cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.6084/m9.figshare.756031
title: Gaussian Job Archive for C15H25NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.756032.v1
title: Gaussian Job Archive for C15H25NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.756030.v1
title: Gaussian Job Archive for C15H25NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.756031.v1
title: Gaussian Job Archive for C15H25NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.756072.v4
title: Development of the Drosophila central complex

description: This dataset consists of confocal stacks of the developing <em>Drosophila</em> brain, focussing on the central complex region. Throughout the dataset you can observe the central complex structure developing. All data is in .lsm format: I recommend that you download ImageJ (http://imagej.en.softonic.com/) to view the images. Each image stack is of a different brain. Brains were extracted at 1-4 hour intervals throughout metamorphosis (~100 hours) and stained with an antibody for Echinoid + a fluorescent secondary antibody. Brains were imaged using a confocal microscope. The central complex (CX) The adult Drosophila brain is divided into several neuropil masses (Power, 1943; Strausfeld, 1976) and is comprised of 100,000 neurons. The central complex (CX) is an intricate, symmetrical collection of neuropils located on the midline of the protocerebrum that has been observed in several insect species and implicated in several behaviors (reviewed in Homberg, 1987, 2008; Heisenberg,1994; Wessnitzer and Webb, 2006). In Drosophila the CX has been implicated in flight control (Ilius et al., 1994), multimodal information processing (Muller et al., 1997), coordination of motor behavior (Strauss and Heisenberg,1993; Martin et al., 1999; Strauss, 2002; Poeck et al.,2008), courtship behavior (Popov et al., 2003, 2004), visual pattern memory (Liu et al., 2006; Pan et al., 2009), olfactory memory (Wu et al., 2007), spatial orientation (Heinze and Homberg, 2007), and spatial orientation memory (Neuser et al., 2008). The paper that accompanies this dataset is: Young JM, Armstrong JD (2010) Building the central complex in Drosophila: the generation and development of distinct neural subsets. J Comp Neurol. 2010 May 1;518(9):1525-41.
DOI: 10.6084/m9.figshare.755981
title: Supplemental File

description: Supplemental file
DOI: 10.6084/m9.figshare.755981.v1
title: Supplemental File

description: Supplemental file
DOI: 10.6084/m9.figshare.755978
title: Gaussian Job Archive for C33H27CuI2N3P

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.755978.v1
title: Gaussian Job Archive for C33H27CuI2N3P

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754622
title: Stanford GSE Student Open Access vote breakdown

description: The vote breakdown for the GSE Student Open Access policy passed in 2013. See the official announcement of the policy at the link below.
DOI: 10.6084/m9.figshare.754620
title: Reduce Hathi File Python Script

description: There are several scripts, each with its own purpose, all written in Python, using an Enthought Python 2.7 distribution. One script uses regular expressions to collect IDs from Hathi Trust search results pages, then uses those IDs, which represent aggregate records sometimes consisting of multiple scanned documents, to collect the individual Hathi Trust Identifiers for each item in the search results. These identifiers are compared in another script to a monthly Hathi File, which then outputs the final data set.
DOI: 10.6084/m9.figshare.754621
title: Hathi Trust Astronomy articles

description: This project began as an attempt to match articles possessed by the Hathi Trust with Articles in the Astrophysics Data System, in order to establish links between the two. The project only got as far as collecting a data set of articles under the subject heading for Astronomy and Astrophysics in the Hathi Trust Data set. However, this data set is useful in understanding the holdings of Hathi Trust which pertain to Astronomy and Astrophysics. The scripts used to generate this data set can also be adapted to systematically access metadata for other subject areas and queries within the Hathi Trust.
DOI: 10.6084/m9.figshare.754622.v1
title: Stanford GSE Student Open Access vote breakdown

description: The vote breakdown for the GSE Student Open Access policy passed in 2013. See the official announcement of the policy at the link below.
DOI: 10.6084/m9.figshare.754619
title: Get Hathi IDs Python Script

