Pub Date : 2017-02-01Epub Date: 2017-02-09DOI: 10.3847/1538-4365/228/2/19
Duane F Carbon, Christopher Henze, Bron C Nelson
We present the results of a search for EMP, CEMP, and cataclysmic variable stars using a new exploration tool based on linked scatter plots (LSPs). Our approach is especially designed to work with very large spectrum data sets such as the SDSS, LAMOST, RAVE, and Gaia data sets and can be applied to stellar, galaxy, and quasar spectra. As a demonstration, we conduct a search for EMP, CEMP, and cataclysmic variable stars in the SDSS DR10 data set. We first created a 3326-dimensional phase space containing nearly 2 billion measures of the strengths of over 1600 spectral features in 569,738 SDSS stars. These measures capture essentially all the stellar atomic and molecular species visible at the resolution of SDSS spectra. We show how LSPs can be used to quickly isolate and examine interesting portions of this phase space. To illustrate, we use LSPs coupled with cuts in selected portions of phase space to extract EMP stars, C-rich EMP stars, and CV stars. We present identifications for 59 previously unrecognized candidate EMP stars and 11 previously unrecognized candidate CEMP stars. We also call attention to 2 candidate He II emission CV stars found by the LSP approach that have not yet been discussed in the literature.
{"title":"Exploring the SDSS Dataset with Linked Scatter Plots: I. EMP, CEMP, and CV Stars.","authors":"Duane F Carbon, Christopher Henze, Bron C Nelson","doi":"10.3847/1538-4365/228/2/19","DOIUrl":"10.3847/1538-4365/228/2/19","url":null,"abstract":"<p><p>We present the results of a search for EMP, CEMP, and cataclysmic variable stars using a new exploration tool based on linked scatter plots (LSPs). Our approach is especially designed to work with very large spectrum data sets such as the SDSS, LAMOST, RAVE, and Gaia data sets and can be applied to stellar, galaxy, and quasar spectra. As a demonstration, we conduct a search for EMP, CEMP, and cataclysmic variable stars in the SDSS DR10 data set. We first created a 3326-dimensional phase space containing nearly 2 billion measures of the strengths of over 1600 spectral features in 569,738 SDSS stars. These measures capture essentially all the stellar atomic and molecular species visible at the resolution of SDSS spectra. We show how LSPs can be used to quickly isolate and examine interesting portions of this phase space. To illustrate, we use LSPs coupled with cuts in selected portions of phase space to extract EMP stars, C-rich EMP stars, and CV stars. We present identifications for 59 previously unrecognized candidate EMP stars and 11 previously unrecognized candidate CEMP stars. We also call attention to 2 candidate He II emission CV stars found by the LSP approach that have not yet been discussed in the literature.</p>","PeriodicalId":8588,"journal":{"name":"Astrophysical Journal Supplement Series","volume":"228 2","pages":""},"PeriodicalIF":8.6,"publicationDate":"2017-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5495198/pdf/nihms864022.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"35148527","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2017-01-01Epub Date: 2017-01-20DOI: 10.3847/1538-4365/228/1/10
J E Lawler, C Sneden, G Nave, E A Den Hartog, N Emrahođlu, J J Cowan
New emission branching fraction (BF) measurements for 183 lines of the second spectrum of chromium (Cr II) and new radiative lifetime measurements from laser-induced fluorescence for 8 levels of Cr+ are reported. The goals of this study are to improve transition probability measurements in Cr II and reconcile solar and stellar Cr abundance values based on Cr I and Cr II lines. Eighteen spectra from three Fourier Transform Spectrometers supplemented with ultraviolet spectra from a high-resolution echelle spectrometer are used in the BF measurements. Radiative lifetimes from this study and earlier publications are used to convert the BFs into absolute transition probabilities. These new laboratory data are applied to determine the Cr abundance log ε in the Sun and metal-poor star HD 84937. The mean result in the Sun is 〈logε (Cr II)〉 = 5.624±0.009 compared to 〈logε(Cr I)〉 = 5.644 ± 0.006 on a scale with the hydrogen abundance log ε(H) = 12 and with the uncertainty representing only line-to-line scatter. A Saha (ionization balance) test on the photosphere of HD 84937 is also performed, yielding 〈logε(Cr II)〉 = 3.417 ± 0.006 and 〈log ε(Cr I, lower level excitation potential E. P. >30 eV)〉 = 3.3743±30.011 for this dwarf star. We find a correlation of Cr with the iron-peak element Ti, suggesting an associated nucleosynthetic production. Four iron-peak elements (Cr along with Ti, V, and Sc) appear to have a similar (or correlated) production history-other iron-peak elements appear not to be associated with Cr.
