Luminosity Functions of 10 Nearby Clusters of Galaxies. I. Data

By M. Yagi, N. Kashikawa, M. Sekiguchi, M. Doi, N. Yasuda, K. Shimasaku, S. Okamura. 2002

209 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Electrical and Electronic Engineering

View Paper: https://www.semanticscholar.org/paper/6aa5493d6c40f512dfedcc91e79cb99e9701c1c4

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Citations in the corpus

A large Hα survey at z = 2.23, 1.47, 0.84 and 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS (2012, methodology): “In brief, all the raw NB921 data were reduced with the Suprime-Cam Deep field REDuction package (SDFRED, Yagi et al. 2002; Ouchi et al. 2004) and IRAF.”
Star formation at z=1.47 from HiZELS: an Hα+[O ii] double-blind study* (2011, methodology): “The raw NB921 data were downloaded from the archive and reduced with the Suprime-Cam Deep field Reduction (SDFRED) package (Yagi et al. 2002; Ouchi et al. 2004) and IRAF.”
STATISTICS OF 207 Lyα EMITTERS AT A REDSHIFT NEAR 7: CONSTRAINTS ON REIONIZATION AND GALAXY FORMATION MODELS (2010, methodology): “The narrow-band data are reduced with the Suprime-Cam Deep field REDuction package (SDFRED; Yagi et al. 2002; Ouchi et al. 2004a).”
The Discovery of Two Lyman α Emitters beyond Redshift 6 in the Subaru Deep Field (2003, methodology): “The data reduction procedures are the same as those given in Yagi et al. (2002).”
HUBBLE FRONTIER FIELDS FIRST COMPLETE CLUSTER DATA: FAINT GALAXIES AT z ∼ 5–10 FOR UV LUMINOSITY FUNCTIONS AND COSMIC REIONIZATION (2014, unknown): “′′4-diameter circular aperture using sdfred (Yagi et al. 2002; Ouchi et al. 2004).”
Subaru Weak Lensing Study of Seven Merging Clusters: Distributions of Mass and Baryons (2007, methodology): “Each Subaru data set was reduced using the software SDFRED (Yagi et al. 2002; Ouchi et al. 2004).”
Large-Scale Structure of Emission-Line Galaxies at z = 3.1 (2004, methodology): “The data were reduced using IRAF and the mosaicCCD data reduction software developed by Yagi et al. (2002).”
Combined strong and weak lensing analysis of 28 clusters from the Sloan Giant Arcs Survey (2011, methodology): “The data are reduced using SDFRED and SDFRED2 (Yagi et al. 2002; Ouchi et al. 2004).”
The SUBARU Deep Field Project: Lymanα Emitters at a Redshift of 6.6 (2004, methodology): “The individual CCD data were reduced and combined using both our own data-reduction software (Yagi et al. 2002) and IRAF.”
LARGE AREA SURVEY FOR z = 7 GALAXIES IN SDF AND GOODS-N: IMPLICATIONS FOR GALAXY FORMATION AND COSMIC REIONIZATION (2009, methodology): “Our data were reduced using Suprime-cam Deep Field REDuction package (SDFRED; Yagi et al. 2002; Ouchi et al. 2004a).”
THE MULTIWAVELENGTH SURVEY BY YALE–CHILE (MUSYC): DEEP MEDIUM-BAND OPTICAL IMAGING AND HIGH-QUALITY 32-BAND PHOTOMETRIC REDSHIFTS IN THE ECDF-S (2010, methodology): “The data were reduced using a combination of standard IRAF14 tasks; sdfred, a data reduction and analysis software package written for Suprime Cam (Yagi et al. 2002; Ouchi et al. 2004); and custom tasks.”
The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lyα Emitters from z = 3.1 to 5.7 in the 1 deg2 Field: Luminosity Functions and AGN (2007, methodology): “The narrowband data are reducedwith the SuprimeCam Deep Field Reduction package (SDFRED; Yagi et al. 2002; Ouchi et al. 2004a).”
LoCuSS: Subaru Weak Lensing Study of 30 Galaxy Clusters (2009, methodology): “Briefly, the standard pipeline reduction software for Suprime-Cam, SDFRED (Yagi et al. 2002; Ouchi et al. 2004), was used for flatfielding, instrumental distortion correction, differential refraction, PSF matching, sky subtraction, and stacking.”
The Subaru/XMM-Newton Deep Survey (SXDS). II. Optical Imaging and Photometric Catalogs (2008, methodology): “This pipeline is based on a software package developed for SuprimeCam data reduction (Yagi et al. 2002) and several IRAF tasks (geomap, geotran, etc.) are used in the process of a geometrical transformation and alignment of final stacked images.”
Total Galaxy Magnitudes and Effective Radii from Petrosian Magnitudes and Radii (2005, background): “…Petrosian index has experienced a resurgence (e.g., Wirth, Koo, & Kron 1994; Bershady, Lowenthal, & Koo 1998; Dalcanton 1998; Takamiya 1999; Bershady et al. 2000; Volonteri, Saracco, & Chincarini 2000; Blanton et al. 2001; Lubin & Sandage 2001; Conselice, Gallagher, & Wyse 2002; Yagi et al. 2002).”
Reionization and Galaxy Evolution Probed by z = 7 Lyα Emitters (2007, methodology): “We have reduced NB973 image frames using the software SDFRED (Ouchi et al. 2004; Yagi et al. 2002) in the same manner as in Kashikawa et al. (2004).”
A DOZEN NEW GALAXIES CAUGHT IN THE ACT: GAS STRIPPING AND EXTENDED EMISSION LINE REGIONS IN THE COMA CLUSTER (2010, methodology): “Overscan subtraction, flat-fielding, distortion correction, background subtraction and mosaicing were performed using another implementation (nekosoft; Yagi et al. 2002) of the standard Suprime-Cam reduction software.”
A Subaru Search for Lyα Blobs in and around the Protocluster Region At Redshift z = 3.1 (2004, methodology): “The raw data are the same as presented in H04 and were reduced with IRAF and a custom software developed for Suprime-Cam data reduction (Yagi et al. 2002; Ouchi et al. 2003) in a manner similar to that presented in H04.”
Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample (2002, unknown): “See Yagi et al. (2002) for a similar discussion.”