description: There are several scripts, each with its own purpose, all written in Python, using an Enthought Python 2.7 distribution. One script uses regular expressions to collect IDs from Hathi Trust search results pages, then uses those IDs, which represent aggregate records sometimes consisting of multiple scanned documents, to collect the individual Hathi Trust Identifiers for each item in the search results. These identifiers are compared in another script to a monthly Hathi File, which then outputs the final data set.
DOI: 10.6084/m9.figshare.754620.v1
title: Reduce Hathi File Python Script

description: There are several scripts, each with its own purpose, all written in Python, using an Enthought Python 2.7 distribution. One script uses regular expressions to collect IDs from Hathi Trust search results pages, then uses those IDs, which represent aggregate records sometimes consisting of multiple scanned documents, to collect the individual Hathi Trust Identifiers for each item in the search results. These identifiers are compared in another script to a monthly Hathi File, which then outputs the final data set.
DOI: 10.6084/m9.figshare.754621.v1
title: Hathi Trust Astronomy articles

description: This project began as an attempt to match articles possessed by the Hathi Trust with Articles in the Astrophysics Data System, in order to establish links between the two. The project only got as far as collecting a data set of articles under the subject heading for Astronomy and Astrophysics in the Hathi Trust Data set. However, this data set is useful in understanding the holdings of Hathi Trust which pertain to Astronomy and Astrophysics. The scripts used to generate this data set can also be adapted to systematically access metadata for other subject areas and queries within the Hathi Trust.
DOI: 10.6084/m9.figshare.754615
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754618
title: Astronomy and Astrophysics Hathi Trust holdings

description: Project This project began as an attempt to match articles possessed by the Hathi Trust with Articles in the Astrophysics Data System, in order to establish links between the two. The project only got as far as collecting a data set of articles under the subject heading for Astronomy and Astrophysics in the Hathi Trust Data set. However, this data set is useful in understanding the holdings of Hathi Trust which pertain to Astronomy and Astrophysics. Data The data collected consists of comma separated value spreadsheet with metadata fromHathi Trust’s tab delimited Hathifiles. Field descriptions are available at the previous link. The data consists mostly of documents available in the public domain, but some articles not available in the public domain are included because of the way that the data was accessed.
DOI: 10.6084/m9.figshare.754619.v1
title: Get Hathi IDs Python Script

description: There are several scripts, each with its own purpose, all written in Python, using an Enthought Python 2.7 distribution. One script uses regular expressions to collect IDs from Hathi Trust search results pages, then uses those IDs, which represent aggregate records sometimes consisting of multiple scanned documents, to collect the individual Hathi Trust Identifiers for each item in the search results. These identifiers are compared in another script to a monthly Hathi File, which then outputs the final data set.
DOI: 10.6084/m9.figshare.754614
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754613
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754614.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754615.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754611
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754612
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754613.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754608
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754609
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754610
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754611.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754612.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754606
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754607
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754609.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754605
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754606.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754608.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754610.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754604
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754605.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754607.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754601
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754602
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754603
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754604.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754600
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754601.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754603.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754598
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754600.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754596
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754596.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754593
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754594
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754598.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754594.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754593.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754588
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754589
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754587
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754586
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754587.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754588.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754589.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754582
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754583
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754584
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754581
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754582.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754586.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754580
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754583.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754579
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754581.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.6084/m9.figshare.754584.v1
title: Gaussian Job Archive for C18H23NO3

description: Archive of work produced using the resources of the Imperial College High Performance Computing Service.
DOI: 10.15468/dl.7tdrt6
title: Occurrence Download

