cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.3255081
title: IMRPhenomD_NRTidal_128s

description: Contains data for linear and quadratic parts of the ROQ. Parameter ranges are specified in the params.dat file.

B_linear: EIM "B matrix" for the linear roq of the likelihood function

B_quadratic: EIM "B matrix" for the quadratic roq of the likelihood function

fnodes_linear: EIM frequency nodes for the linear roq of the likelihood function

fnodes_quadratic: EIM frequency nodes for the quadratic roq of the likelihood function
description: {"references": ["https://doi.org/10.1103/PhysRevD.94.044031"]}
DOI: 10.14272/onzumvhqtbbloc-ksrietaesa-n.1
title: C30H37Cl3FNO13
title: InChI=1S/C30H37Cl3FNO13/c1-5-11-42-27-21(35-29(40)30(31,32)33)24(23(43-15(2)36)20(47-27)14-41-13-18-9-7-6-8-10-18)48-28-26(45-17(4)38)25(44-16(3)37)22(39)19(12-34)46-28/h5-10,19-28,39H,1,11-14H2,2-4H3,(H,35,40)/t19?,20?,21?,22-,23-,24-,25+,26?,27-,28+/m1/s1

description: This dataset contains experimental data from a sample (InChI=1S/C30H37Cl3FNO13/c1-5-11-42-27-21(35-29(40)30(31,32)33)24(23(43-15(2)36)20(47-27)14-41-13-18-9-7-6-8-10-18)48-28-26(45-17(4)38)25(44-16(3)37)22(39)19(12-34)46-28/h5-10,19-28,39H,1,11-14H2,2-4H3,(H,35,40)/t19?,20?,21?,22-,23-,24-,25+,26?,27-,28+/m1/s1).
      The datasets from the following experiments are available:
      
      IR
DOI: 10.14272/onzumvhqtbbloc-ksrietaesa-n/ir
title: IR (, InChI=1S/C30H37Cl3FNO13/c1-5-11-42-27-21(35-29(40)30(31,32)33)24(23(43-15(2)36)20(47-27)14-41-13-18-9-7-6-8-10-18)48-28-26(45-17(4)38)25(44-16(3)37)22(39)19(12-34)46-28/h5-10,19-28,39H,1,11-14H2,2-4H3,(H,35,40)/t19?,20?,21?,22-,23-,24-,25+,26?,27-,28+/m1/s1)

description: dataset for IR
      
      IR (ATR, ṽ) = 2936, 2871, 1749, 1717, 1653, 1540, 1523, 1509, 1456, 1436, 1422, 1371, 1317, 1221, 1162, 1118, 1051, 1037, 931, 912, 837, 822, 756, 742, 698, 673, 654, 632, 602, 565, 492, 475, 442, 384 cm–1.
DOI: 10.14272/vwfqzaufgduffv-kgwxupnosa-n.1
title: C30H40FNO13
title: InChI=1S/C30H40FNO13/c1-6-12-39-29-23(32-16(2)33)26(25(40-17(3)34)22(44-29)15-38-14-20-10-8-7-9-11-20)45-30-28(42-19(5)36)27(41-18(4)35)24(37)21(13-31)43-30/h6-11,21-30,37H,1,12-15H2,2-5H3,(H,32,33)/t21?,22?,23?,24-,25-,26-,27+,28?,29-,30+/m1/s1

description: This dataset contains experimental data from a sample (InChI=1S/C30H40FNO13/c1-6-12-39-29-23(32-16(2)33)26(25(40-17(3)34)22(44-29)15-38-14-20-10-8-7-9-11-20)45-30-28(42-19(5)36)27(41-18(4)35)24(37)21(13-31)43-30/h6-11,21-30,37H,1,12-15H2,2-5H3,(H,32,33)/t21?,22?,23?,24-,25-,26-,27+,28?,29-,30+/m1/s1).
      The datasets from the following experiments are available:
      
