1
Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds
Biny
2
The 2.5 m Telescope of the Sloan Digital Sky Survey
Available
3
Double-blind test program for astrometric planet detection with Gaia
Nayana
4
A Modified Magnitude System that Produces Well-Behaved Magnitudes, Colors, and Errors Even for Low Signal-to-Noise Ratio Measurements
Avishek
5
An Improved Photometric Calibration of the Sloan Digital Sky Survey Imaging Data
Available
6
SExtractor: Software for source extraction
Omkar
7
Faint U-Band Dropouts in the WFPC2 Parallels of the Hubble Ultra Deep Field
Available
8
Precision Determination of Atmospheric Extinction at Optical and Near-infrared Wavelengths
Aishawnnya
9
The Orthogonal Transfer CCD
Preetish
10
Weak Lensing Measurements: A Revisited Method and Application to Hubble Space Telescope Images
Debajyoti
11
The Sloan Digital Sky Survey Photometric Camera
Available
12
The WFPC2 Archival Pure Parallels Project
Available
13
MoMaF: the Mock Map Facility
Available
14
Drizzle: A Method for the Linear Reconstruction of Undersampled Images
Available
15
The Characterization, Subtraction, and Addition of Astronomical Images
Sushma
16
Estimating Photometric Redshifts Using Support Vector Machines
Sushmita
17
New insight on galaxy structure from GALPHAT I. Motivation, methodology, and benchmarks for Sersic models
Available
18
Detailed Decomposition of Galaxy Images. II. Beyond Axisymmetric Models
Niladri
19
WFPC2 Observations of the Hubble Deep Field South
Available
20
Pixel-based correction for Charge Transfer Inefficiency in the Hubble Space Telescope Advanced Camera for Surveys
Available
21
Toward High-Precision Astrometry with WFPC2. I. Deriving an Accurate Point-Spread Function
Available
22
An Empirical Pixel-Based Correction for Imperfect CTE. I. HST's Advanced Camera for Surveys
Available
23
A New Method for Band-limited Imaging with Undersampled Detectors
Kaustubh
24
Preparing Red-Green-Blue Images from CCD Data
Ruchika
25
The Three-Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey
Dinesh
26
K-Corrections and Filter Transformations in the Ultraviolet, Optical, and Near-Infrared
Available
27
A Photometricity and Extinction Monitor at the Apache Point Observatory
Available
28
High-efficiency Autonomous Laser Adaptive Optics
Atul
29
A Novel Technique to Improve Photometry in Confused Images Using Graphs and Bayesian Priors
Suman
30
Parallax beyond a Kiloparsec from Spatially Scanning the Wide Field Camera 3 on the Hubble Space Telescope
Swagat