{"title":"IMPROVED Cr II log(<i>gf</i> ) VALUES AND ABUNDANCE DETERMINATIONS IN THE PHOTOSPHERES OF THE SUN AND METAL-POOR STAR HD 84937.","authors":"J E Lawler, C Sneden, G Nave, E A Den Hartog, N Emrahođlu, J J Cowan","doi":"10.3847/1538-4365/228/1/10","DOIUrl":"10.3847/1538-4365/228/1/10","url":null,"abstract":"<p><p>New emission branching fraction (BF) measurements for 183 lines of the second spectrum of chromium (Cr II) and new radiative lifetime measurements from laser-induced fluorescence for 8 levels of Cr<sup>+</sup> are reported. The goals of this study are to improve transition probability measurements in Cr II and reconcile solar and stellar Cr abundance values based on Cr I and Cr II lines. Eighteen spectra from three Fourier Transform Spectrometers supplemented with ultraviolet spectra from a high-resolution echelle spectrometer are used in the BF measurements. Radiative lifetimes from this study and earlier publications are used to convert the BFs into absolute transition probabilities. These new laboratory data are applied to determine the Cr abundance log <i>ε</i> in the Sun and metal-poor star HD 84937. The mean result in the Sun is 〈log<i>ε</i> (Cr II)〉 = 5.624±0.009 compared to 〈log<i>ε</i>(Cr I)〉 = 5.644 ± 0.006 on a scale with the hydrogen abundance log <i>ε</i>(H) = 12 and with the uncertainty representing only line-to-line scatter. A Saha (ionization balance) test on the photosphere of HD 84937 is also performed, yielding 〈log<i>ε</i>(Cr II)〉 = 3.417 ± 0.006 and 〈log <i>ε</i>(Cr I, lower level excitation potential E. P. >30 eV)〉 = 3.3743±30.011 for this dwarf star. We find a correlation of Cr with the iron-peak element Ti, suggesting an associated nucleosynthetic production. Four iron-peak elements (Cr along with Ti, V, and Sc) appear to have a similar (or correlated) production history-other iron-peak elements appear not to be associated with Cr.</p>","PeriodicalId":8588,"journal":{"name":"Astrophysical Journal Supplement Series","volume":"228 1","pages":""},"PeriodicalIF":8.6,"publicationDate":"2017-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5455792/pdf/nihms856012.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"35060272","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2017-01-01DOI: 10.3847/1538-4365/aa656e
C. Lavín, A. M. Velasco
Theoretical transition energies and absorption oscillator strengths for the (v′ = 0–2, 5, 7, 8) − and (v′ = 0, 2) − (v″ = 0–14) Rydberg bands, and (v′ = 0–9, 11, 12, 14–19, 21, 22) − (v″ = 0–14) valence bands of molecular nitrogen are reported. The strong interaction between states has been dealt with through a vibronic interaction matrix. As a consequence of the Rydberg-valence interaction, irregularities in the vibrational structure of the above band systems are observed. Good agreement is found with the scarce high-resolution data that are available for oscillator strengths. The new band oscillator strengths reported here may be useful for a reliable interpretation of the spectra from atmospheres of the Earth, Titan, and Triton, where is the mayor constituent.