      IR
DOI: 10.14272/vwfqzaufgduffv-kgwxupnosa-n/ir
title: IR (, InChI=1S/C30H40FNO13/c1-6-12-39-29-23(32-16(2)33)26(25(40-17(3)34)22(44-29)15-38-14-20-10-8-7-9-11-20)45-30-28(42-19(5)36)27(41-18(4)35)24(37)21(13-31)43-30/h6-11,21-30,37H,1,12-15H2,2-5H3,(H,32,33)/t21?,22?,23?,24-,25-,26-,27+,28?,29-,30+/m1/s1)

description: dataset for IR
      
      IR (ATR, ṽ) = 1748, 1734, 1653, 1558, 1541, 1523, 1507, 1456, 1431, 1419, 1371, 1227, 1159, 1115, 1084, 1050, 931, 911, 741, 698, 601, 561, 487 cm–1.
DOI: 10.14272/zmgydkiqpmhmeg-ugylpvgzsa-n.1
title: C35H43Cl3INO15
title: InChI=1S/C35H43Cl3INO15/c1-6-14-48-32-26(40-34(46)35(36,37)38)29(28(49-19(3)42)24(53-32)17-47-16-22-10-8-7-9-11-22)55-33-31(51-21(5)44)30(50-20(4)43)27(23(15-39)52-33)54-25(45)13-12-18(2)41/h6-11,23-24,26-33H,1,12-17H2,2-5H3,(H,40,46)/t23?,24?,26?,27-,28-,29-,30+,31?,32-,33+/m1/s1

description: This dataset contains experimental data from a sample (InChI=1S/C35H43Cl3INO15/c1-6-14-48-32-26(40-34(46)35(36,37)38)29(28(49-19(3)42)24(53-32)17-47-16-22-10-8-7-9-11-22)55-33-31(51-21(5)44)30(50-20(4)43)27(23(15-39)52-33)54-25(45)13-12-18(2)41/h6-11,23-24,26-33H,1,12-17H2,2-5H3,(H,40,46)/t23?,24?,26?,27-,28-,29-,30+,31?,32-,33+/m1/s1).
      The datasets from the following experiments are available:
      
      IR
DOI: 10.3886/e101760v2-12185
title: Housing and Urban Development: Family Unification Program Youth Data

description: In 2012, Mathematica Policy Research developed and fielded two surveys for the U.S. Department of Housing and Urban Development (HUD), under the project Housing for Youth Aging Out of Foster Care. The surveys were administered to providers of Family Unification Program (FUP) vouchers. They were designed to address the extent to which and how FUP vouchers are being used to provide housing for youth aging out of foster care. This study includes the public data from the Family Unification Program that was used in the production of HUD's study titled Housing For Youth Aging Out of Foster Care .<br><br>
description: These datasets were based on surveys administered to providers of HUD's Family Unification Program (FUP) vouchers.
DOI: 10.5281/zenodo.3260167
title: Organic aerosol source apportionment in Zurich using extractive electrospray ionization time-of-flight mass spectrometry (EESI-TOF): Part I, biogenic influences and day/night chemistry in summer

description: Ambient measurement campaign took place during summer 2016 in Zurich. The sources of organic aerosol were disclosed. The novel extractive electrospray ionization time-of-flight mass spectrometer (EESI-TOF) could provide direct chemical evidence linking ambient SOA to its precursor emissions including a strong influence of biogenic emissions. Additionally provided some insight into the day/night reaction environment and high-detailed chemical composition.
DOI: 10.5281/zenodo.3260168
title: Organic aerosol source apportionment in Zurich using extractive electrospray ionization time-of-flight mass spectrometry (EESI-TOF): Part I, biogenic influences and day/night chemistry in summer

