A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2017; you can also visit the original URL.
The file type is application/pdf.
Filters
Software citation principles
2016
PeerJ Computer Science
Preserved Fulltext
Seinstra, Netherlands eScience Center Arfon Smith, GitHub (co-chair) Kaitlin Thaney, Mozilla Science Lab Ilian Todorov, Science and Technology Facilities Council Matt Turk, University of Illinois Miguel ...
Smith et al. (2016), PeerJ Comput. ...
The researcher needs to know which version was used, for
Competing Interests Arfon M. Smith is an employee of GitHub, Inc., San Francisco, California.
Author Contributions Arfon M. ...
doi:10.7717/peerj-cs.86
fatcat:ezkr3sa72fflndu7tjjh6i5koy
The demise of the filesystem and multi level service architecture
[article]
2019
arXiv
pre-print
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2020; you can also visit the original URL.
The file type is application/pdf.
Other Versions
(See also the decadal paper on Cloud infrastructure by Arfon Smith et. Al.)
The catch Switching to an object store removes the filesystem bottle neck however it also removes the filesystem index. ...
arXiv:1907.13060v2
fatcat:44idxf3i7jc6bl2vdrawppm2ry
Introducing JOSS: The Journal of Open Source Software
[article]
2017
Figshare
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2020; you can also visit the original URL.
The file type is application/pdf.
M Smith
orcid: 0000-0000-0000-1234
affiliation: 1
-name: Mickey Mouse
orcid: 0000-0000-0000-1234
affiliation: 2
affiliations:
-name: Space Telescope Science Institute
index: 1
-name: Disney Inc ...
$275 + ($1 × 200) + ($19 × 12)) / 100 = $3.51
Business model (2/2)
article.md
---
title: 'Fidgit: An ungodly union of GitHub and figshare'
tags:
-example
-tags
-for the paper
authors:
-name: Arfon ...
doi:10.6084/m9.figshare.5208151
fatcat:s3qlrvcylzhyvgx33mgjdi74vi
PLANET HUNTERS: ASSESSING THEKEPLERINVENTORY OF SHORT-PERIOD PLANETS
2012
Astrophysical Journal
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2017; you can also visit the original URL.
The file type is application/pdf.
Other Versions
. , 2008 Land et al. 2008) , the search for supernovae (Smith et al. 2011) , the identification of solar coronal mass ejections (Davis et al. 2012) , cataloging of star forming regions (Simpson et al ...
doi:10.1088/0004-637x/754/2/129
fatcat:xytzklqlybfcvfuro6xgy4lyma
Planet Four: Probing Springtime Winds On Mars By Mapping The Southern Polar Co2 Jet Deposits
2018
Zenodo
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2020; you can also visit the original URL.
The file type is application/pdf.
About 97% of all fans are below 100 m in length, with a median value of 24 m. ...
median of 59 m for MY30. ...
doi:10.5281/zenodo.1475479
fatcat:7mqmlcxh3nb6lcxr6ixwdr6nwa
Galaxy Zoo: bar lengths in local disc galaxies★
2011
Monthly notices of the Royal Astronomical Society
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2017; you can also visit the original URL.
The file type is application/pdf.
Other Versions
AC K N OW L E D G M E N T S The authors would like to thank an anonymous referee for comments which improve the paper. ...
the lower panel, we see that the brightest galaxies (M r < −24) which have bars are more easily identified than the fainter galaxies (M r > −22). ...
Almost all 3150 bars are significantly larger than the typical SDSS seeing of <2.5 arcsec (Smith et al. 2002) , only 28 are close to this value (<5) arcsec. ...
doi:10.1111/j.1365-2966.2011.18979.x
fatcat:vzlaf2k4rngflbsp5k3aso3bsm
Small-scale structure in the interstellar medium: time-varying interstellar absorption towards κ Velorum
2012
Monthly notices of the Royal Astronomical Society
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is application/pdf.
Other Versions
AC K N OW L E D G M E N T S The authors thank PATT for the award of UHRF time on the AAT and for T&S. ...
However, there are no systematic differences in b values between species in component B, over a range m = 23 (Na I) to m = 40 (Ca I and Ca II). ...
Preliminary results from these observations were presented by Smith (2010) ; they are superseded by the results presented here. ...
doi:10.1093/mnras/sts310
fatcat:2zsk3mxkbjfvrozgo43j7y2x4y
Galaxy Zoo: Mergers – Dynamical models of interacting galaxies
2016
Monthly notices of the Royal Astronomical Society
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is application/pdf.
Other Versions
simulation )T 2 simulation = a 3 (M actual )T 2 actual = a 3 (8) T actual = T simulation M simulation M actual . (9) For most of our systems, this can be simplified to T actual = T simulation √ m l , ( ...
However, Smith et al. (2010) found four distinct best-fitting models for the pair of galaxies NGC 7714/5. ...
AC K N OW L E D G E M E N T S The authors would like to thank the thousands of members of Galaxy Zoo: Mergers for their help on the project. ...
doi:10.1093/mnras/stw649
fatcat:cwteigb24bczna2sa5342b5adq
Galaxy Zoo: bars in disc galaxies★
2010
Monthly notices of the Royal Astronomical Society
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2017; you can also visit the original URL.