{"title":"Transition Energies and Absorption Oscillator Strengths for , , and Band Systems in N2","authors":"C. Lavín, A. M. Velasco","doi":"10.3847/1538-4365/aa656e","DOIUrl":"https://doi.org/10.3847/1538-4365/aa656e","url":null,"abstract":"Theoretical transition energies and absorption oscillator strengths for the (v′ = 0–2, 5, 7, 8) − and (v′ = 0, 2) − (v″ = 0–14) Rydberg bands, and (v′ = 0–9, 11, 12, 14–19, 21, 22) − (v″ = 0–14) valence bands of molecular nitrogen are reported. The strong interaction between states has been dealt with through a vibronic interaction matrix. As a consequence of the Rydberg-valence interaction, irregularities in the vibrational structure of the above band systems are observed. Good agreement is found with the scarce high-resolution data that are available for oscillator strengths. The new band oscillator strengths reported here may be useful for a reliable interpretation of the spectra from atmospheres of the Earth, Titan, and Triton, where is the mayor constituent.","PeriodicalId":8588,"journal":{"name":"Astrophysical Journal Supplement Series","volume":"229 1","pages":""},"PeriodicalIF":8.7,"publicationDate":"2017-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.3847/1538-4365/aa656e","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"70000806","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2016-05-13DOI: 10.3847/0067-0049/225/1/16
Xin Cheng, M. Ding
We investigate the footpoints of four erupted magnetic flux ropes (MFRs) that appear as sigmoidal hot channels prior to the eruptions in the Atmospheric Imaging Assembly high temperaure passbands. The simultaneous Helioseismic and Magnetic Imager observations disclose that one footpoint of the MFRs originates in the penumbra or penumbra edge with a stronger magnetic field, while the other in the moss region with a weaker magnetic field. The significant deviation of the axis of the MFRs from the main polarity inversion lines and associated filaments suggests that the MFRs have ascended to a high altitude, thus being distinguishable from the source sigmoidal ARs. The more interesting thing is that, with the eruption of the MFRs, the average inclination angle and direct current at the footpoints with stronger magnetic field tend to decrease, which is suggestive of a straightening and untwisting of the magnetic field in the MFR legs. Moreover, the associated flare ribbons also display an interesting evolution. They initially appear as sporadical brightenings at the two footpoints of and in the regions below the MFRs and then quickly extend to two slender sheared J-shaped ribbons with the two hooks corresponding to the two ends of the MFRs. Finally, the straight parts of the two ribbons separate from each other, evolving into two widened parallel ones. These features mostly conforms to and supports the recently proposed three-dimensional standard CME/flare model, i.e., the twisted MFR eruption stretches and leads to the reconnection of the overlying field that transits from a strong to weak shear with the increasing height.
{"title":"On the Characteristics of Footpoints of Solar Magnetic Flux Ropes during the Eruption","authors":"Xin Cheng, M. Ding","doi":"10.3847/0067-0049/225/1/16","DOIUrl":"https://doi.org/10.3847/0067-0049/225/1/16","url":null,"abstract":"We investigate the footpoints of four erupted magnetic flux ropes (MFRs) that appear as sigmoidal hot channels prior to the eruptions in the Atmospheric Imaging Assembly high temperaure passbands. The simultaneous Helioseismic and Magnetic Imager observations disclose that one footpoint of the MFRs originates in the penumbra or penumbra edge with a stronger magnetic field, while the other in the moss region with a weaker magnetic field. The significant deviation of the axis of the MFRs from the main polarity inversion lines and associated filaments suggests that the MFRs have ascended to a high altitude, thus being distinguishable from the source sigmoidal ARs. The more interesting thing is that, with the eruption of the MFRs, the average inclination angle and direct current at the footpoints with stronger magnetic field tend to decrease, which is suggestive of a straightening and untwisting of the magnetic field in the MFR legs. Moreover, the associated flare ribbons also display an interesting evolution. They initially appear as sporadical brightenings at the two footpoints of and in the regions below the MFRs and then quickly extend to two slender sheared J-shaped ribbons with the two hooks corresponding to the two ends of the MFRs. Finally, the straight parts of the two ribbons separate from each other, evolving into two widened parallel ones. These features mostly conforms to and supports the recently proposed three-dimensional standard CME/flare model, i.e., the twisted MFR eruption stretches and leads to the reconnection of the overlying field that transits from a strong to weak shear with the increasing height.","PeriodicalId":8588,"journal":{"name":"Astrophysical Journal Supplement Series","volume":"225 1","pages":"16"},"PeriodicalIF":8.7,"publicationDate":"2016-05-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.3847/0067-0049/225/1/16","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"70001217","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2016-02-01Epub Date: 2015-12-15DOI: 10.1210/en.2015-1645