description: Ambient measurement campaign took place during summer 2016 in Zurich. The sources of organic aerosol were disclosed. The novel extractive electrospray ionization time-of-flight mass spectrometer (EESI-TOF) could provide direct chemical evidence linking ambient SOA to its precursor emissions including a strong influence of biogenic emissions. Additionally provided some insight into the day/night reaction environment and high-detailed chemical composition.
DOI: 10.14272/aezwfidftkgwhz-kclgdljqsa-n.1
title: C35H44Cl3NO15
title: InChI=1S/C35H44Cl3NO15/c1-7-15-47-32-26(39-34(45)35(36,37)38)29(28(49-20(4)41)24(52-32)17-46-16-23-11-9-8-10-12-23)54-33-31(51-22(6)43)30(50-21(5)42)27(19(3)48-33)53-25(44)14-13-18(2)40/h7-12,19,24,26-33H,1,13-17H2,2-6H3,(H,39,45)/t19?,24?,26?,27-,28-,29-,30+,31?,32-,33+/m1/s1

description: This dataset contains experimental data from a sample (InChI=1S/C35H44Cl3NO15/c1-7-15-47-32-26(39-34(45)35(36,37)38)29(28(49-20(4)41)24(52-32)17-46-16-23-11-9-8-10-12-23)54-33-31(51-22(6)43)30(50-21(5)42)27(19(3)48-33)53-25(44)14-13-18(2)40/h7-12,19,24,26-33H,1,13-17H2,2-6H3,(H,39,45)/t19?,24?,26?,27-,28-,29-,30+,31?,32-,33+/m1/s1).
      The datasets from the following experiments are available:
      
      IR
DOI: 10.14272/aezwfidftkgwhz-kclgdljqsa-n/ir
title: IR (, InChI=1S/C35H44Cl3NO15/c1-7-15-47-32-26(39-34(45)35(36,37)38)29(28(49-20(4)41)24(52-32)17-46-16-23-11-9-8-10-12-23)54-33-31(51-22(6)43)30(50-21(5)42)27(19(3)48-33)53-25(44)14-13-18(2)40/h7-12,19,24,26-33H,1,13-17H2,2-6H3,(H,39,45)/t19?,24?,26?,27-,28-,29-,30+,31?,32-,33+/m1/s1)

description: dataset for IR
      
      IR (ATR, ṽ) = 3332, 2928, 2880, 1749, 1734, 1717, 1540, 1523, 1509, 1456, 1418, 1367, 1217, 1150, 1125, 1099, 1055, 1030, 916, 902, 837, 820, 756, 698, 673, 602, 486 cm–1.
DOI: 10.14272/mhuscjjxlccvlt-mkvhhkbrsa-n.1
title: C35H42Cl3N5O15
title: InChI=1S/C35H42Cl3N5O15/c1-6-14-51-32-24(39-34(49)35(36,37)38)26(25(52-18(3)45)22(55-32)16-50-15-21-10-8-7-9-11-21)57-33-30(54-20(5)47)28(53-19(4)46)27(56-23(48)13-12-17(2)44)29(58-33)31-40-42-43-41-31/h6-11,22,24-30,32-33H,1,12-16H2,2-5H3,(H,39,49)(H,40,41,42,43)/t22?,24?,25-,26-,27+,28+,29?,30?,32-,33-/m1/s1

description: This dataset contains experimental data from a sample (InChI=1S/C35H42Cl3N5O15/c1-6-14-51-32-24(39-34(49)35(36,37)38)26(25(52-18(3)45)22(55-32)16-50-15-21-10-8-7-9-11-21)57-33-30(54-20(5)47)28(53-19(4)46)27(56-23(48)13-12-17(2)44)29(58-33)31-40-42-43-41-31/h6-11,22,24-30,32-33H,1,12-16H2,2-5H3,(H,39,49)(H,40,41,42,43)/t22?,24?,25-,26-,27+,28+,29?,30?,32-,33-/m1/s1).
      The datasets from the following experiments are available:
      
