Photometric Reduction
Photometric Reduction is a data reduction method in observational astronomy that calibrates raw detector measurements to derive precise apparent brightness values of celestial sources by correcting for instrumental, atmospheric, and geometric effects.
76
Publications
5K
Citations
428
Authors
220
Institutions
Publications per year
2017–2026
15
Parents
76
PypeIt: The Python Spectroscopic Data Reduction Pipeline
J. X. Prochaska, Joseph F. Hennawi, Kyle B. Westfall et al. · The Journal of Open Source Software · 2020 · 425 citations · Full text
Natural Sciences, Astronomy, Physics +17
GaBoDS: The Garching‐Bonn Deep Survey
T. Erben, M. Schirmer, J. P. Dietrich et al. · Astronomische Nachrichten · 2005 · 318 citations · Full text
The Dark Energy Survey Data Release 2
The Astrophysical Journal Supplement Series · 2021 · 305 citations · Full text
1–5 of 76
428
3
h-index
3
h-index
Kharkiv National University of Radio Electronics, Ukraine
2 publications · 60 citations
2
h-index
2
h-index
2
h-index
1–5 of 428
220
University of Arizona
Tucson, United States
9 h-index
31 publications
1.2K citations
California Institute of Technology
Pasadena, United States
8 h-index
17 publications
698 citations

Centre National de la Recherche Scientifique
Paris, France
6 h-index
16 publications
1.6K citations
University of California, Santa Cruz
Santa Cruz, United States
6 h-index
8 publications
1.2K citations
Princeton University
Princeton, United States
5 h-index
22 publications
1.8K citations
University of California, Berkeley
Berkeley, United States
5 h-index
14 publications
1.3K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
5 h-index
7 publications
620 citations
European Southern Observatory
Garching bei München, Germany
5 h-index
8 publications
1.4K citations
1–8 of 220
PASP · 9 publications · 1K citations
9
h-index
6 publications · 377 citations
6
h-index
ApJ · 7 publications · 402 citations
6
h-index
AJ · 5 publications · 204 citations
5
h-index
5 publications · 438 citations
5
h-index
1–5