Noll, Angela

[["dc.bibliographiccitation.artnumber","239"],["dc.bibliographiccitation.issue","1"],["dc.bibliographiccitation.journal","BMC Genomics"],["dc.bibliographiccitation.volume","22"],["dc.contributor.author","Malukiewicz, Joanna"],["dc.contributor.author","Cartwright, Reed A."],["dc.contributor.author","Curi, Nelson H. A."],["dc.contributor.author","Dergam, Jorge A."],["dc.contributor.author","Igayara, Claudia S."],["dc.contributor.author","Moreira, Silvia B."],["dc.contributor.author","Molina, Camila V."],["dc.contributor.author","Nicola, Patricia A."],["dc.contributor.author","Noll, Angela"],["dc.contributor.author","Passamani, Marcello"],["dc.contributor.author","Pereira, Luiz C. M."],["dc.contributor.author","Pissinatti, Alcides"],["dc.contributor.author","Ruiz-Miranda, Carlos R."],["dc.contributor.author","Silva, Daniel L."],["dc.contributor.author","Stone, Anne C."],["dc.contributor.author","Zinner, Dietmar"],["dc.contributor.author","Roos, Christian"],["dc.date.accessioned","2021-06-01T09:42:14Z"],["dc.date.accessioned","2022-08-18T12:34:07Z"],["dc.date.available","2021-06-01T09:42:14Z"],["dc.date.available","2022-08-18T12:34:07Z"],["dc.date.issued","2021-04-06"],["dc.date.updated","2022-07-29T12:07:00Z"],["dc.description.abstract","Abstract\r\n \r\n Background\r\n Callithrix marmosets are a relatively young primate radiation, whose phylogeny is not yet fully resolved. These primates are naturally para- and allopatric, but three species with highly invasive potential have been introduced into the southeastern Brazilian Atlantic Forest by the pet trade. There, these species hybridize with each other and endangered, native congeners. We aimed here to reconstruct a robust Callithrix phylogeny and divergence time estimates, and identify the biogeographic origins of autochthonous and allochthonous Callithrix mitogenome lineages. We sequenced 49 mitogenomes from four species (C. aurita, C. geoffroyi, C. jacchus, C. penicillata) and anthropogenic hybrids (C. aurita x Callithrix sp., C. penicillata x C. jacchus, Callithrix sp. x Callithrix sp., C. penicillata x C. geoffroyi) via Sanger and whole genome sequencing. We combined these data with previously published Callithrix mitogenomes to analyze five Callithrix species in total.\r\n \r\n \r\n Results\r\n We report the complete sequence and organization of the C. aurita mitogenome. Phylogenetic analyses showed that C. aurita was the first to diverge within Callithrix 3.54 million years ago (Ma), while C. jacchus and C. penicillata lineages diverged most recently 0.5 Ma as sister clades. MtDNA clades of C. aurita, C. geoffroyi, and C. penicillata show intraspecific geographic structure, but C. penicillata clades appear polyphyletic. Hybrids, which were identified by phenotype, possessed mainly C. penicillata or C. jacchus mtDNA haplotypes. The biogeographic origins of mtDNA haplotypes from hybrid and allochthonous Callithrix were broadly distributed across natural Callithrix ranges. Our phylogenetic results also evidence introgression of C. jacchus mtDNA into C. aurita.\r\n \r\n \r\n Conclusion\r\n Our robust Callithrix mitogenome phylogeny shows C. aurita lineages as basal and C. jacchus lineages among the most recent within Callithrix. We provide the first evidence that parental mtDNA lineages of anthropogenic hybrid and allochthonous marmosets are broadly distributed inside and outside of the Atlantic Forest. We also show evidence of cryptic hybridization between allochthonous Callithrix and autochthonous C. aurita. Our results encouragingly show that further development of genomic resources will allow to more clearly elucidate Callithrix evolutionary relationships and understand the dynamics of Callithrix anthropogenic introductions into the Brazilian Atlantic Forest."],["dc.identifier.citation","BMC Genomics. 