      IR
DOI: 10.14272/mhuscjjxlccvlt-mkvhhkbrsa-n/ir
title: IR (, InChI=1S/C35H42Cl3N5O15/c1-6-14-51-32-24(39-34(49)35(36,37)38)26(25(52-18(3)45)22(55-32)16-50-15-21-10-8-7-9-11-21)57-33-30(54-20(5)47)28(53-19(4)46)27(56-23(48)13-12-17(2)44)29(58-33)31-40-42-43-41-31/h6-11,22,24-30,32-33H,1,12-16H2,2-5H3,(H,39,49)(H,40,41,42,43)/t22?,24?,25-,26-,27+,28+,29?,30?,32-,33-/m1/s1)

description: dataset for IR
      
      IR (ATR, ṽ) = 2924, 2876, 1749, 1717, 1653, 1647, 1558, 1540, 1523, 1509, 1456, 1429, 1419, 1405, 1368, 1227, 1214, 1146, 1040, 933, 912, 837, 822, 755, 742, 698, 673, 666, 629, 619, 602, 581, 564, 486, 398 cm–1.
DOI: 10.14272/txcsgofpwynwnq-irxsfqpesa-n.1
title: C34H44Cl3NO15S
title: InChI=1S/C34H44Cl3NO15S/c1-6-54-32-25(38-33(45)34(35,36)37)28(27(47-18(3)41)23(51-32)16-46-15-21-10-8-7-9-11-21)53-31-30(49-20(5)43)29(48-19(4)42)26(22(14-39)50-31)52-24(44)13-12-17(2)40/h7-11,22-23,25-32,39H,6,12-16H2,1-5H3,(H,38,45)/t22?,23?,25?,26-,27-,28-,29+,30?,31+,32+/m1/s1

description: This dataset contains experimental data from a sample (InChI=1S/C34H44Cl3NO15S/c1-6-54-32-25(38-33(45)34(35,36)37)28(27(47-18(3)41)23(51-32)16-46-15-21-10-8-7-9-11-21)53-31-30(49-20(5)43)29(48-19(4)42)26(22(14-39)50-31)52-24(44)13-12-17(2)40/h7-11,22-23,25-32,39H,6,12-16H2,1-5H3,(H,38,45)/t22?,23?,25?,26-,27-,28-,29+,30?,31+,32+/m1/s1).
      The datasets from the following experiments are available:
      
      IR
DOI: 10.14272/txcsgofpwynwnq-irxsfqpesa-n/ir
title: IR (, InChI=1S/C34H44Cl3NO15S/c1-6-54-32-25(38-33(45)34(35,36)37)28(27(47-18(3)41)23(51-32)16-46-15-21-10-8-7-9-11-21)53-31-30(49-20(5)43)29(48-19(4)42)26(22(14-39)50-31)52-24(44)13-12-17(2)40/h7-11,22-23,25-32,39H,6,12-16H2,1-5H3,(H,38,45)/t22?,23?,25?,26-,27-,28-,29+,30?,31+,32+/m1/s1)

description: dataset for IR
      
      IR (ATR, ṽ) = 2928, 2871, 1749, 1717, 1558, 1540, 1533, 1523, 1509, 1456, 1429, 1419, 1397, 1367, 1217, 1153, 1113, 1038, 902, 836, 822, 754, 698, 662, 626, 620, 602 cm–1.
DOI: 10.14272/xjwjekcatjzecp-wwojfqdfsa-n.1
title: C24H34FNO10
title: InChI=1S/C24H34FNO10/c1-3-9-33-23-17(26-13(2)27)22(36-24-21(31)20(30)18(28)15(10-25)34-24)19(29)16(35-23)12-32-11-14-7-5-4-6-8-14/h3-8,15-24,28-31H,1,9-12H2,2H3,(H,26,27)/t15?,16?,17?,18-,19-,20+,21?,22-,23-,24+/m1/s1

description: This dataset contains experimental data from a sample (InChI=1S/C24H34FNO10/c1-3-9-33-23-17(26-13(2)27)22(36-24-21(31)20(30)18(28)15(10-25)34-24)19(29)16(35-23)12-32-11-14-7-5-4-6-8-14/h3-8,15-24,28-31H,1,9-12H2,2H3,(H,26,27)/t15?,16?,17?,18-,19-,20+,21?,22-,23-,24+/m1/s1).
      The datasets from the following experiments are available:
      