Amanda L Mereness, Zachary C Murphy, Andrew C Forrestel, Susan Butler, CheMyong Ko, JoAnne S Richards, Michael T Sellix
Rhythmic events in female reproductive physiology, including ovulation, are tightly controlled by the circadian timing system. The molecular clock, a feedback loop oscillator of clock gene transcription factors, dictates rhythms of gene expression in the hypothalamo-pituitary-ovarian axis. Circadian disruption due to environmental factors (eg, shift work) or genetic manipulation of the clock has negative impacts on fertility. Although the central pacemaker in the suprachiasmatic nucleus classically regulates the timing of ovulation, we have shown that this rhythm also depends on phasic sensitivity to LH. We hypothesized that this rhythm relies on clock function in a specific cellular compartment of the ovarian follicle. To test this hypothesis we generated mice with deletion of the Bmal1 locus in ovarian granulosa cells (GCs) (Granulosa Cell Bmal1 KO; GCKO) or theca cells (TCs) (Theca Cell Bmal1 KO; TCKO). Reproductive cycles, preovulatory LH secretion, ovarian morphology and behavior were not grossly altered in GCKO or TCKO mice. We detected phasic sensitivity to LH in wild-type littermate control (LC) and GCKO mice but not TCKO mice. This decline in sensitivity to LH is coincident with impaired fertility and altered patterns of LH receptor (Lhcgr) mRNA abundance in the ovary of TCKO mice. These data suggest that the TC is a pacemaker that contributes to the timing and amplitude of ovulation by modulating phasic sensitivity to LH. The TC clock may play a critical role in circadian disruption-mediated reproductive pathology and could be a target for chronobiotic management of infertility due to environmental circadian disruption and/or hormone-dependent reprogramming in women.
{"title":"Conditional Deletion of Bmal1 in Ovarian Theca Cells Disrupts Ovulation in Female Mice.","authors":"Amanda L Mereness, Zachary C Murphy, Andrew C Forrestel, Susan Butler, CheMyong Ko, JoAnne S Richards, Michael T Sellix","doi":"10.1210/en.2015-1645","DOIUrl":"10.1210/en.2015-1645","url":null,"abstract":"<p><p>Rhythmic events in female reproductive physiology, including ovulation, are tightly controlled by the circadian timing system. The molecular clock, a feedback loop oscillator of clock gene transcription factors, dictates rhythms of gene expression in the hypothalamo-pituitary-ovarian axis. Circadian disruption due to environmental factors (eg, shift work) or genetic manipulation of the clock has negative impacts on fertility. Although the central pacemaker in the suprachiasmatic nucleus classically regulates the timing of ovulation, we have shown that this rhythm also depends on phasic sensitivity to LH. We hypothesized that this rhythm relies on clock function in a specific cellular compartment of the ovarian follicle. To test this hypothesis we generated mice with deletion of the Bmal1 locus in ovarian granulosa cells (GCs) (Granulosa Cell Bmal1 KO; GCKO) or theca cells (TCs) (Theca Cell Bmal1 KO; TCKO). Reproductive cycles, preovulatory LH secretion, ovarian morphology and behavior were not grossly altered in GCKO or TCKO mice. We detected phasic sensitivity to LH in wild-type littermate control (LC) and GCKO mice but not TCKO mice. This decline in sensitivity to LH is coincident with impaired fertility and altered patterns of LH receptor (Lhcgr) mRNA abundance in the ovary of TCKO mice. These data suggest that the TC is a pacemaker that contributes to the timing and amplitude of ovulation by modulating phasic sensitivity to LH. The TC clock may play a critical role in circadian disruption-mediated reproductive pathology and could be a target for chronobiotic management of infertility due to environmental circadian disruption and/or hormone-dependent reprogramming in women. </p>","PeriodicalId":8588,"journal":{"name":"Astrophysical Journal Supplement Series","volume":"49 1","pages":"913-27"},"PeriodicalIF":4.8,"publicationDate":"2016-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1210/en.2015-1645","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"82616977","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2015-11-27DOI: 10.1002/14651858.CD009736.pub2
Katie Gillies, Seonaidh C Cotton, Jamie C Brehaut, Mary C Politi, Zoe Skea
Background: Several interventions have been developed to promote informed consent for participants in clinical trials. However, many of these interventions focus on the content and structure of information (e.g. enhanced information or changes to the presentation format) rather than the process of decision making. Patient decision aids support a decision making process about medical options. Decision aids support the decision process by providing information about available options and their associated outcomes, alongside information that enables patients to consider what value they place on particular outcomes, and provide structured guidance on steps of decision making. They have been shown to be effective for treatment and screening decisions but evidence on their effectiveness in the context of informed consent for clinical trials has not been synthesised.