description: A dataset containing 34498 records in GBIF matching the query:
SELECT
 kingdom,
 kingdomkey,
 phylum,
 phylumkey,
 class,
 classkey,
 "order",
 orderkey,
 family,
 familykey,
 genus,
 genuskey,
 species,
 specieskey,
 "year",
 IF(ISNULL(kingdomkey), NULL, SUM(COUNT(*)) OVER (
 PARTITION BY kingdomkey, "year")) kingdomcount,
 IF(ISNULL(phylumkey), NULL, SUM(COUNT(*)) OVER (
 PARTITION BY phylumkey, "year")) phylumcount,
 IF(ISNULL(classkey), NULL, SUM(COUNT(*)) OVER (
 PARTITION BY classkey, "year")) classcount,
 IF(ISNULL(orderkey), NULL, SUM(COUNT(*)) OVER (
 PARTITION BY orderkey, "year")) ordercount,
 IF(ISNULL(familykey), NULL, SUM(COUNT(*)) OVER (
 PARTITION BY familykey, "year")) familycount,
 IF(ISNULL(genuskey), NULL, SUM(COUNT(*)) OVER (
 PARTITION BY genuskey, "year")) genuscount,
 COUNT(*) occurrences,
 MIN(GBIF_TEMPORALUNCERTAINTY(eventdate, eventtime)) mintemporaluncertainty,
 MIN(COALESCE(coordinateuncertaintyinmeters, 1000)) mincoordinateuncertaintyinmeters
FROM
 occurrence
WHERE
 occurrence.countrycode = 'NP'
 AND occurrence.occurrencestatus = 'PRESENT'
 AND (occurrence."year" &gt;= 2000 AND occurrence."year" &lt;= 2024)
 AND occurrence.hasgeospatialissues = FALSE
 AND NOT GBIF_STRINGARRAYCONTAINS(occurrence.issue, 'TAXON_MATCH_FUZZY', TRUE)
 AND (occurrence.distancefromcentroidinmeters &gt;= 2000.0 OR occurrence.distancefromcentroidinmeters IS NULL)
 AND NOT occurrence.basisofrecord IN ('FOSSIL_SPECIMEN', 'LIVING_SPECIMEN')
 AND (occurrence.specieskey IS NOT NULL AND occurrence."year" IS NOT NULL)
GROUP BY
 occurrence.kingdom,
 occurrence.kingdomkey,
 occurrence.phylum,
 occurrence.phylumkey,
 occurrence.class,
 occurrence.classkey,
 occurrence."order",
 occurrence.orderkey,
 occurrence.family,
 occurrence.familykey,
 occurrence.genus,
 occurrence.genuskey,
 occurrence.species,
 occurrence.specieskey,
 occurrence."year"

 The dataset's 34498 records were derived from 209 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0021400-250402121839773/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.34820/fk2/xacwlx/rensrg
title: 5_ji_2_1.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/n62hmc
title: 24_ma_3_2.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/hoq7ql
title: 23_la_3_1.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/btq9ol
title: 7_khon_2_2.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/pstnri
title: 3_tsi_2_4.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/jm531t
title: 11_zun_3_1.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/0e7pha
title: 14_shi_3_1.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/hdebba
title: 14_shin_3_4.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/rxeqyf
title: 24_mu_3_3.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/wdn1nm
title: 12_sa_2_3.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/qtii1q
title: 8_din_2_4.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/mif4rr
title: 9_dzi_3_1.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/svhhea
title: 13_syan_2_3.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/wghov2
title: 24_ma_3_4.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/aqmjdp
title: 23_lin_2_4.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/reykg6
title: 16_tho_3_2.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/bshvrw
title: 12_sun_2_3.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/yfvglo
title: 13_sya_2_4.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/eu1m7l
title: 12_si_3_1.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/wbuj62
title: 8_du_3_3.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/msw7i6
title: 17_dzhon_3_1.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/knvk0p
title: 11_za_2_3.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/usfp1p
title: 25_na_2_4.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/smdtxq
title: 10_ru_3_2.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/jqoxv5
title: 21_qun_2_3.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/amnc5d
title: 16_thin_2_3.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/z0lmde
title: 25_nu_3_1.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/u10pnh
title: 9_dzan_2_2.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/ruc1sq
title: 21_qan_2_4.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/hbe4mq
title: 10_ran_2_3.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/lnztpv
title: 17_dzhon_3_4.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/fmc1ye
title: 26_win_3_3.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/m3vudj
title: 3_tin_3_3.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/9dt3zl
title: 10_ri_2_4.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/djgyny
title: 10_ri_2_3.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/quxocb
title: 6_ha_2_3.wav

description: :unav
DOI: 10.34820/fk2/xacwlx/vnx8xn
title: 8_dun_3_4.wav

description: :unav