Homec4science
Diffusion invenio-infoscience (maint-2.0) Browse

R3600/modules/bibfield/lib/bibfield_marcreader_unit_tests.py
6cfac47dfe32maint-2.0

Last Change
Raw File

bibfield_marcreader_unit_tests.py
View Options

# -*- coding: utf-8 -*-
##
## This file is part of Invenio.
## Copyright (C) 2004, 2005, 2006, 2007, 2008, 2010, 2011 CERN.
##
## Invenio is free software; you can redistribute it and/or
## modify it under the terms of the GNU General Public License as
## published by the Free Software Foundation; either version 2 of the
## License, or (at your option) any later version.
##
## Invenio is distributed in the hope that it will be useful, but
## WITHOUT ANY WARRANTY; without even the implied warranty of
## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
## General Public License for more details.
##
## You should have received a copy of the GNU General Public License
## along with Invenio; if not, write to the Free Software Foundation, Inc.,
## 59 Temple Place, Suite 330, Boston, MA 02111-1307, USA.
"""
BibField Marc21 reader regression tests.
"""
__revision__ = "$Id$"
from invenio.testutils import InvenioTestCase
from invenio.bibfield_marcreader import MarcReader
from invenio.bibfield import Record
from invenio.testutils import make_test_suite, run_test_suite
class BibFieldMarcReaderMarcXML(InvenioTestCase):
"""
"""
@classmethod
def setUpClass(cls):
from invenio.bibfield_config_engine import BibFieldParser
BibFieldParser.reparse()
def test_marcxml_to_cool_struct_preparation(self):
"""Bibfield - intermediate structure from marc xml"""
#First record from demobibcfg.xml
xml = """
<record>
<datafield tag="037" ind1=" " ind2=" ">
<subfield code="a">CERN-EX-0106015</subfield>
</datafield>
<datafield tag="100" ind1=" " ind2=" ">
<subfield code="a">Photolab</subfield>
</datafield>
<datafield tag="245" ind1=" " ind2=" ">
<subfield code="a">ALEPH experiment: Candidate of Higgs boson production</subfield>
</datafield>
<datafield tag="246" ind1=" " ind2="1">
<subfield code="a">Expérience ALEPH: Candidat de la production d'un boson Higgs</subfield>
</datafield>
<datafield tag="260" ind1=" " ind2=" ">
<subfield code="c">14 06 2000</subfield>
</datafield>
<datafield tag="340" ind1=" " ind2=" ">
<subfield code="a">FILM</subfield>
</datafield>
<datafield tag="520" ind1=" " ind2=" ">
<subfield code="a">Candidate for the associated production of the Higgs boson and Z boson. Both, the Higgs and Z boson decay into 2 jets each. The green and the yellow jets belong to the Higgs boson. They represent the fragmentation of a bottom andanti-bottom quark. The red and the blue jets stem from the decay of the Z boson into a quark anti-quark pair. Left: View of the event along the beam axis. Bottom right: Zoom around the interaction point at the centre showing detailsof the fragmentation of the bottom and anti-bottom quarks. As expected for b quarks, in each jet the decay of a long-lived B meson is visible. Top right: "World map" showing the spatial distribution of the jets in the event.</subfield>
</datafield>
<datafield tag="595" ind1=" " ind2=" ">
<subfield code="a">Press</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Experiments and Tracks</subfield>
</datafield>
<datafield tag="653" ind1="1" ind2=" ">
<subfield code="a">LEP</subfield>
</datafield>
<datafield tag="856" ind1="0" ind2=" ">
<subfield code="f">neil.calder@cern.ch</subfield>
</datafield>
<datafield tag="FFT" ind1=" " ind2=" ">
<subfield code="a">http://invenio-software.org/download/invenio-demo-site-files/0106015_01.jpg</subfield>
<subfield code="r">restricted_picture</subfield>
</datafield>
<datafield tag="FFT" ind1=" " ind2=" ">
<subfield code="a">http://invenio-software.org/download/invenio-demo-site-files/0106015_01.gif</subfield>
<subfield code="f">.gif;icon</subfield>