Objectives: To assess the effectiveness of decision aids for clinical trial informed consent compared to no intervention, standard information (i.e. usual practice) or an alternative intervention on the decision making process.
Search methods: We searched the following databases and to March 2015: Cochrane Central Register of Controlled Trials (CENTRAL), The Cochrane Library; MEDLINE (OvidSP) (from 1950); EMBASE (OvidSP) (from 1980); PsycINFO (OvidSP) (from 1806); ASSIA (ProQuest) (from 1987); WHO International Clinical Trials Registry Platform (ICTRP) (http://apps.who.int/trialsearch/); ClinicalTrials.gov; ISRCTN Register (http://www.controlled-trials.com/isrctn/). We also searched reference lists of included studies and relevant reviews. We contacted study authors and other experts. There were no language restrictions.
Selection criteria: We included randomised and quasi-randomised controlled trials comparing decision aids in the informed consent process for clinical trials alone, or in conjunction with standard information (such as written or verbal) or alongside alternative interventions (e.g. paper-based versus web-based decision aids). Included trials involved potential trial participants, or their guardians, being asked to consider participating in a real or hypothetical clinical trial.
Data collection and analysis: At least two authors independently assessed studies for inclusion, extracted reported data and assessed risk of bias. Findings were pooled where appropriate. We used GRADE to assess the quality of the evidence for each outcome.
Main results: We identified one study (290 randomised participants) that investigated the effectiveness of decision aids compared to standard information in the informed consent process for clinical trials. This study reported two separate decision aid randomised controlled trials (RCTs). The decision aid trials were nested within two different parent trials focusing on breast cancer in postmenopausal women. One tri
背景:为促进临床试验参与者的知情同意,已经制定了一些干预措施。然而,这些干预措施大多侧重于信息的内容和结构(如增强信息或改变演示格式),而不是决策过程。患者决策辅助工具支持有关医疗选择的决策过程。决策辅助工具通过提供有关现有选择及其相关结果的信息,以及使患者能够考虑其对特定结果的价值的信息,来支持决策过程,并为决策步骤提供结构化指导。这些辅助工具已被证明对治疗和筛查决策有效,但有关其在临床试验知情同意方面的有效性的证据尚未汇总:评估临床试验知情同意决策辅助工具与无干预措施、标准信息(即常规做法)或其他干预措施相比在决策过程中的有效性:截至 2015 年 3 月,我们检索了以下数据库:Cochrane 图书馆的 Cochrane Central Register of Controlled Trials (CENTRAL);MEDLINE (OvidSP)(1950 年起);EMBASE (OvidSP)(1980 年起);PsycINFO (OvidSP)(1806 年起);ASSIA (ProQuest)(1987 年起);WHO International Clinical Trials Registry Platform (ICTRP) (http://apps.who.int/trialsearch/);ClinicalTrials.gov;ISRCTN Register (http://www.controlled-trials.com/isrctn/)。我们还检索了纳入研究的参考文献目录和相关综述。我们还联系了研究报告的作者和其他专家。没有语言限制:我们纳入了随机和准随机对照试验,这些试验比较了临床试验知情同意程序中的决策辅助工具单独使用、与标准信息(如书面或口头信息)结合使用或与其他干预措施(如纸质决策辅助工具与网络决策辅助工具)结合使用的情况。纳入的试验涉及要求潜在试验参与者或其监护人考虑参与真实或假设的临床试验:至少有两名作者独立评估研究是否纳入、提取报告数据并评估偏倚风险。在适当的情况下对研究结果进行汇总。我们使用 GRADE 对每项结果的证据质量进行了评估:我们发现一项研究(290 名随机参与者)调查了决策辅助工具与临床试验知情同意程序中标准信息的有效性比较。该研究报告了两项独立的决策辅助随机对照试验(RCT)。决策辅助工具试验嵌套在两个不同的母试验中,重点是绝经后妇女的乳腺癌。其中一项试验的重点是曾接受过乳腺导管原位癌(DCIS)手术的妇女在治疗方面的知情同意,另一项试验的重点是乳腺癌高危妇女在预防方面的知情同意。这些 RCT 中使用了两种不同的决策辅助工具,并与标准信息进行了比较。汇总的研究结果突显了大多数报告结果的不确定性,包括知识、决策冲突、焦虑、试验参与和自然减员。有极低质量的证据表明,决策辅助工具在很小程度上降低了决策后悔的程度(MD -5.53,95% CI -10.29至-0.76)。关于几项预先指定的主要结果,包括准确的风险认知、基于价值观的决策,或潜在参与者是否认识到需要做出决策、能否识别对个人而言最重要的选项特征或是否参与决策,均未找到相关数据:目前尚无充分证据表明,用于支持临床试验知情同意程序的决策辅助工具是否比标准信息更有效。需要在更多不同的临床和社会人群中开展更多设计合理、有充分证据支持的临床试验,以加强本综述的结果。从更广泛的意义上讲,未来对哪些结果最适合在这种情况下进行评估的研究将有所帮助。