2021 Apr 06;22(1):239"],["dc.identifier.doi","10.1186/s12864-021-07533-1"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/17751"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/85188"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/112926"],["dc.language.iso","en"],["dc.notes.intern","DOI-Import GROB-425"],["dc.notes.intern","Merged from goescholar"],["dc.publisher","BioMed Central"],["dc.relation.eissn","1471-2164"],["dc.rights","CC BY 4.0"],["dc.rights.holder","The Author(s)"],["dc.rights.uri","https://creativecommons.org/licenses/by/4.0"],["dc.subject","mtDNA"],["dc.subject","Marmoset"],["dc.subject","Divergence"],["dc.subject","Atlantic forest"],["dc.subject","Brazil"],["dc.subject","Callitrichidae"],["dc.subject","Primate"],["dc.title","Mitogenomic phylogeny of Callithrix with special focus on human transferred taxa"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","885"],["dc.bibliographiccitation.issue","3"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.lastpage","906"],["dc.bibliographiccitation.volume","418"],["dc.contributor.author","Noll, S."],["dc.contributor.author","Mehlert, D."],["dc.contributor.author","Appenzeller, I."],["dc.contributor.author","Bender, R."],["dc.contributor.author","Bohm, A."],["dc.contributor.author","Gabasch, A."],["dc.contributor.author","Heidt, J."],["dc.contributor.author","Hopp, U."],["dc.contributor.author","Jager, Kitty J."],["dc.contributor.author","Seitz, Sebastian"],["dc.contributor.author","Stahl, O."],["dc.contributor.author","Tapken, C."],["dc.contributor.author","Ziegler, Bodo L."],["dc.date.accessioned","2018-11-07T10:49:07Z"],["dc.date.available","2018-11-07T10:49:07Z"],["dc.date.issued","2004"],["dc.description.abstract","We present a catalogue and atlas of low-resolution spectra of a well defined sample of 341 objects in the FORS Deep Field. All spectra were obtained with the FORS instruments at the ESO VLT with essentially the same spectroscopic set-up. The observed extragalactic objects cover the redshift range 0.1 to 5.0. 98 objects are starburst galaxies and QSOs at z > 2. Using this data set we investigated the evolution of the characteristic spectral properties of bright starburst galaxies and their mutual relations as a function of redshift. Significant evolutionary effects were found for redshifts 2 < z < 4. Most conspicuous are the increase of the average C IV absorption strength, of the dust reddening, and of the intrinsic UV luminosity, and the decrease of the average Lyalpha emission strength with decreasing redshift. In part the observed evolutionary effects can be attributed to an increase of the metallicity of the galaxies with cosmic age. Moreover, the increase of the total star-formation rates and the stronger obscuration of the starburst cores by dusty gas clouds suggest the occurrence of more massive starbursts at later cosmic epochs."],["dc.identifier.doi","10.1051/0004-6361:20034434"],["dc.identifier.fs","21437"],["dc.identifier.isi","000221646300012"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/9819"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/48355"],["dc.notes.intern","Merged from goescholar"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","E D P Sciences"],["dc.relation.issn","0004-6361"],["dc.relation.orgunit","Fakultät für Physik"],["dc.title","The FORS Deep Field spectroscopic survey"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","471"],["dc.bibliographiccitation.issue","181"],["dc.bibliographiccitation.journal","Zoological Journal of the Linnean Society"],["dc.bibliographiccitation.lastpage","483"],["dc.contributor.author","Dolotovskaya, Sofya"],["dc.contributor.author","Torroba Bordallo, Juan"],["dc.contributor.author","Haus, Tanja"],["dc.contributor.author","Noll, Angela"],["dc.contributor.author","Hofreiter, Michael"],["dc.contributor.author","Zinner, Dietmar"],["dc.contributor.author","Roos, Christian"],["dc.date.accessioned","2019-12-09T12:27:38Z"],["dc.date.accessioned","2021-10-27T13:13:12Z"],["dc.date.available","2019-12-09T12:27:38Z"],["dc.date.available","2021-10-27T13:13:12Z"],["dc.date.issued","2017"],["dc.description.abstract","Complete mitochondrial (mtDNA) genomes have proved to be useful in reconstructing primate phylogenies with higher resolution and confidence compared to reconstructions based on partial mtDNA sequences. Here, we analyse complete mtDNA genomes of African green monkeys (genus Chlorocebus), a widely distributed primate genus in Africa representing an interesting phylogeographical model for the evolution of savannah species. Previous studies on partial mtDNA sequences revealed nine major clades, suggesting several