The Future of Photometric, Spectrophotometric and Polarimetric Standardization

By G. Kleijn, R. Vermeij, E. Valentijn, K. Kuijken. 2007

450 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/d04509f1c451e5bbc0666dff10fbca5f4772b627

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Citations in the corpus

SPECTRA AND HUBBLE SPACE TELESCOPE LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511 < z < 1.12 AND THE UNION2 COMPILATION (2010, methodology): “The synthetic Vega magnitudes of the stars were calculated by multiplying the spectra and the Vega spectrum (Bohlin 2007) with the filter and instrument throughputs provided by the different observatories.”
SAGITTARIUS II, DRACO II AND LAEVENS 3: THREE NEW MILKY WAY SATELLITES DISCOVERED IN THE PAN-STARRS 1 3π SURVEY (2015, methodology): “Once the individual frames have been taken at Haleakala and downloaded from the summit, the photometry is generated through the Image Processing Pipeline (Magnier 2006, 2007; Magnier et al. 2008).”
Sweating the small stuff: simulating dwarf galaxies, ultra-faint dwarf galaxies, and their own tiny satellites (2015, background): “…near future, largearea, deep-sky surveys such as LSST, DES, PanSTARRS, and SkyMapper will push current detection limits to lower surface brightness and may be able to see ultra-faint satellites of isolated dwarf galaxies if they exist (Ivezic et al. 2008; Kaiser et al. 2002; Keller et al. 2007).”
The VAST Survey - III. The multiplicity of A-type stars within 75 pc (2013, unknown): “2in Gray 2007).”
Gaia broad band photometry (2010, background): “In that way,G =GBP=GRP=GRVS= V = 0.03 mag for a Vega-like 3 Bohlin & Gilliland (2004) give a value ofV = 0.026± 0.008 for the same flux at 555.6 nm, and Bohlin (2007) gives a revised value V = 0.023± 0.008 mag. star.”
SPECTROSCOPY OF THE LARGEST EVER γ-RAY-SELECTED BL LAC SAMPLE (2013, methodology): “We performed spectrophotometric calibration using standard stars from Oke (1990) and Bohlin (2007).”
COSMOLOGICAL CONSTRAINTS FROM MEASUREMENTS OF TYPE Ia SUPERNOVAE DISCOVERED DURING THE FIRST 1.5 yr OF THE Pan-STARRS1 SURVEY (2013, methodology): “However, even in space, complications like charge transfer efficiencies, non-linearity of detectors, and secular degradation of the optics and detectors contribute to systematic measurement biases (Bohlin 2007).”
MEASURING BARYON ACOUSTIC OSCILLATIONS ALONG THE LINE OF SIGHT WITH PHOTOMETRIC REDSHIFTS: THE PAU SURVEY (2008, background): “In terms of global photometry, it has now been shown that a homogeneous global relative calibration below 2%–3% accuracy is possible in current and future surveys (e.g., Sterken 2007 and references therein).”
The ATLAS All-Sky Stellar Reference Catalog (2018, methodology): “These data have been homogenized using an “ubercal” procedure (Padmanabhan et al. 2008; Schlafly et al. 2012) and tied to the Space Telescope Science Institute’s “Calspec” stars (Bohlin et al. 2001; Bohlin 2007, 2014).”
Fundamental properties of core-collapse Supernova and GRB progenitors: predicting the look of massive stars before death (2013, methodology): “We performed synthetic photometry of our SN progenitor models using the Chorizos code (Maíz-Apellániz 2004), adopting its built-in passband and zero point definitions that were obtained from Cohen et al. (2003); Maíz Apellániz (2006); Holberg & Bergeron (2006); Maíz-Apellániz (2007).”
A NEW FAINT MILKY WAY SATELLITE DISCOVERED IN THE PAN-STARRS1 3π SURVEY (2015, methodology): “A photometric catalogue is automatically generated with the Image Processing Pipeline (Magnier 2006, 2007; Magnier et al. 2008), once the individual frames have been downloaded from the summit.”
CARS: the CFHTLS-Archive-Research Survey. I. Five-band multi-colour data from 37 sq. deg. CFHTLS-wid (2008, background): “…absolute photometric calibration [determination of zeropoints, colour terms and extinction coefficients, corrections for scattered light effects which lead to significant inhomogeneous photometric zeropoints across the CCD mosaic (see e.g. Manfroid et al. 2001; Koch et al. 2004; Regnault 2007)].”
Synthetic stellar photometry – I. General considerations and new transformations for broad-band systems (2014, methodology): “The overall accuracy of this absolute flux is ∼ 1% (Bohlin 2007), which translates to about 0.01 mag in ZPζ .”
HERMES: a high-resolution fibre-fed spectrograph for the Mercator telescope (2010, methodology): “Presently, the data reduction pipeline works in a frame-per- frame mode, but the final goal is to execute a number of reduc- tion steps in a differential mode to gain robustness in the tempo- ral model of the spatial and wavelength geometry on the detector (Hensberge 2007).”
Evolution of asymptotic giant branch stars. II. Optical to far-infrared isochrones with improved TP- (2007, methodology): “We start discussing the LMC case depicted in the left panel.”