{"title":"Decision aids for people considering taking part in clinical trials.","authors":"Katie Gillies, Seonaidh C Cotton, Jamie C Brehaut, Mary C Politi, Zoe Skea","doi":"10.1002/14651858.CD009736.pub2","DOIUrl":"10.1002/14651858.CD009736.pub2","url":null,"abstract":"<p><strong>Background: </strong>Several interventions have been developed to promote informed consent for participants in clinical trials. However, many of these interventions focus on the content and structure of information (e.g. enhanced information or changes to the presentation format) rather than the process of decision making. Patient decision aids support a decision making process about medical options. Decision aids support the decision process by providing information about available options and their associated outcomes, alongside information that enables patients to consider what value they place on particular outcomes, and provide structured guidance on steps of decision making. They have been shown to be effective for treatment and screening decisions but evidence on their effectiveness in the context of informed consent for clinical trials has not been synthesised.</p><p><strong>Objectives: </strong>To assess the effectiveness of decision aids for clinical trial informed consent compared to no intervention, standard information (i.e. usual practice) or an alternative intervention on the decision making process.</p><p><strong>Search methods: </strong>We searched the following databases and to March 2015: Cochrane Central Register of Controlled Trials (CENTRAL), The Cochrane Library; MEDLINE (OvidSP) (from 1950); EMBASE (OvidSP) (from 1980); PsycINFO (OvidSP) (from 1806); ASSIA (ProQuest) (from 1987); WHO International Clinical Trials Registry Platform (ICTRP) (http://apps.who.int/trialsearch/); ClinicalTrials.gov; ISRCTN Register (http://www.controlled-trials.com/isrctn/). We also searched reference lists of included studies and relevant reviews. We contacted study authors and other experts. There were no language restrictions.</p><p><strong>Selection criteria: </strong>We included randomised and quasi-randomised controlled trials comparing decision aids in the informed consent process for clinical trials alone, or in conjunction with standard information (such as written or verbal) or alongside alternative interventions (e.g. paper-based versus web-based decision aids). Included trials involved potential trial participants, or their guardians, being asked to consider participating in a real or hypothetical clinical trial.</p><p><strong>Data collection and analysis: </strong>At least two authors independently assessed studies for inclusion, extracted reported data and assessed risk of bias. Findings were pooled where appropriate. We used GRADE to assess the quality of the evidence for each outcome.</p><p><strong>Main results: </strong>We identified one study (290 randomised participants) that investigated the effectiveness of decision aids compared to standard information in the informed consent process for clinical trials. This study reported two separate decision aid randomised controlled trials (RCTs). The decision aid trials were nested within two different parent trials focusing on breast cancer in postmenopausal women. One tri","PeriodicalId":8588,"journal":{"name":"Astrophysical Journal Supplement Series","volume":"64 1","pages":"CD009736"},"PeriodicalIF":8.6,"publicationDate":"2015-11-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8725643/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"82640038","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2015-06-01DOI: 10.1088/00647-0049/218/2/15