<subfield code="r">restricted_picture</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="0">
<subfield code="o">0003717PHOPHO</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="0">
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="0">
<subfield code="b">81</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="1">
<subfield code="c">2001-06-14</subfield>
<subfield code="l">50</subfield>
<subfield code="m">2001-08-27</subfield>
<subfield code="o">CM</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="P">
<subfield code="p">Bldg. 2</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="P">
<subfield code="r">Calder, N</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="S">
<subfield code="s">n</subfield>
<subfield code="w">200231</subfield>
</datafield>
<datafield tag="980" ind1=" " ind2=" ">
<subfield code="a">PICTURE</subfield>
</datafield>
</record>
"""
reader = MarcReader(blob=xml, schema='xml')
reader._prepare_blob()
self.assertTrue(reader.rec_tree)
self.assertTrue(len(reader.rec_tree.keys()) >= 14)
self.assertTrue('100__' in reader.rec_tree)
def test_rec_json_creation_from_marcxml(self):
"""BibField - recjson from marcxml"""
xml = """
<record>
<datafield tag="037" ind1=" " ind2=" ">
<subfield code="a">astro-ph/9812226</subfield>
</datafield>
<datafield tag="041" ind1=" " ind2=" ">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1=" " ind2=" ">
<subfield code="a">Efstathiou, G P</subfield>
<subfield code="u">Cambridge University</subfield>
</datafield>
<datafield tag="245" ind1=" " ind2=" ">
<subfield code="a">Constraints on $\Omega_{\Lambda}$ and $\Omega_{m}$from Distant Type 1a Supernovae and Cosmic Microwave Background Anisotropies</subfield>
</datafield>
<datafield tag="260" ind1=" " ind2=" ">
<subfield code="c">14 Dec 1998</subfield>
</datafield>
<datafield tag="300" ind1=" " ind2=" ">
<subfield code="a">6 p</subfield>
</datafield>
<datafield tag="520" ind1=" " ind2=" ">
<subfield code="a">We perform a combined likelihood analysis of the latest cosmic microwave background anisotropy data and distant Type 1a Supernova data of Perlmutter etal (1998a). Our analysis is restricted tocosmological models where structure forms from adiabatic initial fluctuations characterised by a power-law spectrum with negligible tensor component. Marginalizing over other parameters, our bestfit solution gives Omega_m = 0.25 (+0.18, -0.12) and Omega_Lambda = 0.63 (+0.17, -0.23) (95 % confidence errors) for the cosmic densities contributed by matter and a cosmological constantrespectively. The results therefore strongly favour a nearly spatially flat Universe with a non-zero cosmological constant.</subfield>
</datafield>
<datafield tag="595" ind1=" " ind2=" ">
<subfield code="a">LANL EDS</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Astrophysics and Astronomy</subfield>
</datafield>
<datafield tag="700" ind1=" " ind2=" ">
<subfield code="a">Lasenby, A N</subfield>
</datafield>
<datafield tag="700" ind1=" " ind2=" ">
<subfield code="a">Hobson, M P</subfield>
</datafield>
<datafield tag="700" ind1=" " ind2=" ">
<subfield code="a">Ellis, R S</subfield>
</datafield>
<datafield tag="700" ind1=" " ind2=" ">
<subfield code="a">Bridle, S L</subfield>
</datafield>
<datafield tag="856" ind1="0" ind2=" ">
<subfield code="f">George Efstathiou &lt;gpe@ast.cam.ac.uk&gt;</subfield>
</datafield>
<datafield tag="FFT" ind1=" " ind2=" ">
<subfield code="a">http://invenio-software.org/download/invenio-demo-site-files/9812226.pdf</subfield>
</datafield>
<datafield tag="FFT" ind1=" " ind2=" ">
<subfield code="a">http://invenio-software.org/download/invenio-demo-site-files/9812226.fig1.ps.gz</subfield>
<subfield code="t">Additional</subfield>
</datafield>
<datafield tag="FFT" ind1=" " ind2=" ">
<subfield code="a">http://invenio-software.org/download/invenio-demo-site-files/9812226.fig3.ps.gz</subfield>