      IR
DOI: 10.14272/xjwjekcatjzecp-wwojfqdfsa-n/ir
title: IR (, InChI=1S/C24H34FNO10/c1-3-9-33-23-17(26-13(2)27)22(36-24-21(31)20(30)18(28)15(10-25)34-24)19(29)16(35-23)12-32-11-14-7-5-4-6-8-14/h3-8,15-24,28-31H,1,9-12H2,2H3,(H,26,27)/t15?,16?,17?,18-,19-,20+,21?,22-,23-,24+/m1/s1)

description: dataset for IR
      
      IR (ATR, ṽ) = 3336, 2877, 1669, 1663, 1653, 1647, 1636, 1623, 1557, 1541, 1456, 1374, 1364, 1312, 1238, 1163, 1111, 1064, 1011, 984, 949, 938, 919, 895, 749, 698, 592, 517, 486, 473, 418, 397, 382 cm–1.
DOI: 10.14272/zmgydkiqpmhmeg-ugylpvgzsa-n/ir
title: IR (, InChI=1S/C35H43Cl3INO15/c1-6-14-48-32-26(40-34(46)35(36,37)38)29(28(49-19(3)42)24(53-32)17-47-16-22-10-8-7-9-11-22)55-33-31(51-21(5)44)30(50-20(4)43)27(23(15-39)52-33)54-25(45)13-12-18(2)41/h6-11,23-24,26-33H,1,12-17H2,2-5H3,(H,40,46)/t23?,24?,26?,27-,28-,29-,30+,31?,32-,33+/m1/s1)

description: dataset for IR
      
      IR (ATR, ṽ) = 2922, 2851, 1749, 1734, 1717, 1684, 1540, 1533, 1523, 1509, 1456, 1419, 1367, 1217, 1174, 1146, 1050, 989, 902, 839, 820, 755, 742, 698, 601, 483 cm–1.
DOI: 10.17632/mh8krrtwb5.1
title: Data for: The cause of the spring strengthening of the Antarctic polar vortex

description: Data of Fig. 1, 3, 4 for this study.
DOI: 10.25919/5d1596b9ea4e1
title: Parkes observations for project P976 semester 2018APRS_14

description: Spider pulsars - black widows (BW) and redbacks (RB) - reside in incredibly tight orbits with low-mass stellar companions. The close proximity of the two orbiting bodies leads to heavy irradiation of the companion by the pulsar wind, causing material to be driven from its surface. This excess material is not gravitationally bound to the star, and the extent to which it reaches can only be constrained by observing the duration of eclipses of the radio pulsar emission that it causes. Little information about these systems is set in stone: the physical processes behind the eclipses, the dimensions, densities and magnetic properties of the eclipse medium, mass loss rates and subsequent evolution of the companions, are all unknown. Previous radio studies of a handful of spider systems have highlighted the importance of high-time resolution and large frequency coverage in constraining their properties. Measurement of the flux density, dispersion measure, rotation measure and depolarisation of the pulsars, as a function of the orbits, directly probes the eclipse process and properties of the medium causing it. All of these measurables are frequency dependent, thus with ultra-wideband observations we will have access to an unparalleled insight into spider pulsar systems. We plan to observe three eclipses for each of three BWs and two RBs in order to constrain variability between the two classes, multiple systems within each class, and the eclipses in an individual system. In addition, such observations will demonstrate and help to optimise the capabilities of the new UWL receiver.
DOI: 10.14272/ceavsmbxrjidbr-kcdwtjqasa-n.1
title: C42H50Cl3NO18S
title: InChI=1S/C42H50Cl3NO18S/c1-7-19-56-39-33(46-41(52)42(43,44)45)36(34(58-25(4)48)30(61-39)21-55-20-28-11-9-8-10-12-28)64-40-38(60-27(6)50)37(59-26(5)49)35(63-32(51)18-15-24(3)47)31(62-40)22-57-65(53,54)29-16-13-23(2)14-17-29/h7-14,16-17,30-31,33-40H,1,15,18-22H2,2-6H3,(H,46,52)/t30?,31?,33?,34-,35-,36-,37+,38?,39-,40+/m1/s1