M. Kriek, A. Shapley, N. Reddy, B. Siana, A. Coil, B. Mobasher, W. Freeman, L. D. Groot, S. Price, R. Sanders, I. Shivaei, G. Brammer, I. Momcheva, R. Skelton, P. Dokkum, K. Whitaker, J. Aird, Mojegan Azadi, M. Kassis, J. Bullock, C. Conroy, R. Davé, D. Keres̆, M. Krumholz
Author(s): Kriek, Mariska; Shapley, Alice E; Reddy, Naveen A; Siana, Brian; Coil, Alison L; Mobasher, Bahram; Freeman, William R; de Groot, Laura; Price, Sedona H; Sanders, Ryan; Shivaei, Irene; Brammer, Gabriel B; Momcheva, Ivelina G; Skelton, Rosalind E; van Dokkum, Pieter G; Whitaker, Katherine E; Aird, James; Azadi, Mojegan; Kassis, Marc; Bullock, James S; Conroy, Charlie; Dave, Romeel; Keres, Dusan; Krumholz, Mark
作者:Kriek, Mariska;Alice E . Shapley;Reddy, Naveen A;布莱恩Siana;线圈,艾莉森·L;Mobasher检测;威廉·弗里曼;劳拉·德·格鲁特;塞多娜·H·普莱斯;桑德斯,瑞安;艾琳Shivaei;加布里埃尔·B·布拉默;艾维琳娜·蒙切娃;斯克尔顿,罗莎琳德·E;范多库姆,彼得·G;凯瑟琳·惠特克;Aird,詹姆斯;阿扎迪,Mojegan;Kassis,马克;詹姆斯·布洛克;康罗伊,查理;戴夫,Romeel;凯瑞斯语,科维奇;Krumholz,马克
{"title":"THE MOSFIRE DEEP EVOLUTION FIELD (MOSDEF) SURVEY: REST-FRAME OPTICAL SPECTROSCOPY FOR similar to 1500 H-SELECTED GALAXIES AT 1.37 <= z <= 3.8","authors":"M. Kriek, A. Shapley, N. Reddy, B. Siana, A. Coil, B. Mobasher, W. Freeman, L. D. Groot, S. Price, R. Sanders, I. Shivaei, G. Brammer, I. Momcheva, R. Skelton, P. Dokkum, K. Whitaker, J. Aird, Mojegan Azadi, M. Kassis, J. Bullock, C. Conroy, R. Davé, D. Keres̆, M. Krumholz","doi":"10.1088/00647-0049/218/2/15","DOIUrl":"https://doi.org/10.1088/00647-0049/218/2/15","url":null,"abstract":"Author(s): Kriek, Mariska; Shapley, Alice E; Reddy, Naveen A; Siana, Brian; Coil, Alison L; Mobasher, Bahram; Freeman, William R; de Groot, Laura; Price, Sedona H; Sanders, Ryan; Shivaei, Irene; Brammer, Gabriel B; Momcheva, Ivelina G; Skelton, Rosalind E; van Dokkum, Pieter G; Whitaker, Katherine E; Aird, James; Azadi, Mojegan; Kassis, Marc; Bullock, James S; Conroy, Charlie; Dave, Romeel; Keres, Dusan; Krumholz, Mark","PeriodicalId":8588,"journal":{"name":"Astrophysical Journal Supplement Series","volume":"218 1","pages":""},"PeriodicalIF":8.7,"publicationDate":"2015-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"60355198","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
The WISE All-Sky Survey Catalog presents an opportunity to expand the number of detections of warm (>100K) circumstellar dust in asteroid belt-analog regions. Such detections are useful to statistically constrain the occurrence rate of dusty systems, and imaging campaigns aiming to characterize the morphology of the dust populations can choose their targets form the nearest ( 30μm excesses (289, with 171 in common), even if the latter have been found to have a higher occurrence rate. 114 Finding Warm Debris Disks with WISE Around Bright Stars
