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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34R/42NM865
Repositóriosid.inpe.br/mtc-m21c/2020/06.25.11.11   (acesso restrito)
Última Atualização2020:06.25.11.11.44 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m21c/2020/06.25.11.11.44
Última Atualização dos Metadados2022:01.04.01.35.13 (UTC) administrator
DOI10.3847/1538-3881/ab7cce
ISSN0004-6256
Chave de CitaçãoSzkodyDHHRRLGBBKPMMGCCDGHKKMNPRSS:2020:CaVaFi
TítuloCataclysmic variables in the first year of the zwicky transient facility
Ano2020
MêsMay
Data de Acesso11 maio 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho2398 KiB
2. Contextualização
Autor 1 Szkody, Paula
 2 Dicenzo, Brooke
 3 Ho, Anna Y. Q.
 4 Hillenbrand, Lynne A.
 5 van Roestel, Jan
 6 Ridder, Margaret
 7 Lima, Isabel de Jesus
 8 Graham, Melissa Lynn
 9 Bellm, Eric Christopher
10 Burdge, Kevin
11 Kupfer, Thomas
12 Prince, Thomas A.
13 Masci, Frank J.
14 Mróz, Przemyslaw J.
15 Golkhou, V. Zach
16 Coughlin, Michael
17 Cunningham, Virginia A.
18 Dekany, Richard
19 Graham, Matthew J.
20 Hale, David
21 Kaplan, David
22 Kasliwal, Mansi M.
23 Miller, Adam A.
24 Niell, James D.
25 Patterson, Maria T.
26 Riddle, Reed
27 Smith, Roger
28 Soumagnac, Maayane T.
ORCID 1 0000-0003-4373-7777
 2 0000-0002-8257-9727
 3 0000-0002-9017-3567
 4
 5 0000-0002-2626-2872
 6
 7
 8 0000-0002-9154-3136
 9 0000-0001-8018-5348
10 0000-0002-7226-836X
11 0000-0002-6540-1484
12 0000-0002-8850-3627
13 0000-0002-8532-9395
14 0000-0001-7016-1692
15
16 0000-0002-8262-2924
17 0000-0003-2292-0441
18
19 0000-0002-3168-0139
20
21 0000-0001-6295-2881
22 0000-0002-5619-4938
23 0000-0001-9515-478X
24
25
26 0000-0002-0387-370X
27
28 0000-0001-6753-1488
Grupo 1
 2
 3
 4
 5
 6
 7 AST-CEA-SESPG-INPE-MCTIC-GOV-BR
Afiliação 1 University of Washington
 2 University of Washington
 3 California Institute of Technology
 4 California Institute of Technology
 5 California Institute of Technology
 6 University of Washington
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 University of Washington
 9 University of Washington
10 California Institute of Technology
11 University of California Santa Barbara
12 California Institute of Technology
13 California Institute of Technology
14 California Institute of Technology
15 University of Washington
16 California Institute of Technology
17 University of Maryland
18 California Institute of Technology
19 California Institute of Technology
20 California Institute of Technology
21 University of Wisconsin-Milwaukee
22 California Institute of Technology
23 Northwestern University
24 California Institute of Technology
25 High Alpha
26 California Institute of Technology
27 California Institute of Technology
28 Lawrence Berkeley National Lab
Endereço de e-Mail do Autor 1
 2
 3
 4
 5
 6
 7 isabel.lima@inpe.br
RevistaAstronomical Journal
Volume159
Número5
Páginase198
Nota SecundáriaA1_GEOCIÊNCIAS A2_INTERDISCIPLINAR A2_ASTRONOMIA_/_FÍSICA
Histórico (UTC)2020-06-25 11:11:44 :: simone -> administrator ::
2020-06-25 11:11:45 :: administrator -> simone :: 2020
2020-06-25 11:18:19 :: simone -> administrator :: 2020
2022-01-04 01:35:13 :: administrator -> simone :: 2020
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
ResumoUsing selection criteria based on amplitude, time, and color, we have identified 329 objects as known or candidate cataclysmic variables (CVs) during the first year of testing and operation of the Zwicky Transient Facility. Of these, 90 are previously confirmed CVs, 218 are strong candidates based on the shape and color of their light curves obtained during 3-562 days of observation, and the remaining 21 are possible CVs but with too few data points to be listed as good candidates. Almost half of the strong candidates are within 10 deg of the galactic plane, in contrast to most other large surveys that have avoided crowded fields. The available Gaia parallaxes are consistent with sampling the low mass transfer CVs, as predicted by population models. Our follow-up spectra have confirmed Balmer/helium emission lines in 27 objects, with four showing high-excitation He ii emission, including candidates for an AM CVn, a polar, and an intermediate polar. Our results demonstrate that a complete survey of the Galactic plane is needed to accomplish an accurate determination of the number of CVs existing in the Milky Way.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção pgr ATUAIS > AST > Cataclysmic variables in...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
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4. Condições de acesso e uso
Idiomaen
Arquivo AlvoSzkody_2020_AJ_159_198.pdf
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
simone
Visibilidadeshown
Política de Arquivamentodenypublisher denyfinaldraft
Permissão de Leituradeny from all and allow from 150.163
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3F2NE4L
DivulgaçãoWEBSCI; PORTALCAPES; SCOPUS.
Acervo Hospedeirourlib.net/www/2017/11.22.19.04
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn keywords label lineage mark mirrorrepository nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
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