Search
| Leader | 00000nz a2200037n 45 0 | ||
|---|---|---|---|
| 001 | WKP|Q89654410 (VIAF cluster) (Authority/Source Record) | ||
| 003 | WKP | ||
| 005 | 20241121000309.0 | ||
| 008 | 241121nneanz||abbn n and d | ||
| 035 | ‡a (WKP)Q89654410 | ||
| 024 | ‡a 0000-0001-6293-9062 ‡2 orcid | ||
| 035 | ‡a (OCoLC)Q89654410 | ||
| 100 | 0 | ‡a Carlos Contreras Velasquez ‡9 en-gb ‡9 fr ‡9 pt ‡9 de ‡9 sv ‡9 it ‡9 cy ‡9 pt-br ‡9 es | |
| 375 | ‡a 1 ‡2 iso5218 | ||
| 400 | 0 | ‡a Carlos Contreras Velasquez ‡c researcher ‡9 en | |
| 400 | 0 | ‡a Carlos Contreras Velasquez ‡c wetenschapper ‡9 nl | |
| 670 | ‡a Author's Electromagnetic evidence that SSS17a is the result of a binary neutron star merger. | ||
| 670 | ‡a Author's Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis. | ||
| 670 | ‡a Author's Persistent C II absorption in the normal type Ia supernova 2002fk | ||
| 670 | ‡a Author's Probing type Ia supernova properties using bolometric light curves from the Carnegie Supernova Project and the CfA Supernova Group | ||
| 670 | ‡a Author's Red versus Blue: Early Observations of Thermonuclear Supernovae Reveal Two Distinct Populations? | ||
| 909 | ‡a (orcid) 0000000162939062 ‡9 1 | ||
| 919 | ‡a redversusblueearlyobservationsofthermonuclearsupernovaereveal2distinctpopulations ‡A Red versus Blue: Early Observations of Thermonuclear Supernovae Reveal Two Distinct Populations? ‡9 1 | ||
| 919 | ‡a probingtypeiasupernovapropertiesusingbolometriclightcurvesfromthecarnegiesupernovaprojectandthecfasupernovagroup ‡A Probing type Ia supernova properties using bolometric light curves from the Carnegie Supernova Project and the CfA Supernova Group ‡9 1 | ||
| 919 | ‡a persistent1002absorptioninthenormaltypeiasupernova2002fk ‡A Persistent C II absorption in the normal type Ia supernova 2002fk ‡9 1 | ||
| 919 | ‡a lightcurvesoftheneutronstarmergergw170817sss17aimplicationsforrprocessnucleosynthesis ‡A Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis. ‡9 1 | ||
| 919 | ‡a electromagneticevidencethatsss17aistheresultofabinaryneutronstarmerger ‡A Electromagnetic evidence that SSS17a is the result of a binary neutron star merger. ‡9 1 | ||
| 946 | ‡a b ‡9 1 | ||
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| 996 | ‡2 J9U|987007332481305171 | ||
| 996 | ‡2 J9U|987007320647105171 | ||
| 996 | ‡2 DNB|1056523271 | ||
| 996 | ‡2 BNCHL|10000000000000000055481 | ||
| 996 | ‡2 DNB|114440620X | ||
| 996 | ‡2 DNB|1249151635 | ||
| 996 | ‡2 BNF|16931552 | ||
| 996 | ‡2 RERO|A005914615 | ||
| 996 | ‡2 LC|ns2014003810 | ||
| 996 | ‡2 LC|no2016091384 | ||
| 996 | ‡2 LC|ns2015000531 | ||
| 996 | ‡2 CAOONL|ncf11593093 | ||
| 996 | ‡2 SUDOC|235861081 | ||
| 996 | ‡2 LC|no2010184879 | ||
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| 996 | ‡2 ISNI|0000000433156116 | ||
| 996 | ‡2 BNCHL|10000000000000000173187 | ||
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| 996 | ‡2 LC|n 79070263 | ||
| 996 | ‡2 BNCHL|10000000000000000290107 | ||
| 996 | ‡2 LC|n 86107841 | ||
| 996 | ‡2 NII|DA18822043 | ||
| 996 | ‡2 DNB|1112677364 | ||
| 996 | ‡2 BNCHL|10000000000000000128252 | ||
| 996 | ‡2 DNB|1197939067 | ||
| 996 | ‡2 LC|no2012143484 | ||
| 996 | ‡2 BNCHL|10000000000000000832540 | ||
| 996 | ‡2 ISNI|000000002829913X | ||
| 996 | ‡2 LC|no2023126015 | ||
| 996 | ‡2 LC|no2021120492 | ||
| 996 | ‡2 ISNI|0000000359899316 | ||
| 996 | ‡2 LC|nr2003005675 | ||
| 996 | ‡2 LC|n 2023051953 | ||
| 996 | ‡2 LC|ns2012003968 | ||
| 996 | ‡2 LC|n 2013017346 | ||
| 996 | ‡2 W2Z|1542227324754 | ||
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| 996 | ‡2 LC|no2017003347 | ||
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| 996 | ‡2 LC|nr2004017171 | ||
| 996 | ‡2 LC|n 2023003246 | ||
| 996 | ‡2 BIBSYS|1542227324754 | ||
| 996 | ‡2 SUDOC|171134079 | ||
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| 996 | ‡2 ISNI|000000003369912X | ||
| 996 | ‡2 SUDOC|199819084 | ||
| 996 | ‡2 SUDOC|16103716X | ||
| 996 | ‡2 RERO|A006107107 | ||
| 996 | ‡2 LC|no2018019560 | ||
| 996 | ‡2 LC|no2011139614 | ||
| 996 | ‡2 LC|no2016050917 | ||
| 996 | ‡2 ISNI|0000000043859123 | ||
| 996 | ‡2 DNB|1170715591 | ||
| 996 | ‡2 LC|n 97013964 | ||
| 997 | ‡a 0 0 lived 0 0 ‡9 1 |