description: This dataset contains experimental data from a sample (InChI=1S/C42H50Cl3NO18S/c1-7-19-56-39-33(46-41(52)42(43,44)45)36(34(58-25(4)48)30(61-39)21-55-20-28-11-9-8-10-12-28)64-40-38(60-27(6)50)37(59-26(5)49)35(63-32(51)18-15-24(3)47)31(62-40)22-57-65(53,54)29-16-13-23(2)14-17-29/h7-14,16-17,30-31,33-40H,1,15,18-22H2,2-6H3,(H,46,52)/t30?,31?,33?,34-,35-,36-,37+,38?,39-,40+/m1/s1).
      The datasets from the following experiments are available:
      
      IR
DOI: 10.14272/ceavsmbxrjidbr-kcdwtjqasa-n/ir
title: IR (, InChI=1S/C42H50Cl3NO18S/c1-7-19-56-39-33(46-41(52)42(43,44)45)36(34(58-25(4)48)30(61-39)21-55-20-28-11-9-8-10-12-28)64-40-38(60-27(6)50)37(59-26(5)49)35(63-32(51)18-15-24(3)47)31(62-40)22-57-65(53,54)29-16-13-23(2)14-17-29/h7-14,16-17,30-31,33-40H,1,15,18-22H2,2-6H3,(H,46,52)/t30?,31?,33?,34-,35-,36-,37+,38?,39-,40+/m1/s1)

description: dataset for IR
      
      IR (ATR, ṽ) = 2919, 2871, 1752, 1717, 1596, 1540, 1524, 1509, 1456, 1419, 1404, 1364, 1319, 1286, 1217, 1190, 1176, 1147, 1125, 1094, 1054, 1031, 993, 941, 919, 836, 819, 756, 744, 698, 670, 654, 602, 564, 552, 516, 490 cm–1.
DOI: 10.14272/modsvoghzqaamj-ugylpvgzsa-n.1
title: C35H43Cl4NO15
title: InChI=1S/C35H43Cl4NO15/c1-6-14-48-32-26(40-34(46)35(37,38)39)29(28(49-19(3)42)24(53-32)17-47-16-22-10-8-7-9-11-22)55-33-31(51-21(5)44)30(50-20(4)43)27(23(15-36)52-33)54-25(45)13-12-18(2)41/h6-11,23-24,26-33H,1,12-17H2,2-5H3,(H,40,46)/t23?,24?,26?,27-,28-,29-,30+,31?,32-,33+/m1/s1

description: This dataset contains experimental data from a sample (InChI=1S/C35H43Cl4NO15/c1-6-14-48-32-26(40-34(46)35(37,38)39)29(28(49-19(3)42)24(53-32)17-47-16-22-10-8-7-9-11-22)55-33-31(51-21(5)44)30(50-20(4)43)27(23(15-36)52-33)54-25(45)13-12-18(2)41/h6-11,23-24,26-33H,1,12-17H2,2-5H3,(H,40,46)/t23?,24?,26?,27-,28-,29-,30+,31?,32-,33+/m1/s1).
      The datasets from the following experiments are available:
      
