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Curve fitting
Known as:
Curve-fitted
, Curve-fitting
, Non linear curve fitting
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Curve fitting is the process of constructing a curve, or mathematical function, that has the best fit to a series of data points, possibly subject to…
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Related topics
Related topics
50 relations
B-spline
Curve-fitting compaction
Difference engine
Estimation theory
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Broader (1)
Numerical analysis
Papers overview
Semantic Scholar uses AI to extract papers important to this topic.
Highly Cited
2015
Highly Cited
2015
A TURNOVER IN THE GALAXY MAIN SEQUENCE OF STAR FORMATION AT M* ∼ 1010 M☉ FOR REDSHIFTS z < 1.3
N. Lee
,
D. Sanders
,
+14 authors
Q. Xiao
2015
Corpus ID: 31409870
The relationship between galaxy star formation rates (SFRs) and stellar masses (M*) is reexamined using a mass-selected sample of…
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Review
2013
Review
2013
A SUBSTANTIAL POPULATION OF MASSIVE QUIESCENT GALAXIES AT z ∼ 4 FROM ZFOURGE
C. Straatman
,
I. Labb'e
,
+21 authors
V. Tilvi
2013
Corpus ID: 118506629
We report the likely identification of a substantial population of massive M ∼ 1011 M☉ galaxies at z ∼ 4 with suppressed star…
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Review
2012
Review
2012
THE BRIGHTEST OF REIONIZING GALAXIES SURVEY: CONSTRAINTS ON THE BRIGHT END OF THE z ∼ 8 LUMINOSITY FUNCTION
L. Bradley
,
M. Trenti
,
+6 authors
N. Pirzkal
2012
Corpus ID: 73582913
We report the discovery of 33 Lyman-break galaxy candidates at z ∼ 8 detected in Hubble Space Telescope Wide Field Camera 3 (WFC3…
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Highly Cited
2010
Highly Cited
2010
Mass profiles and concentration-dark matter relation in X-ray luminous galaxy clusters
S. Ettori
,
A. Leccardi
,
+4 authors
M. Meneghetti
2010
Corpus ID: 119106893
Context. Galaxy clusters represent valuable cosmological probes us ing tests that mainly rely on measurements of cluster masses…
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Review
2009
Review
2009
A WIDE-FIELD HIGH-RESOLUTION H i MOSAIC OF MESSIER 31. I. OPAQUE ATOMIC GAS AND STAR FORMATION RATE DENSITY
R. Braun
,
D. Thilker
,
R. Walterbos
,
E. Corbelli
2009
Corpus ID: 17996197
We have undertaken a deep, wide-field H i imaging survey of M31, reaching a maximum resolution of about 50 pc and 2 km s−1 across…
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Highly Cited
2006
Highly Cited
2006
Accepted for publication in ApJL Preprint typeset using L ATEX style emulateapj v. 6/22/04 SPECTROSCOPIC IDENTIFICATION OF MASSIVE GALAXIES AT Z ∼ 2.3 WITH STRONGLY SUPPRESSED STAR FORMATION 1
2006
Corpus ID: 16145121
Highly Cited
2004
Highly Cited
2004
Dissipative trigonometrically-fitted methods for linear second-order IVPs with oscillating solution
T. Simos
Applied Mathematics Letters
2004
Corpus ID: 27641107
Highly Cited
2001
Highly Cited
2001
Practical Time-Scale Fitting of Self-Similar Traffic with Markov-Modulated Poisson Process
Tadafumi Yoshihara
,
S. Kasahara
,
Yutaka Takahashi
Telecommunications Systems
2001
Corpus ID: 17365974
Recent measurements of packet/cell streams in multimedia communication networks have revealed that they have the self-similar…
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Highly Cited
1993
Highly Cited
1993
Optical control of molecular dynamics: Molecular cannons, reflectrons, and wave‐packet focusers
J. Krause
,
R. Whitnell
,
K. Wilson
,
Yijing Yan
,
S. Mukamel
1993
Corpus ID: 85505352
We consider the control of molecular dynamics using tailored light fields, based on a phase space theory of control [Y. J. Yan et…
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Highly Cited
1990
Highly Cited
1990
Evidence for Extrathymic Changes in the T Cell Receptor Y/b Repertoire
Christina
,
Parker
,
+14 authors
Brenner
1990
Corpus ID: 16758437
Lymphocytes express two types of TCRs, either a/f (1-3) or y/b (4). The genes encoding the TCR y and b chains are composed of V…
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