cases of para- and polyphyly among Chlorocebus species. However, in these studies, phylogenetic relationships among several clades were not resolved, and divergence times were not estimated. We analysed complete mtDNA genomes for ten Chlorocebus samples representing major mtDNA clades to find stronger statistical support in the phylogenetic reconstruction than in the previous studies and to estimate divergence times. Our results confirmed para- and polyphyletic relationships of most Chlorocebus species, while the support for the phylogenetic relationships between the mtDNA clades increased compared to the previous studies. Our results indicate an initial west–east division in the northern part of the Chlorocebus range with subsequent divergence into north-eastern and southern clades. This phylogeographic scenario contrasts with that for another widespread African savannah primate genus, the baboons (Papio), for which a dispersal from southern Africa into East and West Africa was suggested."],["dc.identifier.doi","10.1093/zoolinnean/zlx001"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/16877"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/91760"],["dc.language.iso","en"],["dc.notes.intern","Migrated from goescholar"],["dc.relation.eissn","1096-3642"],["dc.relation.issn","1096-3642"],["dc.relation.issn","0024-4082"],["dc.relation.orgunit","Deutsches Primatenzentrum"],["dc.rights","CC BY 4.0"],["dc.rights.uri","https://creativecommons.org/licenses/by/4.0"],["dc.subject.ddc","599"],["dc.title","Comparing mitogenomic timetrees for two African savannah primate genera (Chlorocebus and Papio)"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","809"],["dc.bibliographiccitation.issue","3"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.lastpage","819"],["dc.bibliographiccitation.volume","393"],["dc.contributor.author","Mehlert, D."],["dc.contributor.author","Noll, S."],["dc.contributor.author","Appenzeller, I."],["dc.contributor.author","Saglia, R. P."],["dc.contributor.author","Bender, R."],["dc.contributor.author","Bohm, A."],["dc.contributor.author","Drory, N."],["dc.contributor.author","Fricke, K. J."],["dc.contributor.author","Gabasch, A."],["dc.contributor.author","Heidt, J."],["dc.contributor.author","Hopp, U."],["dc.contributor.author","Jager, Kitty J."],["dc.contributor.author","Mollenhoff, C."],["dc.contributor.author","Seitz, Sebastian"],["dc.contributor.author","Stahl, O."],["dc.contributor.author","Ziegler, Bodo L."],["dc.date.accessioned","2018-11-07T09:57:32Z"],["dc.date.available","2018-11-07T09:57:32Z"],["dc.date.issued","2002"],["dc.description.abstract","Using a sample of 57 VLT FORS spectra in the redshift range 1.37 < z < 3.40 (selected mainly from the FORS Deep Field survey) and a comparison sample with 36 IUE spectra of local (z approximate to 0) starburst galaxies we derive C and Si equivalent width values and estimate metallicities of starburst galaxies as a function of redshift. Assuming that a calibration of the C equivalent widths in terms of the metallicity based on the local sample of starburst galaxies is applicable to high-z objects, we find a significant increase of the average metallicities from about 0.16 Z(.) at the cosmic epoch corresponding to z approximate to 3.2 to about 0.42 Z(.) at z approximate to 2.3. A significant further increase in metallicity during later epochs cannot be detected in our data. Compared to the local starburst galaxies our high-redshift objects tend to be overluminous for a fixed metallicity. Our observational results are in good agreement with published observational data by other authors and with theoretical predictions of the cosmic chemical evolution."],["dc.identifier.doi","10.1051/0004-6361:20021052"],["dc.identifier.fs","19116"],["dc.identifier.isi","000178313000019"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/9731"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/37177"],["dc.notes.intern","Merged from goescholar"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Edp Sciences S A"],["dc.relation.issn","1432-0746"],["dc.relation.orgunit","Fakultät für Physik"],["dc.title","Evidence for chemical evolution in the spectra of high redshift