<subfield code="t">Additional</subfield>
</datafield>
<datafield tag="FFT" ind1=" " ind2=" ">
<subfield code="a">http://invenio-software.org/download/invenio-demo-site-files/9812226.fig5.ps.gz</subfield>
<subfield code="t">Additional</subfield>
</datafield>
<datafield tag="FFT" ind1=" " ind2=" ">
<subfield code="a">http://invenio-software.org/download/invenio-demo-site-files/9812226.fig6.ps.gz</subfield>
<subfield code="t">Additional</subfield>
</datafield>
<datafield tag="FFT" ind1=" " ind2=" ">
<subfield code="a">http://invenio-software.org/download/invenio-demo-site-files/9812226.fig7.ps.gz</subfield>
<subfield code="t">Additional</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="0">
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="0">
<subfield code="b">11</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="1">
<subfield code="c">1998-12-14</subfield>
<subfield code="l">50</subfield>
<subfield code="m">2001-04-07</subfield>
<subfield code="o">BATCH</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="4">
<subfield code="p">Mon. Not. R. Astron. Soc.</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="O">
<subfield code="i">SLAC</subfield>
<subfield code="s">4162242</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="5">
<subfield code="b">CER</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="S">
<subfield code="s">n</subfield>
<subfield code="w">200231</subfield>
</datafield>
<datafield tag="980" ind1=" " ind2=" ">
<subfield code="a">PREPRINT</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Bond, J.R. 1996, Theory and Observations of the Cosmic Background Radiation, in "Cosmology and Large Scale Structure", Les Houches Session LX, August 1993, eds. R. Schaeffer, J. Silk, M. Spiro and J. Zinn-Justin, Elsevier SciencePress, Amsterdam, p469</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Bond J.R., Efstathiou G., Tegmark M., 1997</subfield>
<subfield code="p">L33</subfield>
<subfield code="t">Mon. Not. R. Astron. Soc.</subfield>
<subfield code="v">291</subfield>
<subfield code="y">1997</subfield>
<subfield code="s">Mon. Not. R. Astron. Soc. 291 (1997) L33</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Bond, J.R., Jaffe, A. 1997, in Proc. XXXI Rencontre de Moriond, ed. F. Bouchet, Edition Fronti eres, in press</subfield>
<subfield code="r">astro-ph/9610091</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Bond J.R., Jaffe A.H. and Knox L.E., 1998</subfield>
<subfield code="r">astro-ph/9808264</subfield>
<subfield code="s">Astrophys.J. 533 (2000) 19</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Burles S., Tytler D., 1998a, to appear in the Proceedings of the Second Oak Ridge Symposium on Atomic &amp; Nuclear Astrophysics, ed. A. Mezzacappa, Institute of Physics, Bristol</subfield>
<subfield code="r">astro-ph/9803071</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Burles S., Tytler D., 1998b, Astrophys. J.in press</subfield>
<subfield code="r">astro-ph/9712109</subfield>
<subfield code="s">Astrophys.J. 507 (1998) 732</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Caldwell, R.R., Dave, R., Steinhardt P.J., 1998</subfield>
<subfield code="p">1582</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">80</subfield>
<subfield code="y">1998</subfield>
<subfield code="s">Phys. Rev. Lett. 80 (1998) 1582</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Carroll S.M., Press W.H., Turner E.L., 1992, Ann. Rev. Astr. Astrophys., 30, 499. Chaboyer B., 1998</subfield>
<subfield code="r">astro-ph/9808200</subfield>
<subfield code="s">Phys.Rept. 307 (1998) 23</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Devlin M.J., De Oliveira-Costa A., Herbig T., Miller A.D., Netterfield C.B., Page L., Tegmark M., 1998, submitted to Astrophys. J</subfield>
