def get_record(recid, reset_cache=False):
"""
Record factory, it retrieves the record from bibfmt table if it is there,
if not, or reset_cache is set to True, it searches for the appropriate
reader to create the representation of the record.
@return: Bibfield object representing the record or None if the recid is not
present in the system
"""
#Search for recjson
if not reset_cache:
res = run_sql(
"SELECT value FROM bibfmt WHERE id_bibrec=%s AND format='recjson'",
(recid, ))
if res:
return JsonReader(BlobWrapper(pickle.loads(res[0][0])))
#There is no version cached or we want to renew it
#Then retrieve information and blob
blob_wrapper = _build_wrapper(recid)
if not blob_wrapper:
return None
record = CFG_BIBFIELD_READERS[blob_wrapper.master_format](blob_wrapper)
#Update bibfmt for future uses
run_sql(
"REPLACE INTO bibfmt(id_bibrec, format, last_updated, value) VALUES (%s, 'recjson', NOW(), %s)",
(recid, pickle.dumps((record.rec_json))))
return record
def test_rectruct_to_cool_struct_preparation(self):
"""docstring for test_rectruct_to_cool_struct_preparation"""
from invenio.search_engine import get_record as search_engine_get_record
bibrecord = search_engine_get_record(13)
blob = BlobWrapper(blob=bibrecord,
master_format='marc',
schema='recstruct')
r = MarcReader(blob)
self.assertTrue(r.rec_tree)
self.assertTrue(len(r.rec_tree.keys()) >= 14)
self.assertTrue('100__' in r.rec_tree)
def create_record(blob, master_format='marc', verbose=0, **aditional_info):
"""
Creates a record object from the blob description using the apropiate reader
for it.
@return Record object
"""
blob_wrapper = BlobWrapper(blob=blob,
master_format=master_format,
**aditional_info)
return CFG_BIBFIELD_READERS[master_format](blob_wrapper)
def test_recjson_creation_from_recstruct(self):
"""docstring for test_recjson_creation_from_recstruc"""
from invenio.search_engine import get_record as search_engine_get_record
bibrecord = search_engine_get_record(7)
blob = BlobWrapper(blob=bibrecord,
master_format='marc',
schema='recstruct')
r = MarcReader(blob)
self.assertTrue(r.rec_json)
self.assertTrue(r['__master_format'] == 'marc')
self.assertTrue('title' in r)
self.assertTrue(r['title.title'] == 'Tim Berners-Lee')
self.assertTrue('collection.primary' in r)
self.assertTrue(r['collection.primary'] == 'PICTURE')
def _build_wrapper(recid):
#TODO: update to look inside mongoDB for the parameters and the blob
# Now is just working for marc and recstruct
try:
master_format = run_sql("SELECT master_format FROM bibrec WHERE id=%s",
(recid, ))[0][0]
except:
return None
schema = 'recstruct'
if master_format == 'marc':
from invenio.search_engine import get_record as se_get_record
blob = se_get_record(recid)
else:
return None
return BlobWrapper(blob, master_format=master_format, schema=schema)
def test_rec_json_creation_from_marcxml_file(self):
"""docstring for test_rec_json_creation_from_marcxml_file"""
import os
import tempfile
from invenio.config import CFG_TMPDIR
xml = """
<record>
<datafield tag="041" ind1=" " ind2=" ">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="080" ind1=" " ind2=" ">
<subfield code="a">621.38</subfield>
</datafield>
<datafield tag="100" ind1=" " ind2=" ">
<subfield code="a">Hughes, Robert James</subfield>
</datafield>
<datafield tag="245" ind1=" " ind2=" ">
<subfield code="a">Introduction to electronics</subfield>
</datafield>
<datafield tag="260" ind1=" " ind2=" ">
<subfield code="a">London</subfield>
<subfield code="b">English Univ. Press</subfield>
<subfield code="c">1962</subfield>
</datafield>
<datafield tag="300" ind1=" " ind2=" ">
<subfield code="a">432 p</subfield>
</datafield>
<datafield tag="700" ind1=" " ind2=" ">
<subfield code="a">Pipe, Peter</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="0">
<subfield code="y">1962</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">50</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">198606</subfield>
</datafield>
<datafield tag="980" ind1=" " ind2=" ">
<subfield code="a">BOOK</subfield>
</datafield>
</record>
"""
fd, name = tempfile.mkstemp(suffix='.xml', dir=CFG_TMPDIR)
os.write(fd, xml)
os.close(fd)
blob = BlobWrapper(blob='',
master_format='marc',
schema='file:xml',
blob_file_name=name)
r = MarcReader(blob)
self.assertTrue(r.rec_json)
self.assertTrue('authors' in r)
self.assertTrue(r['authors[0].full_name'] == "Hughes, Robert James")
def test_marcxml_to_cool_struct_preparation(self):
"""docstring for test_marcxml_to_cool_struct_preparation"""
#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">[email protected]</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>
"""
blob = BlobWrapper(blob=xml, master_format='marc', schema='xml')
r = MarcReader(blob)
self.assertTrue(r.rec_tree)
self.assertTrue(len(r.rec_tree.keys()) >= 14)
self.assertTrue('100__' in r.rec_tree)
def test_rec_json_creation_from_marcxml(self):
"""docstring for test_rec_json_creation_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 <[email protected]></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 & 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>
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<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>
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<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>
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<subfield code="m">Goobar A., Perlmutter S., 1995</subfield>
<subfield code="p">14</subfield>
<subfield code="t">Astrophys. J.</subfield>
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<subfield code="y">1995</subfield>
<subfield code="s">Astrophys. J. 450 (1995) 14</subfield>
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<subfield code="m">Hamuy M., Phillips M.M., Maza J., Suntzeff N.B., Schommer R.A., Aviles R. 1996</subfield>
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<subfield code="y">1996</subfield>
<subfield code="s">Astrophys. J. 112 (1996) 2391</subfield>
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<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>
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<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>
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<subfield code="y">1998</subfield>
<subfield code="s">Mon. Not. R. Astron. Soc. 294 (1998) L1</subfield>
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<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>
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<subfield code="m">Lineweaver, C.H., Barbosa D., 1998b</subfield>
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<subfield code="r">astro-ph/9808045</subfield>
<subfield code="s">Astrophys. J. 509 (1998) L77-80</subfield>
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<subfield code="m">Ostriker J.P., Steinhardt P.J., 1995</subfield>
<subfield code="p">600</subfield>
<subfield code="t">Nature</subfield>
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<subfield code="y">1995</subfield>
<subfield code="s">Nature 377 (1995) 600</subfield>
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<subfield code="m">Perlmutter S. et al., 1998a, Astrophys. J.in press. (P98)</subfield>
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<subfield code="s">Astrophys. J. 517 (1999) 565-586</subfield>
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<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. & 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>
"""
blob = BlobWrapper(blob=xml, master_format='marc', schema="xml")
r = MarcReader(blob)
self.assertTrue(r.rec_json)
self.assertTrue(r['__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)
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>
"""
blob = BlobWrapper(blob=xml, master_format='marc', schema="xml")
r = MarcReader(blob, check=True)
self.assertTrue('title' in r)
self.assertEquals(len(r['title']), 2)
self.assertEquals(len(r.fatal_errors), 1)
r.rec_json['title'] = r.rec_json['title'][0]
r.check_record(reset=True)