galaxies"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","12997"],["dc.bibliographiccitation.journal","Nature Communications"],["dc.bibliographiccitation.volume","7"],["dc.contributor.author","Schmitz, Jürgen"],["dc.contributor.author","Noll, Angela"],["dc.contributor.author","Raabe, Carsten A."],["dc.contributor.author","Churakov, Gennady"],["dc.contributor.author","Voss, Reinhard"],["dc.contributor.author","Kiefmann, Martin"],["dc.contributor.author","Rozhdestvensky, Timofey"],["dc.contributor.author","Brosius, Jürgen"],["dc.contributor.author","Baertsch, Robert"],["dc.contributor.author","Clawson, Hiram"],["dc.contributor.author","Roos, Christian"],["dc.contributor.author","Zimin, Aleksey"],["dc.contributor.author","Minx, Patrick"],["dc.contributor.author","Montague, Michael J."],["dc.contributor.author","Wilson, Richard K."],["dc.contributor.author","Warren, Wesley C."],["dc.date.accessioned","2019-07-09T11:42:54Z"],["dc.date.available","2019-07-09T11:42:54Z"],["dc.date.issued","2016"],["dc.description.abstract","Tarsiers are phylogenetically located between the most basal strepsirrhines and the most derived anthropoid primates. While they share morphological features with both groups, they also possess uncommon primate characteristics, rendering their evolutionary history somewhat obscure. To investigate the molecular basis of such attributes, we present here a new genome assembly of the Philippine tarsier (Tarsius syrichta), and provide extended analyses of the genome and detailed history of transposable element insertion events. We describe the silencing of Alu monomers on the lineage leading to anthropoids, and recognize an unexpected abundance of long terminal repeat-derived and LINE1-mobilized transposed elements (Tarsius interspersed elements; TINEs). For the first time in mammals, we identify a complete mitochondrial genome insertion within the nuclear genome, then reveal tarsier-specific, positive gene selection and posit population size changes over time. The genomic resources and analyses presented here will aid efforts to more fully understand the ancient characteristics of primate genomes. DOI: 10.1038/ncomms12997 OPEN 1"],["dc.identifier.doi","10.1038/ncomms12997"],["dc.identifier.pmid","27708261"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/13959"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/58780"],["dc.language.iso","en"],["dc.notes.intern","Merged from goescholar"],["dc.relation.issn","2041-1723"],["dc.rights","CC BY 4.0"],["dc.rights.uri","https://creativecommons.org/licenses/by/4.0"],["dc.title","Genome sequence of the basal haplorrhine primate Tarsius syrichta reveals unusual insertions"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","49"],["dc.bibliographiccitation.issue","1"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.lastpage","61"],["dc.bibliographiccitation.volume","398"],["dc.contributor.author","Heidt, J."],["dc.contributor.author","Appenzeller, I."],["dc.contributor.author","Gabasch, A."],["dc.contributor.author","Jager, Kitty J."],["dc.contributor.author","Seitz, Sebastian"],["dc.contributor.author","Bender, R."],["dc.contributor.author","Bohm, A."],["dc.contributor.author","Snigula, J."],["dc.contributor.author","Fricke, K. J."],["dc.contributor.author","Hopp, U."],["dc.contributor.author","Kummel, M."],["dc.contributor.author","Mollenhoff, C."],["dc.contributor.author","Szeifert, T."],["dc.contributor.author","Ziegler, Bodo L."],["dc.contributor.author","Drory, N."],["dc.contributor.author","Mehlert, D."],["dc.contributor.author","Moorwood, A."],["dc.contributor.author","Nicklas, H."],["dc.contributor.author","Noll, S."],["dc.contributor.author","Saglia, R. P."],["dc.contributor.author","Seifert, W."],["dc.contributor.author","Stahl, O."],["dc.contributor.author","Sutorius, E."],["dc.contributor.author","Wagner, S. J."],["dc.date.accessioned","2018-11-07T10:42:00Z"],["dc.date.available","2018-11-07T10:42:00Z"],["dc.date.issued","2003"],["dc.description.abstract","The FORS Deep Field project is a multi-colour, multi-object spectroscopic investigation of a similar to7' x 7' region near the south galactic pole based mostly on observations carried out with the FORS instruments attached to the VLT telescopes. It includes the QSO Q 0103-260 (z = 3.36). The