The file type is application/pdf.
Other Versions
r > −20 (black solid), −20 < M r < −21 (blue dotted), −21 < M r < −22 (green dashed) and M r < −22 (red dot-dashed). ...
< z < 0.03, M g < −18.5. ...
doi:10.1111/j.1365-2966.2010.17834.x
fatcat:2ceymtolvjba3pyslkdy3ybtle
Petabytes to Science
[article]
2019
arXiv
pre-print
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2020; you can also visit the original URL.
The file type is application/pdf.
Other Versions
SOFTWARE Contributors: Arfon Smith <arfon@stsci.edu>, Erik Tollerud <etollerud@stsci.edu>, Kelle Cruz, Stuart Mumford, Nirav Merchant, Gautham Narayan, Alex Drlica-Wagner Note: If you have come directly ...
WORKFORCE & CAREER DEVELOPMENT Contributors: Dara Norman <dnorman@noao.edu>, Kelle Cruz, Vandana Desai, Britt Lundgren, Eric Bellm, Frossie Economou, Arfon Smith, Amanda Bauer, Brian Nord, Chad Schafer ...
arXiv:1905.05116v2
fatcat:lzi3j7hzk5crfbedgraa5ojwbi
Algorithms and Statistical Models for Scientific Discovery in the Petabyte Era
[article]
2019
arXiv
pre-print
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2020; you can also visit the original URL.
The file type is application/pdf.
The field of astronomy has arrived at a turning point in terms of size and complexity of both datasets and scientific collaboration. Commensurately, algorithms and statistical models have begun to adapt --- e.g., via the onset of artificial intelligence --- which itself presents new challenges and opportunities for growth. This white paper aims to offer guidance and ideas for how we can evolve our technical and collaborative frameworks to promote efficient algorithmic development and take
arXiv:1911.02479v1
fatcat:kqwomxs4e5b4lkxphubizr4f74
more »
... age of opportunities for scientific discovery in the petabyte era. We discuss challenges for discovery in large and complex data sets; challenges and requirements for the next stage of development of statistical methodologies and algorithmic tool sets; how we might change our paradigms of collaboration and education; and the ethical implications of scientists' contributions to widely applicable algorithms and computational modeling. We start with six distinct recommendations that are supported by the commentary following them. This white paper is related to a larger corpus of effort that has taken place within and around the Petabytes to Science Workshops (https://petabytestoscience.github.io/).
Galaxy Zoo: quantifying morphological indicators of galaxy interaction★
2012
Monthly notices of the Royal Astronomical Society
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2020; you can also visit the original URL.
The file type is application/pdf.
Other Versions
Formally, this is p(A ∩ M) = p(A|M) p(M) ( 1 ) = f (A) Q⊂M a∈ Q f (a) , (2) where Q are subsets of the set of answers M partitioned by question, and the a are the individual answers in Q. ...
displays morphological features M. ...
doi:10.1093/mnras/sts391
fatcat:rv2rwvnfnzh73ji7y5ihvv66ii
Journal of Open Source Software (JOSS): design and first-year review
2018
PeerJ Computer Science
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is application/pdf.
Other Versions
Arfon Smith is the founding editor-in-chief, and the founding editors are 39 Lorena A. ...
Editor-in-chief 345 Arfon Smith stewarded the majority of articles published in the first year. ...
doi:10.7717/peerj-cs.147
pmid:32704456
pmcid:PMC7340488
fatcat:groqd7oapre3nhxebxrsvunxgy
Galaxy Zoo: morphological classifications for 120 000 galaxies inHSTlegacy imaging
2016
Monthly notices of the Royal Astronomical Society
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is application/pdf.
Other Versions
AC K N OW L E D G E M E N T S KW, MG, CS, MB, and LF gratefully acknowledge support from the US National Science Foundation Grant AST1413610. ...
We also thank Jennifer Lotz for sharing her G-M 20 measurements for the AEGIS sample. We thank Coleman Krawczyk for his assistance in producing Fig. 4 . ...
The effect on the redshifted images is simply an empirical addition to the magnitude of a galaxy of the form M = e × z + M, where M is the corrected magnitude and e is the evolutionary correction in magnitudes ...
doi:10.1093/mnras/stw2568
fatcat:garyifupenb3fpg623aadcqeqe
Galaxy Zoo: an independent look at the evolution of the bar fraction over the last eight billion years from HST-COSMOS★
2014
Monthly notices of the Royal Astronomical Society
Preserved Fulltext
A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2017; you can also visit the original URL.
The file type is application/pdf.
Other Versions
AC K N OW L E D G E M E N T S This work has been made possible by the participation of more than 86 000 volunteers of the Galaxy Zoo: Hubble project. ...
Low-mass sample -10.0 ≤ log (M /M ) < 10.34 Intermediate-mass sample -10.34 ≤ log (M /M ) < 10.64 High-mass sample -log (M /M ) ≥ 10.64 p bar threshold
f bar, 0
γ
≥0.3
0.39 ± 0.11
−0.020 ± 0.017 ...
/M ) > 10.0]. ...
doi:10.1093/mnras/stt2397
fatcat:5qzry5oqdbev3iihwas323eec4
« Previous
Showing results 1 — 15 out of 145 results