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6 references found looking up in 17 out of 17 Archives.
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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3D6G6QL
Repositorysid.inpe.br/mtc-m19/2012/12.07.16.42
Metadata Repositorysid.inpe.br/mtc-m19/2012/12.07.16.42.40
Metadata Last Update2018:06.05.04.13.17 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyCorreiaMakhRaul:2012:PoCoNo
TitlePossible cosmic noise absorption detected in Antarctica produced by solar proton events that occurred on January 2012
Year2012
Access Date2023, Jan. 31
Secondary TypePRE CI
2. Context
Author1 Correia, E.
2 Makhmutov, V.
3 Raulin, J. -P.
Group1 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 ecorreia@craam.mackenzie.br
e-Mail Addressmarcelo.pazos@inpe.br
Conference NameEuropean Cosmic Ray Symposium, 23 and Russian Cosmic Ray Conference, 32.
Conference LocationMoscow, Russia.
DateJuly, 3-7, 2012
History (UTC)2012-12-07 16:43:17 :: marcelo.pazos@sid.inpe.br -> administrator :: 2012
2018-06-05 04:13:17 :: administrator -> marcelo.pazos@inpe.br :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AreaCEA
ArrangementPossible cosmic noise...
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6. Notes
Empty Fieldsabstract archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi edition editor format isbn issn keywords label language lineage mark nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup resumeid rightsholder secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/3D538GU
Repositorydpi.inpe.br/plutao/2012/11.28.14.20.50   (restricted access)
Last Update2015:03.18.15.53.34 (UTC) administrator
Metadata Repositorydpi.inpe.br/plutao/2012/11.28.14.20.51
Metadata Last Update2018:06.05.00.01.56 (UTC) administrator
Secondary KeyINPE--PRE/
Labellattes: 1272123236892781 4 KaufmannABCDFF:2012:TePhOb
Citation KeyKaufmannABCDFFCGHKLLMMMMNPRSSSSTVVZ:2012:TePhOb
TitleSOLAR-T: terahertz photometers to observe solar flare emission on stratospheric balloon flights
Year2012
Access Date2023, Jan. 31
Secondary TypePRE CI
Number of Files1
Size837 KiB
2. Context
Author 1 Kaufmann, P.
 2 Abrantes, A
 3 Bortolucci, E. C.
 4 Correia, Emilia
 5 Diniz, J. A.
 6 Fernandez, G.
 7 Fernandes, Luiz Olavo T.
 8 Castro, C. G. Giménez
 9 Godoy, R.
10 Hurford, G.
11 Kudaka, A. S.
12 Lebedev, M.
13 Lin, R. P.
14 Machado, N.
15 Makhmutov., V. S.
16 Marcon, R.
17 Marun, A.
18 Nicolaev, V. A.
19 Pereyra, P.
20 Raulin, J. P.
21 Silva, C. M.
22 Shih, A.
23 Stozkhov, Y. I.
24 Swart, J. W.
25 Timofeevsky, A. V.
26 Valio, A.
27 Villela Neto, Thyrso
28 Zakia, M. B.
Resume Identifier 1
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Affiliation 1 Universidade Presbiteriana Mackenzie
 2 Propertech Tecnologia Ltda
 3 Universidade Estadual de Campinas (UNICAMP)
 4 Instituto Nacional de Pesquisas Espaciais (INPE)
 5 Universidade Estadual de Campinas (UNICAMP)
 6 Complejo Astronomico El Leoncito (CONICET)
 7 Universidade Presbiteriana Mackenzie
 8 Universidade Presbiteriana Mackenzie
 9 Complejo Astronomico El Leoncito (CONICET)
10 University of California
11 Universidade Presbiteriana Mackenzie
12 Special Astrophysical Observatory of Russian Academy of Sciences
13 University of California
14 Propertech Tecnologia Ltda
15 Lebedev Physics Institute
16 Universidade Estadual de Campinas (UNICAMP)
17 Complejo Astronomico El Leoncito (CONICET)
18 Tydex Co
19 Complejo Astronomico El Leoncito (CONICET)
20 Universidade Presbiteriana Mackenzie
21 Neuron Eletronica Ltda
22 National Aeronautical and Space Administration
23 Lebedev Physics Institut
24 Universidade Estadual de Campinas (UNICAMP)
25 Tydex Co
26 Universidade Presbiteriana Mackenzie
27 Instituto Nacional de Pesquisas Espaciais (INPE)
28 Universidade Estadual de Campinas (UNICAMP)
Author e-Mail Address 1 pierrekau@gmail.com
 2
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 4 ecorreia@craam.mackenzie.br
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27 villela@das.inpe.br
e-Mail Addressecorreia@craam.mackenzie.br
Conference NameSpace Telescopes and Instrumentation: Optical, Infrared, and Millimeter Wave.