goal of this study is to improve our understanding of the formation and evolution of galaxies in the young Universe. In this paper the field selection, the photometric observations, and the data reduction are described. The source detection and photometry of objects in the FORS Deep Field is discussed in detail. A combined B and 1 selected UBgRIJKs photometric catalog of 8753 objects in the FDF is presented and its properties are briefly discussed. The formal 50% completeness limits for point sources, derived from the co-added images, are 25.64, 27.69, 26.86, 26.68, 26.37, 23.60 and 21.57 in U, B, g, R, I, J and Ks (Vega-system), respectively. A comparison of the number counts in the FORS Deep Field to those derived in other deep field surveys shows very good agreement."],["dc.identifier.doi","10.1051/0004-6361:20021620"],["dc.identifier.isi","000180395700008"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/9798"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/46680"],["dc.notes.intern","Merged from goescholar"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","E D P Sciences"],["dc.relation.issn","0004-6361"],["dc.relation.orgunit","Fakultät für Physik"],["dc.title","The FORS deep field: Field selection, photometric observations and photometric catalog"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","41"],["dc.bibliographiccitation.issue","1"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.lastpage","58"],["dc.bibliographiccitation.volume","421"],["dc.contributor.author","Gabasch, A."],["dc.contributor.author","Bender, R."],["dc.contributor.author","Seitz, Sebastian"],["dc.contributor.author","Hopp, U."],["dc.contributor.author","Saglia, R. P."],["dc.contributor.author","Feulner, G."],["dc.contributor.author","Snigula, J."],["dc.contributor.author","Drory, N."],["dc.contributor.author","Appenzeller, I."],["dc.contributor.author","Heidt, J."],["dc.contributor.author","Mehlert, D."],["dc.contributor.author","Noll, S."],["dc.contributor.author","Bohm, A."],["dc.contributor.author","Jager, Kitty J."],["dc.contributor.author","Ziegler, Bodo L."],["dc.contributor.author","Fricke, K. J."],["dc.date.accessioned","2018-11-07T10:47:28Z"],["dc.date.available","2018-11-07T10:47:28Z"],["dc.date.issued","2004"],["dc.description.abstract","We use the very deep and homogeneous I-band selected dataset of the FORS Deep Field (FDF) to trace the evolution of the luminosity function over the redshift range 0.5 < z < 5.0. We show that the FDF I-band selection down to I-AB = 26.8 misses of the order of 10% of the galaxies that would be detected in a K-band selected survey with magnitude limit K-AB = 26.3 (like FIRES). Photometric redshifts for 5558 galaxies are estimated based on the photometry in 9 filters (U, B, Gunn g, R, 1, SDSS z, J, K and a special filter centered at 834 nm). A comparison with 362 spectroscopic redshifts shows that the achieved accuracy of the photometric redshifts is Deltaz/(z(spec) + 1) less than or equal to 0.03 with only similar to1% outliers. This allows us to derive luminosity functions with a reliability similar to spectroscopic surveys. In addition, the luminosity functions can be traced to objects of lower luminosity which generally are not accessible to spectroscopy. We investigate the evolution of the luminosity functions evaluated in the restframe UV (1500 Angstrom and 2800 Angstrom), u', B, and g' bands. Comparison with results from the literature shows the reliability of the derived luminosity functions. Out to redshifts of z similar to 2.5 the data are consistent with a slope of the luminosity function approximately constant with redshift, at a value of -1.07 +/- 0.04 in the UV (1500 Angstrom, 2800 Angstrom) as well as u', and -1.25 +/- 0.03 in the blue (g', B). We do not see evidence for a very steep slope (alpha less than or equal to -1.6) in the UV at similar to 3.0 and similar to 4.0 favoured by other authors. There may be a tendency for the faint-end slope to become shallower with increasing redshift but the effect is marginal. We find a brightening of M and a decrease of phi with redshift for all analyzed wavelengths. The effect is systematic and much stronger than what can be expected to be caused by cosmic variance seen in