      IR
DOI: 10.14272/modsvoghzqaamj-ugylpvgzsa-n/ir
title: IR (, InChI=1S/C35H43Cl4NO15/c1-6-14-48-32-26(40-34(46)35(37,38)39)29(28(49-19(3)42)24(53-32)17-47-16-22-10-8-7-9-11-22)55-33-31(51-21(5)44)30(50-20(4)43)27(23(15-36)52-33)54-25(45)13-12-18(2)41/h6-11,23-24,26-33H,1,12-17H2,2-5H3,(H,40,46)/t23?,24?,26?,27-,28-,29-,30+,31?,32-,33+/m1/s1)

description: dataset for IR
      
      IR (ATR, ṽ) = 3373, 2928, 2880, 1747, 1730, 1718, 1653, 1540, 1526, 1456, 1424, 1373, 1326, 1283, 1214, 1204, 1173, 1147, 1113, 1067, 1038, 993, 965, 931, 899, 843, 817, 742, 721, 700, 674, 650, 613, 596, 531, 486, 402 cm–1.
DOI: 10.25919/5d159f9d027b7
title: Parkes observations for project P1011 semester 2019APRS_13

description: Pulsars with features in their radio spectra, such as curvature or breaks seem to be special cases among the known pulsar population, with only about 20 per cent exhibiting them. Unfortunately, reliable flux density measurements besides at 1.4 GHz are often unavailable, so that their spectral morphologies and features cannot be determined accurately. We propose to utilize the unique capabilities of the newly commissioned UWL receiver at the Parkes telescope, its extremely wide instantaneous frequency coverage from about 700 to 4000 MHz together with its high sensitivity, to determine the spectra of 26 radio pulsars. These have previously been identified to exhibit spectral features or show hints thereof. The new Parkes data are crucial to determine their spectral morphologies in that frequency range, to characterize their spectral features and to resolve these within the recorded bandwidth. Our aim is to understand the physical origin of the features, namely, whether these are perhaps intrinsic to the pulsar emission in these sources, are caused by absorption processes inside the pulsar's magnetosphere, or along the line of sight.
DOI: 10.17632/sjhzss266s.1
title: Data for: TAK-137, an AMPA receptor potentiator with little agonistic effect, produces antidepressant-like effect without causing psychotomimetic effects in rats

description: Raw data for each figure and numerical calculation result
DOI: 10.25919/5d15a66c413c2
title: Parkes observations for project P1007 semester 2019APRS_02

description: Recently, extreme plasma lensing of pulsar emission has been observed in two eclipsing binaries, PSR B1957+20 and PSR B1744-24A.  These lensing events are an extremely sensitive probe of pulsar emission, resolving physical scales of ~10 km at the pulsar, and can be used to measure the magnetization of the intrabinary material, and constrain outflow velocities and mass-loss rates of the binaries.  We propose to observe the 5 brightest eclipsing pulsars (B1718-19, J1723-2837, B1744-24A, B1957+20, J2051-0827), to search for the effects of plasma lensing, and to make use of the new Parkes Ultra Wide Band Low Frequency (UWL) receiver, which will allow us to resolve lensing events in frequency and time, which is crucial for constraining physical parameters.  This study will help determine how ubiquitous the effects of plasma lensing are in eclipsing binaries, put improved physical scales on the locations of pulsar emission, and help shed light on the nature of eclipses and evolutionary pathways of these systems.
DOI: 10.14469/hpc/5916
title: Bromoallene, Def2-SVPD 2AgOAc complex, Reactant acetic acid solvent (S) G=3633.227902 (syn) G=3633.247704

description: Gaussian Calculation
DOI: 10.25592/uhhfdm.136
title: Expression Profile Of Human Lymphatic Endothelial Cells Cultured On Stiff (25 Kpa) Or Soft (0.2 Kpa) Matrix Conditions In The Presence Or Absence Of Gata2