Conference LocationAmsterdam
Date2012
PublisherInternational Society for Optics and Photonics
Volume84424L
Pages84424L-1-84424L-9
Book TitleProceedings
Tertiary TypePaper
History (UTC)2012-11-28 23:06:22 :: lattes -> marciana :: 2012
2012-12-04 17:30:24 :: marciana -> administrator :: 2012
2018-06-05 00:01:56 :: administrator -> marciana :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordssolar flare
THz photometers
ballon flights
AbstractA new solar flare spectral component has been found with intensities increasing for larger sub-THz frequencies, spectrally separated from the well known microwaves component, bringing challenging constraints for interpretation. Higher THz frequencies observations are needed to understand the nature of the mechanisms occurring in flares. A twofrequency THz photometer system was developed to observe outside the terrestrial atmosphere on stratospheric balloons or satellites, or at exceptionally transparent ground stations. 76 mm diameter telescopes were designed to observe the whole solar disk detecting small relative changes in input temperature caused by flares at localized positions at 3 and 7 THz. Golay cell detectors are preceded by low-pass filters to suppress visible and near IR radiation, band-pass filters, and choppers. It can detect temperature variations smaller than 1 K with time resolution of a fraction of a second, corresponding to small burst intensities. The telescopes are being assembled in a thermal controlled box to which a data conditioning and acquisition unit is coupled. While all observations are stored on board, a telemetry system will forward solar activity compact data to the ground station. The experiment is planned to fly on board of long-duration stratospheric balloon flights some time in 2013-2015. One will be coupled to the GRIPS gamma-ray experiment in cooperation with University of California, Berkeley, USA. One engineering flight will be flown in the USA, and a 2 weeks flight is planned over Antarctica in southern hemisphere summer. Another long duration stratospheric balloon flight over Russia (one week) is planned in cooperation with the Lebedev Physics Institute, Moscow, in northern hemisphere summer.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção > DIDAS > SOLAR-T: terahertz photometers...
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Languageen
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marciana
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Next Higher Units8JMKD3MGPCW/3ETR8EH
URL (untrusted data)http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=1362329
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
Empty Fieldsarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi edition editor format isbn issn lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization parameterlist parentrepositories previousedition previouslowerunit progress project publisheraddress rightsholder secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark type
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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3D7AU3S
Repositorysid.inpe.br/mtc-m19/2012/12.12.15.49
Last Update2015:03.17.19.11.09 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2012/12.12.15.49.58
Metadata Last Update2018:06.05.04.13.28 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1063/1.3701933
Citation KeyMagalhaesOCCDDFFGMPRRRST:2012:RePoSo
TitleSOUTH POL: Revealing the Polarized Southern Sky
Year2012
Access Date2023, Jan. 31
Secondary TypePRE CI
Number of Files1
Size620 KiB
2. Context
Author 1 Magalhaes, A. M.
