The Hubble Space Telescope Advanced Camera for Surveys

By H. C. Ford. 2000

858 citations recorded by the source corpus.

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Citations in the corpus

The Multiplicity of the Subgiant Branch of ω Centauri: Evidence for Prolonged Star Formation (2007, methodology): “We measured the F435W magnitudes and F435W F625W colors of their turnoffs in our ACS photometry and used equation (12) of Sirianni et al. (2005), with coefficients taken from their Table 22, to derive the V magnitudes of the two turnoffs.”
THE STRUCTURE OF CLASSICAL BULGES AND PSEUDOBULGES: THE LINK BETWEEN PSEUDOBULGES AND SÉRSIC INDEX (2008, methodology): “We calculate JohnsonV-band magnitude zero points using the transformations in Holtzman et al. (1995) for the WFPC2 images and Sirianni et al. (2005) for the ACS images.”
The ACS Survey of Galactic Globular Clusters. III. The Double Subgiant Branch of NGC 1851 (2007, methodology): “We put the WFC photometry into the VEGAMAG system following the procedures in Bedin et al. (2005), and adopting the encircled energy and zero points as given by Sirianni et al. (2005).”
Advanced Camera for Surveys Imaging of 25 Galaxies in Nearby Groups and in the Field (2005, methodology): “Charge transfer efficiency corrections were made according to Reiss (2003), and our zero points and transformations were made according to Sirianni et al. (2005).”
Leo A: A Late-blooming Survivor of the Epoch of Reionization in the Local Group (2007, methodology): “Extinction in the ACS/WFC filter system was obtained by interpolation within the tables of Sirianni et al. (2005): A814 = 0.039, A475 = 0.078.”
UV LUMINOSITY FUNCTIONS AT REDSHIFTS z ∼ 4 TO z ∼ 10: 10,000 GALAXIES FROM HST LEGACY FIELDS (2014, methodology): “Second, we correct for the light outside the large scalable aperture and on the wings of the PSF using the standard encircled energy distributions for point sources tabulated in Dressel (2013) or Sirianni et al. (2005).”
THE QUENCHING OF THE ULTRA-FAINT DWARF GALAXIES IN THE REIONIZATION ERA (2014, methodology): “Transformation from theHST photometric system to a ground-based system incurs significant systematic errors,as explored by Sirianni et al. (2005).”
Discovery of a Ringlike Dark Matter Structure in the Core of the Galaxy Cluster Cl 0024+17 (2007, methodology): “The postlaunch sensitivity curves of ACS by Sirianni et al. (2005) are used to obtain synthetic photometry of these templates from z ¼ 0:01 to 6 at a redshift interval of z ¼ 0:01.”
A Triple Main Sequence in the Globular Cluster NGC 2808 (2007, methodology): “The photometry was put into the WFC/ACS Vega-mag system according to the proce- dure given in Bedin et al. (2005), and using the encircled energy and zero points given by Sirianni et al. (2005).”
Multiple Stellar Populations in Three Rich Large Magellanic Cloud Star Clusters (2008, background): “…dolphot accounts for the hotpixel and cosmic-ray masking information provided with each flat-fielded image, fits the sky locally around each detected source, and provides magnitudes corrected for charge-transfer efficiency (CTE) effects on the calibrated VEGAMAG scale of Sirianni et al. (2005).”
Multiple stellar populations in Magellanic Cloud clusters - I. An ordinary feature for intermediate age globulars in the LMC? (2008, methodology): “Calibration of ACS photometry into the Vega-mag system was performed following recipes in Bedin et al. (2005) and using the zero points given in Sirianni et al. (2005).”
The ACS Survey of Galactic Globular Clusters. II. Stellar Evolution Tracks, Isochrones, Luminosity Functions, and Synthetic Horizontal-Branch Models (2007, methodology): “One is based on the semi-empirical colors and bolometric corrections of Vandenberg & Clem (2003) and the transformation equations found in Appendix D of Sirianni et al. (2005), specifically those in Tables 22 and 24, hereafter referred to as the Empirical transformation.”
THE ACS SURVEY OF GALACTIC GLOBULAR CLUSTERS. IX. HORIZONTAL BRANCH MORPHOLOGY AND THE SECOND PARAMETER PHENOMENON (2009, methodology): “…reduction and calibration are provided in Paper V but, since its publication, the data have been adjusted to account for updated HST/ACS Wide Field Channel zero points (Bohlin 2007); the new F606W and F814W zero points are, respectively, 22 and 35 mmag fainter than given by Sirianni et al. (2005).”
The ACS Virgo Cluster Survey. XII. The Luminosity Function of Globular Clusters in Early-Type Galaxies (2007, methodology): “Photometric zeropoints are taken from Sirianni et al. 2005 (see also Jordán et al. 2004a), and aperture corrections are applied as described by Jordán et al. (2007, in preparation).”
Scaled solar tracks and isochrones in a large region of the Z-Y plane. II. From 2.5 to 20 solar masses (2009, methodology): “The present isochrones are provided in the Johnson-CousinsGlass system as defined by Bessell (1990) and Bessell & Brett (1988), in the Vegamag systems of ACS onboard HST (cf. Sirianni et al. 2005), and in the SDSS system.”
UV Luminosity Functions at z~4, 5, and 6 from the Hubble Ultra Deep Field and Other Deep Hubble Space Telescope ACS Fields: Evolution and Star Formation History (2007, background): “We believe this offset is the result of the ∼ 0.1 mag correction we make for light on the PSF wings (Sirianni et al. 2005).”
The All-Wavelength Extended Groth Strip International Survey (AEGIS) Data Sets (2006, methodology): “These detection maps and the ACS zeropoints (Sirianni et al. 2005) were applied to each band separately to create the ACS photometric catalogs.”