description: Global transcriptome analysis showed that human lymphatic endothelial cells (LECs) grown on a soft matrix exhibit increased GATA2 expression, concomitant with a GATA2-dependent upregulation of genes involved in cell migration and lymphangiogenesis, including the key lymphangiogenic growth factor receptor VEGFR3.<br> Affymetrix GeneChip analysis revealed regulation of 2771 transcripts above or below a 1.4-fold change (log2 fold change &gt;0.5 or &lt;-0.5) threshold on soft versus stiff matrices. Moreover, 406 (27%) of the 1485 transcripts that were increased and 207 (16 %) of the 1286 transcripts that were decreased on soft matrix were regulated in a GATA2 dependent manner. Overall design: In total 18 samples were analyzed (first biological replicate is uploaded here). To identify differentially expressed genes between the ctrl stiff and ctrl soft groups, a stepwise analysis with 6 biological replicates was performed. First, exon set ID’s with an average expression lower than 5 were considered as not significantly expressed and excluded from the analysis. A threshold of 40% increase (&gt;0.5 log2 fold change) or decrease (&lt;-0.5 log2 fold change) of gene expression on the soft matrix (vs. stiff matrix) was considered for further analysis. For all genes with 3 or more exon probe set ID’s regulated above the defined thresholds, the average log2 fold change of the regulated exon probe ID’s was calculated and used to generate the final list of genes regulated by matrix stiffness. To determine which of the genes are regulated in a GATA2 dependent manner, a stepwise analysis with 2 biological replicates ctrl siRNA soft vs GATA2 siRNA soft groups was performed. The previously identified exon probe ID’s for genes differentially regulated between the ctrl stiff and ctrl soft groups were extracted and their average log2 fold change was calculated for the new data set. A threshold of 40% increase (&gt;0.5 log2 fold change) or decrease (&lt;-0.5 log2 fold change) of gene expression in the absence of the GATA2 was used to generate the final list of genes.
DOI: 10.25592/uhhfdm.137
title: Expression Profile Of Human Lymphatic Endothelial Cells Cultured On Stiff (25 Kpa) Or Soft (0.2 Kpa) Matrix Conditions In The Presence Or Absence Of Gata2

description: Global transcriptome analysis showed that human lymphatic endothelial cells (LECs) grown on a soft matrix exhibit increased GATA2 expression, concomitant with a GATA2-dependent upregulation of genes involved in cell migration and lymphangiogenesis, including the key lymphangiogenic growth factor receptor VEGFR3.<br> Affymetrix GeneChip analysis revealed regulation of 2771 transcripts above or below a 1.4-fold change (log2 fold change &gt;0.5 or &lt;-0.5) threshold on soft versus stiff matrices. Moreover, 406 (27%) of the 1485 transcripts that were increased and 207 (16 %) of the 1286 transcripts that were decreased on soft matrix were regulated in a GATA2 dependent manner. Overall design: In total 18 samples were analyzed (first biological replicate is uploaded here). To identify differentially expressed genes between the ctrl stiff and ctrl soft groups, a stepwise analysis with 6 biological replicates was performed. First, exon set ID’s with an average expression lower than 5 were considered as not significantly expressed and excluded from the analysis. A threshold of 40% increase (&gt;0.5 log2 fold change) or decrease (&lt;-0.5 log2 fold change) of gene expression on the soft matrix (vs. stiff matrix) was considered for further analysis. For all genes with 3 or more exon probe set ID’s regulated above the defined thresholds, the average log2 fold change of the regulated exon probe ID’s was calculated and used to generate the final list of genes regulated by matrix stiffness. To determine which of the genes are regulated in a GATA2 dependent manner, a stepwise analysis with 2 biological replicates ctrl siRNA soft vs GATA2 siRNA soft groups was performed. The previously identified exon probe ID’s for genes differentially regulated between the ctrl stiff and ctrl soft groups were extracted and their average log2 fold change was calculated for the new data set. A threshold of 40% increase (&gt;0.5 log2 fold change) or decrease (&lt;-0.5 log2 fold change) of gene expression in the absence of the GATA2 was used to generate the final list of genes.
DOI: 10.18112/openneuro.ds002000.v1.0.0
title: reinstatement_fidelity