 2 Oliveira, C. M.
 3 Carciofi, A.
 4 Costa, R.
 5 Dal Pino, E. M. G.
 6 Diaz, M.
 7 Ferrari, T.
 8 Fernandez, C.
 9 Gomes, A. L.
10 Marrara, L.
11 Pereyrac, A.
12 Ribeiro, N. L.
13 Rodrigues, Cláudia Vilega
14 Rubinho, M. S.
15 Seriacopi, D. B.
16 Taylor, K.
Resume Identifier 1
 2
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13 8JMKD3MGP5W/3C9JGS5
Group 1
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13 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation 1 Universidade de São Paulo (USP)
 2 Universidade de São Paulo (USP)
 3 Universidade de São Paulo (USP)
 4 Universidade de São Paulo (USP)
 5 Universidade de São Paulo (USP)
 6 Universidade de São Paulo (USP)
 7 Universidade de São Paulo (USP)
 8 Universidade de São Paulo (USP)
 9 Universidade de São Paulo (USP)
10 Universidade de São Paulo (USP)
11 Observatório Nacional
12 Universidade de São Paulo (USP)
13 Instituto Nacional de Pesquisas Espaciais (INPE)
14 Universidade de São Paulo (USP)
15 Universidade de São Paulo (USP)
16 Universidade de São Paulo (USP)
Author e-Mail Address 1
 2
 3
 4
 5
 6
 7
 8
 9
10
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13 claudia.rodrigues@inpe.br
EditorHoffman, JL
Bjorkman, J
Whitney, B.
e-Mail Addressmarcelo.pazos@inpe.br
Conference NameConference on Stellar Polarimetry: From Birth to Death.
Conference LocationMadison, WI
DateJun. 27-30, 2011
Volume1429
Pages244-247
Book TitleProceedings
OrganizationAIP Conference Proceedings
History (UTC)2012-12-12 15:50:56 :: marcelo.pazos@sid.inpe.br -> administrator :: 2012
2018-06-05 04:13:28 :: administrator -> marcelo.pazos@inpe.br :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typefinaldraft
KeywordsPolarization
Stars
Interstellar Medium
Dust
Milky Way
AGN
CMB
AbstractSOUTH POL will be a survey of the Southern sky in optical polarized light. It will use a newly designed polarimetric module at an 80cm Robotic Telescope. Telescope and polarimeter will be installed at CTIO, Chile, in late 2012. The initial goal is to cover the sky south of declination -15° in two years of observing time, aiming at a polarimetric accuracy 㸟 0.1% down to V=15, with a camera covering a field of about 2.0 square degrees. SOUTH POL will impact areas such as Cosmology, Extragalactic Astronomy, Interstellar Medium of the Galaxy and Magellanic Clouds, Star Formation, Stellar Envelopes, Stellar explosions and Solar System, among others.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > SOUTH POL: Revealing...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP7W/3D7AU3S
zipped data URLhttp://urlib.net/zip/8JMKD3MGP7W/3D7AU3S
Target Filemagalhaes_south.pdf
User Groupmarcelo.pazos@inpe.br
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Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination edition format isbn issn label language lineage mark nextedition notes numberofvolumes orcid parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress rightsholder secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url
7. Description control
e-Mail (login)marcelo.pazos@inpe.br
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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/3C63LTB
Repositorydpi.inpe.br/plutao/2012/06.21.18.40.12   (restricted access)
Last Update2015:03.17.19.05.04 (UTC) administrator
Metadata Repositorydpi.inpe.br/plutao/2012/06.21.18.40.13
Metadata Last Update2018:06.05.00.01.44 (UTC) administrator
Labellattes: 1272123236892781 5 MakhmutovRMBCKMFE:2012:AnCoRa
Citation KeyMakhmutovRMBCKMFE:2012:AnCoRa
TitleAnalysis of cosmic ray variations observed by the CARPET in association with solar flares in 2011-2012
FormatDVD
Year2012
Access Date2023, Jan. 31
Secondary TypePRE CI
Number of Files1
Size402 KiB
2. Context
Author1 Makhmutov, V. S.