<subfield code="r">astro-ph/9808043</subfield>
<subfield code="s">Astrophys. J. 509 (1998) L69-72</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Efstathiou G. 1996, Observations of Large-Scale Structure in the Universe, in "Cosmology and Large Scale Structure", Les Houches Session LX, August 1993, eds. R. Schaeffer, J. Silk, M. Spiro and J. Zinn-Justin, Elsevier SciencePress, Amsterdam, p135. Efstathiou G., Bond J.R., Mon. Not. R. Astron. Soc.in press</subfield>
<subfield code="r">astro-ph/9807130</subfield>
<subfield code="s">Astrophys. J. 518 (1999) 2-23</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Evrard G., 1998, submitted to Mon. Not. R. Astron. Soc</subfield>
<subfield code="r">astro-ph/9701148</subfield>
<subfield code="s">Mon.Not.Roy.Astron.Soc. 292 (1997) 289</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Freedman J.B., Mould J.R., Kennicutt R.C., Madore B.F., 1998</subfield>
<subfield code="r">astro-ph/9801090</subfield>
<subfield code="s">Astrophys. J. 480 (1997) 705</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Garnavich P.M. et al. 1998</subfield>
<subfield code="r">astro-ph/9806396</subfield>
<subfield code="s">Astrophys.J. 509 (1998) 74-79</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Goobar A., Perlmutter S., 1995</subfield>
<subfield code="p">14</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">450</subfield>
<subfield code="y">1995</subfield>
<subfield code="s">Astrophys. J. 450 (1995) 14</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Hamuy M., Phillips M.M., Maza J., Suntzeff N.B., Schommer R.A., Aviles R. 1996</subfield>
<subfield code="p">2391</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">112</subfield>
<subfield code="y">1996</subfield>
<subfield code="s">Astrophys. J. 112 (1996) 2391</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Hancock S., Gutierrez C.M., Davies R.D., Lasenby A.N., Rocha G., Rebolo R., Watson R.A., Tegmark M., 1997</subfield>
<subfield code="p">505</subfield>
<subfield code="t">Mon. Not. R. Astron. Soc.</subfield>
<subfield code="v">298</subfield>
<subfield code="y">1997</subfield>
<subfield code="s">Mon. Not. R. Astron. Soc. 298 (1997) 505</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Hancock S., Rocha G., Lasenby A.N., Gutierrez C.M., 1998</subfield>
<subfield code="p">L1</subfield>
<subfield code="t">Mon. Not. R. Astron. Soc.</subfield>
<subfield code="v">294</subfield>
<subfield code="y">1998</subfield>
<subfield code="s">Mon. Not. R. Astron. Soc. 294 (1998) L1</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Herbig T., De Oliveira-Costa A., Devlin M.J., Miller A.D., Page L., Tegmark M., 1998, submitted to Astrophys. J</subfield>
<subfield code="r">astro-ph/9808044</subfield>
<subfield code="s">Astrophys.J. 509 (1998) L73-76</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Lineweaver C.H., 1998. Astrophys. J.505, L69. Lineweaver, C.H., Barbosa D., 1998a</subfield>
<subfield code="p">624</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">446</subfield>
<subfield code="y">1998</subfield>
<subfield code="s">Astrophys. J. 446 (1998) 624</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Lineweaver, C.H., Barbosa D., 1998b</subfield>
<subfield code="p">799</subfield>
<subfield code="t">Astron. Astrophys.</subfield>
<subfield code="v">329</subfield>
<subfield code="y">1998</subfield>
<subfield code="s">Astron. Astrophys. 329 (1998) 799</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">De Oliveira-Costa A., Devlin M.J., Herbig T., Miller A.D., Netterfield C.B. Page L., Tegmark M., 1998, submitted to Astrophys. J</subfield>
<subfield code="r">astro-ph/9808045</subfield>
<subfield code="s">Astrophys. J. 509 (1998) L77-80</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Ostriker J.P., Steinhardt P.J., 1995</subfield>
