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title: Data from JPL data

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title: Data from JPL data

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title: Data from JPL data

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description: Babylonian Diaries
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description: Babylonian Diaries
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title: Data from JPL data

description: Babylonian Diaries
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title: Data from JPL data

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title: Data from JPL data

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DOI: 10.17171/1-3-6126-21
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DOI: 10.17171/1-3-6126-22
title: 6126
title: Data from JPL data

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title: 6126
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description: Babylonian Diaries
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title: Data from JPL data

description: Babylonian Diaries
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DOI: 10.17171/1-3-6129-12
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description: Babylonian Diaries
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title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6129-20
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description: Babylonian Diaries
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title: Data from JPL data

description: Babylonian Diaries
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title: 6129
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description: Babylonian Diaries
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description: Babylonian Diaries
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DOI: 10.17171/1-3-6129-29
title: 6129
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description: Babylonian Diaries
DOI: 10.17171/1-3-6129-30
title: 6129
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6129-31
title: 6129
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6129-36
title: 6129
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6129-37
title: 6129
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description: Babylonian Diaries
DOI: 10.17171/1-3-6129-38
title: 6129
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6129-39
title: 6129
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-0
title: 6130
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-1
title: 6130
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description: Babylonian Diaries
DOI: 10.17171/1-3-6130-10
title: 6130
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-12
title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6130
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-16
title: 6130
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-18
title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6130
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-20
title: 6130
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-22
title: 6130
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-24
title: 6130
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-26
title: 6130
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-4
title: 6130
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-5
title: 6130
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-6
title: 6130
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-8
title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6130
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6130-27
title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6130
title: Data from JPL data

description: Babylonian Diaries
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title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-100
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-102
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-104
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-106
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-108
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-110
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-112
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-114
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-116
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-118
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-12
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-120
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-122
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-13
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.17171/1-3-6131-14
title: 6131
title: Data from JPL data

description: Babylonian Diaries
DOI: 10.25919/5d9062ab2bdd0
title: Parkes observations for project P1006 semester 2019APRS_19

description: We propose observations with the ultra-wide-bandwidth, low-frequency receiver installed at the Parkes telescope to carry out the first ultra-high time resolution, coherently de-dispersed search for pulsars in globular clusters. We have chosen the 11 most likely clusters for new discoveries. These clusters all have at least three pulsars already known allowing us to have a precise estimate of the pulsar dispersion measures and our observations will provide the first ultra-wide-bandwidth observation of these pulsars. Our observing strategy will enable us to search for extremely narrow pulsars and even pulsars with sub-millisecond periods.
DOI: 10.25606/surf.578c6039-76c505f8
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-476)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 476 of the 2048³ resolution collection.
DOI: 10.14457/cu.the.2006.1704
title: Thai and Vietnamese university students' language learning strategies

description: To investigate language learning strategies used by Thai and Vietnmese university students, to compare the use of the strategies by the two groups of students, and to study the influence of gender, motivation, and experience in studying English on their choice of the language learning strategies. The participants are 84 Thai and 52 Vietnamese first or second-year students at Chulalongkorn University, Thailand, and The University of Social Science and Humanities, Hanoi, Vietnam. The Strategy Inventory for Language Learning (SILL) developed by Oxford (1990) and semi-structured interviews are used as research instruments. Descriptive and inferential statistics are used to determine the rank of the strategies chosen and the relationship between the three variables and the choices of language learning strategies. The results of the analysis reveal that Thai students used compensation most, followed by cognitive, metacognitive, social, affective and memory strategy categories, respectively. As for Vietnamese students, the most frequently used strategy category is compensation, followed by social, metacognitive, affective, cognitive, and memory categories. The similarity of these two groups of students is that they use compensation category most, and memory category least. Concerning individual strategy, it is found that Thai students tend to guess meanings of unfamiliar words, use circumlocutions or synonyms, use glossaries or dictionaries, whereas Vietnamese students tend to encourage themselves to try harder, and pay attention when someone is speaking. The study also shows that motivation is the most significant factor factor affecting the choice of the strategies, followed by experience in studying English. Gender is the least significant factor. Furthermore, the analysis also shows that lowly-motivated and inexperienced Thai female students tend to use the six strategy categories less than their Vietnamese counterparts. The results of the study are useful particularly to educational planners, methodologists, and classroom teachers; they not only help them understand the strategies used by Thai students in learning English better, but also facilitate the process of improving English education in Thailand.
DOI: 10.25606/surf.578c6039-a2f55b83
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-683)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 683 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-e0a5cf27
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-211)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 211 of the 2048³ resolution collection.
DOI: 10.21227/ky6w-c031
title: Ruling Power Tautology: Error in Big Bang Theory

description: -If Ruling Power were able and willing to create Sun/Mars, he would do so. If Ruling Power were unable to create Sun/Mars, he would be incapable; if he were unwilling to create Sun/Mars, he would be malevolent. Ruling Power creates Sun/Mars. If Ruling Power exists, he is neither incapable nor malevolent. Therefore, Ruling Power exists. The World of PC can’t be created itself just from one factor light. I (programmer) die & consequently light (big bang) become useless.
DOI: 10.21227/nn8y-t779
title: Ruling Power Tautology: Error in Big Bang Theory

description: -If Ruling Power were able and willing to create Sun/Mars, he would do so. If Ruling Power were unable to create Sun/Mars, he would be incapable; if he were unwilling to create Sun/Mars, he would be malevolent. Ruling Power creates Sun/Mars. If Ruling Power exists, he is neither incapable nor malevolent. Therefore, Ruling Power exists. The World of PC can’t be created itself just from one factor light. I (programmer) die & consequently light (big bang) become useless.