2 Raulin, J. P.
3 Mendonça, Rafael R. S.
4 Bazilevskaya, G. A.
5 Correia, Emilia
6 Kaufmann, P.
7 Marun, A.
8 Fernandez, G.
9 Echer, Ezequiel
Resume Identifier1
2
3
4
5 8JMKD3MGP5W/3C9JH2C
6
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9 8JMKD3MGP5W/3C9JH3D
Group1
2
3 DAS-CEA-INPE-MCTI-GOV-BR
4
5 DAS-CEA-INPE-MCTI-GOV-BR
6
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9 DGE-CEA-INPE-MCTI-GOV-BR
Affiliation1 Lebedev Physical Institute
2 Universidade Presbiteriana Mackenzie
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Lebedev Physical Institute
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Universidade Presbiteriana Mackenzie
7 4 Complejo Astronmico el Leoncito (CASLEO)
8 4 Complejo Astronmico el Leoncito, CASLEO
9 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3
4
5 ecorreia@craam.mackenzie.br
6
7
8
9 eecher@dge.inpe.br
e-Mail Addressecorreia@craam.mackenzie.br
Conference NameEuropean Cosmic Ray Symposium, 23 and Russian Cosmic Ray Conference, 32.
Conference LocationMoscou
DateJuly, 3-7, 2012
Volumexx
Pages012185
Book TitleProceedings
History (UTC)2012-06-22 00:10:59 :: lattes -> secretaria.cpa@dir.inpe.br :: 2012
2012-12-07 11:50:31 :: secretaria.cpa@dir.inpe.br -> administrator :: 2012
2018-06-05 00:01:44 :: administrator -> :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordscosmic rays
solar flares
atmosphere
AbstractThe CARPET cosmic ray detector was installed on April 2006 at CASLEO (Complejo Astronmico El Leoncito) at the Argentinean Andes (31.8S, 69.3W, 2550 m, Rc=9.65 GV). This instrument was developed within an international cooperation between the Lebedev Physical Institute RAS (LPI; Russia), the Centro de Radio Astronomia e Astrofsica Mackenzie (CRAAM; Brazil) and the Complejo Astronmico el Leoncito (CASLEO; Argentina). In this paper we present results of analysis of cosmic ray variations recorded by the CARPET during increased solar flare activity in 2011-2012. Available solar and interplanetary medium observational data obtained onboard GOES, FERMI, ISS, as well as cosmic ray measurements by ground-based neutron monitor network were also used in the present analysis.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Analysis of cosmic...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Analysis of cosmic...
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4. Conditions of access and use
Languageen
Target FileMakhmutov_analysis.pdf
User Grouplattes
secretaria.cpa@dir.inpe.br
Reader Groupadministrator
marciana
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Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
8JMKD3MGPCW/3EU29DP
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
Empty Fieldsarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi edition editor isbn issn lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress rightsholder secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url

1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3DCR7E8
Repositorysid.inpe.br/mtc-m19/2013/01.15.15.46
Metadata Repositorysid.inpe.br/mtc-m19/2013/01.15.15.46.02
Metadata Last Update2018:06.05.04.13.48 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyMoroDCASMRGC:2012:SiObOv
TitleCorrelation between the cosmic noise absorption calculated from the SARINET data and the energetic particles measured by MEPED: simultaneous observations over SAMA region
Year2012
Access Date2023, Jan. 31
Secondary TypePRE CI
2. Context
Author1 Moro, Juliano
2 Denardini, Clezio M
3 Correia, Emilia
4 Abdu, Mangalathayil A
5 Schuch, Nelson J
6 Makita, Kazuo
7 Resende, Laysa
8 Guizelli, Lais M
9 Chen, Sony Su
Group1
2
3 DAS-CEA-INPE-MCTI-GOV-BR
4
5 CRS-CCR-INPE-MCTI-GOV-BR
Affiliation1
2
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4
5 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3
4
5 njschuch@lacesm.ufsm.br
e-Mail Addressmarcelo.pazos@inpe.br
Conference NameAGU Fall Meeting.
