Spectroscopy and photometry data
The Carnegie Supernova Project I. Photometry data release of low-redshift stripped-envelope supernovae
... wavelength spectroscopy of this sample is presented and studied in detail in a third companion paper by Holmbo et ...NIR spectroscopy. These data will o ffer a new avenue to study helium and hydrogen ...
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Extensive Spectroscopy and Photometry of the Type IIP Supernova 2013ej
... Without data in all wavebands, it is generally impossible to obtain an exact bolometric ...of data spanning from UV to IR wavelengths for SN 2013ej gives an ideal opportunity to obtain the most accurate ...
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Understanding Planet Formation through High Precision Photometry and Spectroscopy
... measured. A precise telluric removal will provide higher fidelity data, which can be used to constrain molecular abundances as well as line shapes and further guide the disk modeling. 5.2.3 Areas of Continued ...
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Multiband photometry and spectroscopy of an all sky sample of bright white dwarfs
... 2.1 The reference catalogue: APASS APASS data release 9 (DR9; Henden et al. 2016) contains ≈ 61 million objects in the 10th–17th magnitude range. The sur- vey uses two pairs of 20-cm twin telescopes: two in the ...
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The SLUGGS Survey: Measuring globular cluster ages using both photometry and spectroscopy
... optical photometry with metallicity constraints from near-infrared spectroscopy in order to measure ...using data from the SAGES Legacy Unifying Globulars and GalaxieS (SLUGGS) ...
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Spectroscopy and multiband photometry of the afterglow of intermediate duration γ-ray burst GRB and its host galaxy ABSTRACT
... ground-based data from WHT and ...WHT data uncertainties, we perform differential photometry with re- spect to bright field stars present in all WHT epochs, and find brightening with 2 ...
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Photometry and spectroscopy of GRB 060526: A detailed study of the afterglow and host galaxy of a z = 3.2 gamma-ray burst
... Notes. The column densities were derived from CoG fitted for S ii , Si ii , Fe ii , C iv , Si iv and Al ii . Si ii* denotes a fine-structure line. Upper and lower limits were determined by assuming the ions to lie on the ...
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Characterization of low mass, wide separation substellar companions to stars in upper Scorpius : near infrared photometry and spectroscopy
... We reduced the data using custom IDL routines. First, we subtracted the exposures taken at two different nods in the slit to remove the majority of the background signal, resulting in parallel positive and ...
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The semicentennial binary system PSR J2032+4127 at periastron: X-ray photometry, optical spectroscopy, and SPH modelling
... 3.2 Spectral-type reassessment The original classification of MT91-213 was made from a low- resolution spectrum presented by Massey & Thompson ( 1991 ) in their fig. 11. They obtained a spectral type of B0V and noted ...
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The Sloan Digital Sky Survey Reverberation Mapping Project : Hα and Hβ reverberation measurements from first year spectroscopy and photometry
... Spectroscopic Data The SDSS-RM spectroscopic data utilized in this work were all acquired with the BOSS spectrograph between 2014 January and 2014 ...The data were processed by the SDSS-III pipeline ...
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Time resolved photometry and spectroscopy of the new deeply eclipsing SW Sextantis star HS 0728+6738
... optical spectroscopy and photometry, and far-ultraviolet spectroscopy of HS 0728+6738, a cataclysmic variable discovered in the Hamburg Quasar ...
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Conjugate-plane photometry: reducing scintillation in ground-based photometry
... Figure 15. Prototype of the conjugate-plane photometer that we are due to test on-sky shortly. a large fraction of the scintillation. Simulations show that the inten- sity variance can be reduced by an order of ...
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52. Profiling of various elements in Haloxylon griffithiiand Convolvulus leiocalycinus using atomic absorption spectroscopy and flame photometry
... Nine elements including essential and non-essential elements were evaluated in these plants among which the concentration of sodium and potassium were found to be higher [r] ...
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High performance computing of massive Astrometry and Photometry data from Gaia
... mission data set in time ...calibration data set. This step involves the combination of various data and the calculation (prediction) of the source location for the transits involved, ...
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Photometry of star clusters
... The methods used to study the focus problems and thermal properties of the Scott Lang Telescope were applied to the James Gregory Telescope during I 965 # The softness and complexity of[r] ...
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Advanced Modeling of Longitudinal Spectroscopy Data
... interaction) by including them as covariates in the model. However, this approach has its own limitation as discussed in Introduction section. Longitudinal trees (regression trees for longitudinal data) are ...
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Gaia photometry for white dwarfs
... Two di fferent behaviours were observed depending on the WD e ffective temperature. In the ’normal’ regime (T e ff > 5000 K) all WDs with the same composition (pure-H or pure- He) could be fitted by a single law to ...
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Atmospheric scintillation in astronomical photometry
... Accepted 2015 June 22. Received 2015 June 12; in original form 2015 May 15 A B S T R A C T Scintillation noise due to the Earth’s turbulent atmosphere can be a dominant noise source in high-precision astronomical ...
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Multicolour photometry of Mira variables
... UBVRI photometry of Mira variables was lacking, although a significant amount of UBV photometry had been carried out (Smak, 1966), and Mendosa V (1967) bad published some UBVRI* It was also thought that ...
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Photometry and kinematics of pure disk galaxies
... 42 the relative log (I) values quoted in the U.K. Schmidt Handbook for the two wedges were totally wrong. Fortunately, for many plates, we had either the North wedge and one of the KP spots pattern or the North wedge, ...
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