about an hour ...donor emission at all emission wavelengths) or reabsorption (that would lead to the quenching ... See full document
7
Sirtuin1: serendipitous and enigmatic molecule
... Method validation and measurement of biomarker in non- clinical and clinical samples in drug development: a conference report.. Catharine Sturgeon, Robert Hill, Glen [r] ... See full document
9
THOR: The Hi, OH, Recombination line survey of the Milky Way: The pilot study: Hi observations of the giant molecular cloud W43
... i emission and absorption covers a large range of angu- lar scales, which is challenging for the data reduction, as the VLA C-Array filters out most of the large scale ... See full document
18
Space telescope and optical reverberation mapping project IV Anomalous behavior of the broad ultraviolet emission lines in NGC 5548
... broad emission lines from contaminating compo- nents and major advances in methods for recovering the emission line response function, these have facilitated improved dynamical mass estimates for ... See full document
10
Space telescope and optical reverberation mapping project I Ultraviolet observations of the Seyfert 1 galaxy NGC 5548 with the cosmic origins spectrograph on Hubble Space Telescope
... the line pro fi les because this inverse problem is degenerate, with a wide variety of simple velocity models providing satisfactory fi ts ( ...some sources ( ... See full document
15
Velocity resolved reverberation mapping of five bright Seyfert 1 galaxies
... anisotropic line emission, are subsumed into the con- stant f ...every emission line in a given AGN assuming similar ge- ometries and dynamics of the line-emitting ...multiple ... See full document
32
Optical emission lines in radio sources of intermediate power
... radio sources suffered from overresolution effects. All of these sources were am ong those observed only in th e A /B ...these sources because we do not have inform ation at low resolution from com ... See full document
418
Emission Inventory For Area Sources: Case Study For Workshop
... the emission is to create a data set of emission for environment relevant ...of emission for all industrial activities and also included non-industrial sectors such as agriculture, consumers, and ... See full document
24
A review: The physicochemical characteristics of indoor particulate matters in relation to human health
... Organic and elemental carbon (also called black carbon or soot) are the greatest fraction of air pollutant, which mainly derived from combustion process, almost up to 80% - 90% of ultrafine particulate mass [67]. ... See full document
9
The 6 7 keV Line Emission from the Stellar Flare of Algol
... The Suzaku off-line standard version 2.0 software and tools provided in High Energy Astrophysical Software (HEASoft; FTOOLS) version 6.10 software, which run on LINUX. XSELECT and XSPEC software packages which are ... See full document
8
Energy Scenario: Production, Consumption and Prospect of Renewable Energy in Australia
... Energy Production by Renewable Energy Sources Australia is not only gifted with abundant, high quality and diverse non-renewable energy sources but also has large, widely distributed ren[r] ... See full document
7
An ALMA survey of CO in submillimetre galaxies:companions, triggering, and the environment in blended sources
... and sources in our ...significant sources outside of the areas ...continuum sources (Section ...identified emission line sources (Section ...the sources (Table 1), so ... See full document
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