Conference LocationSan Francisco
History (UTC)2013-01-15 15:46:25 :: marcelo.pazos@sid.inpe.br -> administrator :: 2012
2018-06-05 04:13:48 :: administrator -> marcelo.pazos@inpe.br :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractThe cosmic noise absorption is presented in terms of the two-dimensional images obtained from the imaging riometers operated at the Southern Space Observatory, in São Martinho da Serra, Brazil, Concepcion and Punta Arenas in Chile, which belong to the South American Riometer Network and are located at the central and periphery regions of the South American Magnetic Anomaly. Correlations are performed between the maximum cosmic noise absorption observed at these stations and the energetic electron flux in two energies channels (>30 keV and >300 keV) and the proton flux in three energies channels (80-240 keV, 800-2500 keV and >6900 keV) as measured by the Medium Energy Proton and Electron Detector, during a moderate geomagnetic storm that occurred on September 3, 2008. The results show high correlations between the cosmic noise absorption detected at São Martinho da Serra and the flux of protons with energy between 80 and 240 keV, and the flux of electrons with energies higher than 300 keV, while an additional ionization at Concepcion was correlated with electrons of energies higher than 30 keV. The cosmic noise absorption detected at Punta Arenas was probably caused by the increase of the protons flux with energy between 80 and 240 keV.
AreaCEA
doc Directory Contentthere are no files
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agreement Directory Content
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User Groupmarcelo.pazos@inpe.br
Visibilityshown
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryiconet.com.br/banon/2006/11.26.21.31
Next Higher Units8JMKD3MGPCW/3ETR8EH
8JMKD3MGPCW/3EUFCFP
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory date descriptionlevel dissemination doi edition editor format isbn issn keywords label language lineage mark nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup resumeid rightsholder secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
7. Description control
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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3D7B9TS
Repositorysid.inpe.br/mtc-m19/2012/12.12.17.37
Last Update2015:03.16.16.56.50 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2012/12.12.17.37.13
Metadata Last Update2018:06.05.04.13.28 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeySansomMiloVazdSánc:2012:ObVeMo
TitleEffects of Non-Solar Abundance Ratios on Star Spectra: Observations versus Models
Year2012
Access Date2023, Jan. 31
Secondary TypePRE CI
Number of Files1
Size213 KiB
2. Context
Author1 Sansom, Anne E.
2 Milone, André de Castro
3 Vazdekis, Alexandre
4 Sánchez-Blázquez, Patricia
Resume Identifier1
2 8JMKD3MGP5W/3C9JGHK
Group1
2 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1 University of Central Lancashire
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto de Astrofísica de Canarias
4 Universidad Autonoma de Madrid
Author e-Mail Address1 aesansom@uclan.ac.uk
2 andre.milone@inpe.br
e-Mail Addressmarcelo.pazos@inpe.br
Conference NameInternational Astronomical Union Symposium: The Spectral Energy Distribution of Galaxies, 284 (IAUS).
Book TitleProceedings
History (UTC)2012-12-12 17:38:47 :: marcelo.pazos@sid.inpe.br -> administrator :: 2012
2018-06-05 04:13:28 :: administrator -> marcelo.pazos@inpe.br :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsstars: atmospheres
stars: abundances
techniques: spectroscopic
AbstractElement abundance ratios hold important clues to understanding the evolution of stellar populations, through the varying timescales of different nucleosynthetic contributors. Newly measured and compiled [Mg/Fe] ratios in the MILES stellar library are used to confront models of star spectra. Such models have been used in recent years to provide estimates of differential changes in spectral line strengths, due to enhancements in [α/Fe]. In this paper we test one widely used set of theoretical element response functions. Using magnesium as a proxy for all alpha elements we test the reliability of these theoretical response functions against empirical observations, and thus the reliability of current methods of measuring element abundance ratios in the stellar populations.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Effects of Non-Solar...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 12/12/2012 15:37 1.0 KiB 
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP7W/3D7B9TS
zipped data URLhttp://urlib.net/zip/8JMKD3MGP7W/3D7B9TS
Languageen
Target Filesansom_effects.pdf
User Groupmarcelo.pazos@inpe.br
Reader Groupadministrator
marcelo.pazos@inpe.br
Visibilityshown
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ETR8EH
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
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7. Description control
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