{"title":"Finding Warm Debris Disks with WISE Around Bright Stars","authors":"R. Patel, A. Heinze, S. Metchev","doi":"10.5281/ZENODO.10573","DOIUrl":"https://doi.org/10.5281/ZENODO.10573","url":null,"abstract":"The WISE All-Sky Survey Catalog presents an opportunity to expand the number of detections of warm (>100K) circumstellar dust in asteroid belt-analog regions. Such detections are useful to statistically constrain the occurrence rate of dusty systems, and imaging campaigns aiming to characterize the morphology of the dust populations can choose their targets form the nearest ( 30μm excesses (289, with 171 in common), even if the latter have been found to have a higher occurrence rate. 114 Finding Warm Debris Disks with WISE Around Bright Stars","PeriodicalId":8588,"journal":{"name":"Astrophysical Journal Supplement Series","volume":"69 1","pages":""},"PeriodicalIF":8.7,"publicationDate":"2014-06-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"71020560","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2014-01-01DOI: 10.1088/0067-0049/210/2/25
Ji-Wei 伟 Xie 谢基
Following on from Paper I in this series, I report the confirmation of a further 30 planets in 15 multiple-planet systems via transit timing variations (TTVs), using the publicly available Kepler light curves (Q0–Q16). All 15 pairs are near first-order mean motion resonances, showing sinusoidal TTVs consistent with theoretically predicted periods, which demonstrate they are orbiting and interacting in the same systems. Although individual masses cannot be accurately extracted based only on TTVs (because of the well known degeneracy between mass and eccentricity), the measured TTV phases and amplitudes can still place relatively tight constraints on their mass ratios and upper limits on their masses, which confirm their planetary nature. Some of these systems (KOI-274, KOI-285, KOI-370, and KOI-2672) are relatively bright and thus suitable for further follow-up observations.
{"title":"TRANSIT TIMING VARIATION OF NEAR-RESONANCE PLANETARY PAIRS. II. CONFIRMATION OF 30 PLANETS IN 15 MULTIPLE-PLANET SYSTEMS","authors":"Ji-Wei 伟 Xie 谢基","doi":"10.1088/0067-0049/210/2/25","DOIUrl":"https://doi.org/10.1088/0067-0049/210/2/25","url":null,"abstract":"Following on from Paper I in this series, I report the confirmation of a further 30 planets in 15 multiple-planet systems via transit timing variations (TTVs), using the publicly available Kepler light curves (Q0–Q16). All 15 pairs are near first-order mean motion resonances, showing sinusoidal TTVs consistent with theoretically predicted periods, which demonstrate they are orbiting and interacting in the same systems. Although individual masses cannot be accurately extracted based only on TTVs (because of the well known degeneracy between mass and eccentricity), the measured TTV phases and amplitudes can still place relatively tight constraints on their mass ratios and upper limits on their masses, which confirm their planetary nature. Some of these systems (KOI-274, KOI-285, KOI-370, and KOI-2672) are relatively bright and thus suitable for further follow-up observations.","PeriodicalId":8588,"journal":{"name":"Astrophysical Journal Supplement Series","volume":"210 1","pages":""},"PeriodicalIF":8.7,"publicationDate":"2014-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1088/0067-0049/210/2/25","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"60356681","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}