<subfield code="p">600</subfield>
<subfield code="t">Nature</subfield>
<subfield code="v">377</subfield>
<subfield code="y">1995</subfield>
<subfield code="s">Nature 377 (1995) 600</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Peebles P.J.E., 1993, Principles of Physical Cosmology, Princeton University Press, Princeton, New Jersey. Perlmutter S, et al., 1995, In Presentations at the NATO ASI in Aiguablava, Spain, LBL-38400; also published in Thermonuclear Supernova, P. Ruiz-Lapuente, R. Cana and J. Isern (eds), Dordrecht, Kluwer, 1997, p749. Perlmutter S, et al., 1997</subfield>
<subfield code="p">565</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">483</subfield>
<subfield code="y">1997</subfield>
<subfield code="s">Astrophys. J. 483 (1997) 565</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Perlmutter S. et al., 1998a, Astrophys. J.in press. (P98)</subfield>
<subfield code="r">astro-ph/9812133</subfield>
<subfield code="s">Astrophys. J. 517 (1999) 565-586</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Perlmutter S. et al., 1998b, In Presentation at the January 1988 Meeting of the American Astronomical Society, Washington D.C., LBL-42230, available at www-supernova.lbl.gov; B.A.A.S., volume : 29 (1997) 1351Perlmutter S, et al., 1998c</subfield>
<subfield code="p">51</subfield>
<subfield code="t">Nature</subfield>
<subfield code="v">391</subfield>
<subfield code="y">1998</subfield>
<subfield code="s">Nature 391 (1998) 51</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Ratra B., Peebles P.J.E., 1988</subfield>
<subfield code="p">3406</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">37</subfield>
<subfield code="y">1988</subfield>
<subfield code="s">Phys. Rev. D 37 (1988) 3406</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Riess A. et al. 1998, Astrophys. J.in press</subfield>
<subfield code="r">astro-ph/9805201</subfield>
<subfield code="s">Astron. J. 116 (1998) 1009-1038</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Seljak U., Zaldarriaga M. 1996</subfield>
<subfield code="p">437</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">469</subfield>
<subfield code="y">1996</subfield>
<subfield code="s">Astrophys. J. 469 (1996) 437</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Seljak U. &amp; Zaldarriaga M., 1998</subfield>
<subfield code="r">astro-ph/9811123</subfield>
<subfield code="s">Phys. Rev. D60 (1999) 043504</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Tegmark M., 1997</subfield>
<subfield code="p">3806</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">79</subfield>
<subfield code="y">1997</subfield>
<subfield code="s">Phys. Rev. Lett. 79 (1997) 3806</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Tegmark M. 1998, submitted to Astrophys. J</subfield>
<subfield code="r">astro-ph/9809201</subfield>
<subfield code="s">Astrophys. J. 514 (1999) L69-L72</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Tegmark, M., Eisenstein D.J., Hu W., Kron R.G., 1998</subfield>
<subfield code="r">astro-ph/9805117</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Wambsganss J., Cen R., Ostriker J.P., 1998</subfield>
<subfield code="p">29</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">494</subfield>
<subfield code="y">1998</subfield>
<subfield code="s">Astrophys. J. 494 (1998) 29</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Webster M., Bridle S.L., Hobson M.P., Lasenby A.N., Lahav O., Rocha, G., 1998, Astrophys. J.in press</subfield>
<subfield code="r">astro-ph/9802109</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">White M., 1998, Astrophys. J.in press</subfield>
<subfield code="r">astro-ph/9802295</subfield>
<subfield code="s">Astrophys. J. 506 (1998) 495</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Zaldarriaga, M., Spergel D.N., Seljak U., 1997</subfield>
