# LOCAL u'g'r'i'z' STANDARD STARS IN THE CHANDRA DEEP FIELD SOUTH

@article{Smith2003LOCALUS,
title={LOCAL u'g'r'i'z' STANDARD STARS IN THE CHANDRA DEEP FIELD SOUTH},
author={Julian A. Smith and Douglas L. Tucker and Sahar Allam and Christopher Thomas Rodgers},
journal={The Astronomical Journal},
year={2003},
volume={126},
pages={2037-2047}
}
Because several observing programs are under way in various spectral regimes to explore the Chandra Deep Field South (CDF-S), the value of local photometric standards is obvious. As part of an NOAO Survey Program to establish u'g'r'i'z' standard stars in the southern hemisphere, we have observed the central region of the CDF-S to create local standards for use by other investigators using these filters. As a courtesy, we present the CDF-S standards to the public now, although the main program… Expand
A Survey of Open Clusters in the u′g′r′i′z′ Filter System. III. Results for the Cluster NGC 188
• Physics
• 2007
The authors continue the series of papers describing the results of a photometric survey of open star clusters, primarily in the southern hemisphere, taken in the u'g'r'i'z' filter system. The entireExpand
A Survey of Open Clusters in the u′g′r′i′z′ Filter System. I. Results for NGC 2548 (M48)
• Physics
• 2004
We present initial results of a photometric survey of open star clusters, primarily in the southern hemisphere, taken in the u'g'r'i'z' filter system. While our entire observed sample covers moreExpand
Absolute Flux Calibration of the IRAC Instrument on the Spitzer Space Telescope using Hubble Space Telescope Flux Standards
The absolute flux calibration of the James Webb Space Telescope (JWST) will be based on a set of stars observed by the Hubble and Spitzer Space Telescopes. In order to cross-calibrate the twoExpand
Post-merger Signatures of Red-sequence Galaxies in Rich Abell Clusters at $z\lesssim 0.1$
• Physics
• 2012
We have investigated the post-merger signatures of red-sequence galaxies in rich Abell clusters at $z \lesssim$ 0.1: A119, A2670, A3330 and A389. Deep images in u', g', r' and medium-resolutionExpand
GALAXY LUMINOSITY FUNCTION OF THE DYNAMICALLY YOUNG ABELL 119 CLUSTER: PROBING THE CLUSTER ASSEMBLY
• Physics
• 2016
We present the galaxy luminosity function (LF) of the Abell 119 cluster down to $M_r\sim-14$ mag based on deep images in the $u$-, $g$-, and $r$-bands taken by using MOSAIC II CCD mounted on theExpand
STELLAR LOCUS REGRESSION: ACCURATE COLOR CALIBRATION AND THE REAL-TIME DETERMINATION OF GALAXY CLUSTER PHOTOMETRIC REDSHIFTS
• Physics
• 2009
We present Stellar Locus Regression (SLR), a method of directly adjusting the instrumental broadband optical colors of stars to bring them into accord with a universal stellar color-color locus,Expand
The 2.5 m Telescope of the Sloan Digital Sky Survey
• Physics
• 2006
We describe the design, construction, and performance of the Sloan Digital Sky Survey telescope located at Apache Point Observatory. The telescope is a modified two-corrector Ritchey-Chretien designExpand
The Sloan Digital Sky Survey monitor telescope pipeline
The photometric calibration of the Sloan Digital Sky Survey (SDSS) is a multi-step process which involves data from three different telescopes: the 1.0-m telescope at the US Naval Observatory (USNO),Expand

#### References

SHOWING 1-10 OF 17 REFERENCES
H-band observations of the Chandra Deep Field South ?
• Physics
• 2003
We report results of our H-band survey of the Chandra Deep Field South (CDFS). The observations, made with SofI on the NTT, cover 0.027 square degrees to H < 20.5 and 0.17 square degrees to H < 19.8Expand
Deep BVR photometry of the Chandra Deep Field South from the COMBO-17 survey
• Physics
• 2001
We report on deep multi-color imaging ($R_{5\sigma} = 26$) of the Chandra Deep Field South, obtained with the Wide Field Imager (WFI) at the MPG/ESO 2.2 m telescope on La Silla as part of theExpand
Chandra Deep Field South: The 1 Ms Catalog
In this paper we present the source catalog obtained from a 942 ks exposure of the Chandra Deep Field South (CDFS), using the Advanced CCD Imaging Spectrometer (ACIS-I) on the Chandra X-rayExpand
First Results from the X-Ray and Optical Survey of the Chandra Deep Field South
We present our first results from 120 ks of X-ray observations obtained with the Advanced CCD Imaging Spectrometer on the Chandra X-Ray Observatory. The field of the two combined exposures is 0.096Expand
ESO Imaging Survey. The stellar catalogue in the Chandra deep field south
Stellar catalogues in five passbands ( UBVRI ) over an area of approximately 0.3 deg 2 , comprising about 1200 objects, and in seven passbands ( UBVRIJK ) over approximately 0.1 deg 2 , comprisingExpand
The Chandra Deep Field-South: The 1 Million Second Exposure*
We present the main results from our 940 ks observation of the Chandra Deep Field-South using the source catalog described in an accompanying paper by Giacconi et al. We extend the measurement ofExpand
The Great Observatories Origins Deep Survey
The Great Observatories Origins Deep Survey (GOODS) is designed to gather the best and deepest multiwavelength data for studying the formation and evolution of galaxies and active galactic nuclei,Expand
The Sloan Digital Sky Survey: Technical summary
• Physics
• 2000
The Sloan Digital Sky Survey (SDSS) will provide the data to support detailed investigations of the distribution of luminous and nonluminous matter in the universe: a photometrically andExpand
ESO imaging survey - Deep public survey: Multi-color optical data for the Chandra Deep Field South
This paper presents multi-passband optical data obtained from observations of the Chandra Deep Field South (CDF-S), located at 3 h 32 m , 2748 0 . The observations were conducted at the ESO/MPG 2.2 mExpand
The mass of galaxies at low and high redshift : proceedings of the European Southern Observatory and Universitäts-Sternwarte München workshop held in Venice, Italy, 24-26 October 2001
• Physics
• 2003
From the Contents: The Mass of the Milky Way.- Distant Field BHB Stars and the Mass of the Milky Way.- A Pattern Speed in the Galaxy's OH/IR Stars.- Dark Matter in the Local Group: The Dark Haloes ofExpand