<subfield code="p">1</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">488</subfield>
<subfield code="y">1997</subfield>
<subfield code="s">Astrophys. J. 488 (1997) 1</subfield>
</datafield>
</record>
"""
reader = MarcReader(blob=xml, schema="xml")
r = Record(reader.translate())
self.assertTrue(r['__meta_metadata__.__additional_info__.master_format'] == 'marc')
self.assertTrue('authors' in r)
self.assertTrue(r['authors[0].full_name'] == "Efstathiou, G P")
self.assertTrue(len(r['authors']) == 5)
self.assertTrue('title.title' in r)
self.assertTrue(r['title.title'] == "Constraints on $\Omega_{\Lambda}$ and $\Omega_{m}$from Distant Type 1a Supernovae and Cosmic Microwave Background Anisotropies")
self.assertTrue('abstract.summary' in r)
self.assertTrue(r['abstract.summary'] == "We perform a combined likelihood analysis of the latest cosmic microwave background anisotropy data and distant Type 1a Supernova data of Perlmutter etal (1998a). Our analysis is restricted tocosmological models where structure forms from adiabatic initial fluctuations characterised by a power-law spectrum with negligible tensor component. Marginalizing over other parameters, our bestfit solution gives Omega_m = 0.25 (+0.18, -0.12) and Omega_Lambda = 0.63 (+0.17, -0.23) (95 % confidence errors) for the cosmic densities contributed by matter and a cosmological constantrespectively. The results therefore strongly favour a nearly spatially flat Universe with a non-zero cosmological constant.")
self.assertTrue('reference' in r)
self.assertTrue(len(r['reference']) == 36)
class BibFieldCheckRecord(InvenioTestCase):
"""
"""
@classmethod
def setUpClass(cls):
from invenio.bibfield_config_engine import BibFieldParser
BibFieldParser.reparse()
def test_check_error_reporting(self):
"""BibField - check error reporting"""
xml = """
<record>
<datafield tag="020" ind1=" " ind2=" ">
<subfield code="a">2225350574</subfield>
</datafield>
<datafield tag="041" ind1=" " ind2=" ">
<subfield code="a">fre</subfield>
</datafield>
<datafield tag="080" ind1=" " ind2=" ">
<subfield code="a">518.5:62.01</subfield>
</datafield>
<datafield tag="100" ind1=" " ind2=" ">
<subfield code="a">Dasse, Michel</subfield>
</datafield>
<datafield tag="245" ind1=" " ind2=" ">
<subfield code="a">Analyse informatique</subfield>
</datafield>
<datafield tag="245" ind1=" " ind2=" ">
<subfield code="n">t.1</subfield>
<subfield code="p">Les preliminaires</subfield>
</datafield>
<datafield tag="260" ind1=" " ind2=" ">
<subfield code="a">Paris</subfield>
<subfield code="b">Masson</subfield>
<subfield code="c">1972</subfield>
</datafield>
<datafield tag="490" ind1=" " ind2=" ">
<subfield code="a">Informatique</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="0">
<subfield code="y">1972</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="0">
<subfield code="b">21</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="1">
<subfield code="c">1990-01-27</subfield>
<subfield code="l">00</subfield>
<subfield code="m">2002-04-12</subfield>
<subfield code="o">BATCH</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="S">
<subfield code="s">m</subfield>
<subfield code="w">198604</subfield>
</datafield>
<datafield tag="980" ind1=" " ind2=" ">
<subfield code="a">BOOK</subfield>
</datafield>
</record>
"""
reader = MarcReader(blob=xml, schema="xml")
r = Record(reader.translate())
r.check_record(reset = True)
self.assertTrue('title' in r)
self.assertEquals(len(r['title']), 2)
self.assertEquals(len(r.fatal_errors), 1)
r['title'] = r['title'][0]
r.check_record(reset = True)
self.assertEquals(len(r.fatal_errors), 0)
TEST_SUITE = make_test_suite(BibFieldMarcReaderMarcXML,
BibFieldCheckRecord)
if __name__ == "__main__":
run_test_suite(TEST_SUITE)
c4science · Help