the FDF. The evolution of M and phi from z = 0 to z = 5 is well described by the simple approximations M (z) = M-0( ) + a ln (1 + z) and phi (z) = phi(0)( ) (1 + z)(b) for M and phi . The evolution is very pronounced at shorter wavelengths (a = -2.19, and b = -1.76 for 1500 Angstrom rest wavelength) and decreases systematically with increasing wavelength, but is also clearly visible at the longest wavelength investigated here (a = -1.08, and b = -1.29 for g'). Finally we show a comparison with semi-analytical galaxy formation models."],["dc.identifier.doi","10.1051/0004-6361:20035909"],["dc.identifier.fs","38385"],["dc.identifier.isi","000222847800011"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/9825"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/47971"],["dc.notes.intern","Merged from goescholar"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Edp Sciences S A"],["dc.relation.issn","1432-0746"],["dc.relation.orgunit","Fakultät für Physik"],["dc.title","The evolution of the luminosity functions in the FORS Deep Field from low to high redshift - I. The blue bands"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","97"],["dc.bibliographiccitation.issue","1"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.lastpage","114"],["dc.bibliographiccitation.volume","420"],["dc.contributor.author","Bohm, A."],["dc.contributor.author","Ziegler, Bodo L."],["dc.contributor.author","Saglia, R. P."],["dc.contributor.author","Bender, R."],["dc.contributor.author","Fricke, K. J."],["dc.contributor.author","Gabasch, A."],["dc.contributor.author","Heidt, J."],["dc.contributor.author","Mehlert, D."],["dc.contributor.author","Noll, S."],["dc.contributor.author","Seitz, Sebastian"],["dc.date.accessioned","2018-11-07T10:48:16Z"],["dc.date.available","2018-11-07T10:48:16Z"],["dc.date.issued","2004"],["dc.description.abstract","Using the Very Large Telescope in Multi Object Spectroscopy mode, we have observed a sample of 113 field spiral galaxies in the FORS Deep Field (FDF) with redshifts in the range 0.1

[["dc.bibliographiccitation.artnumber","15944"],["dc.bibliographiccitation.issue","1"],["dc.bibliographiccitation.journal","Scientific Reports"],["dc.bibliographiccitation.volume","8"],["dc.contributor.author","Gutleb, Daria Raffaella"],["dc.contributor.author","Ostner, Julia"],["dc.contributor.author","Schülke, Oliver"],["dc.contributor.author","Wajjwalku, Worawidh"],["dc.contributor.author","Sukmak, Manakorn"],["dc.contributor.author","Roos, Christian"],["dc.contributor.author","Noll, Angela"],["dc.date.accessioned","2019-07-09T11:51:07Z"],["dc.date.available","2019-07-09T11:51:07Z"],["dc.date.issued","2018"],["dc.description.abstract","We designed a genotyping panel for the investigation of the genetic underpinnings of inter-individual differences in aggression and the physiological stress response. The panel builds on single nucleotide polymorphisms (SNPs) in genes involved in the three subsystems of the hypothalamic-pituitary-adrenal (HPA)-axis: the catecholamine, serotonin and corticoid metabolism. To promote the pipeline for use with wild animal populations, we used non-invasively collected faecal samples from a wild population of Assamese macaques (Macaca assamensis). We targeted loci of 46 previously reported SNPs in 21 candidate genes coding for elements of the HPA-axis and amplified and sequenced them using next-generation Illumina sequencing technology. We compared multiple bioinformatics pipelines for variant calling and variant effect prediction. Based on this strategy and the application of different quality thresholds, we identified up to 159 SNPs with different types of predicted functional effects among our natural study population. This study provides a massively parallel sequencing panel that will facilitate integrating large-scale SNP data into behavioural and physiological studies. Such a multi-faceted approach will promote understanding of flexibility and constraints of animal behaviour and hormone physiology."],["dc.identifier.doi","10.1038/s41598-018-34223-y"],["dc.identifier.pmid","30374157"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/16052"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/59879"],["dc.language.iso","en"],["dc.notes.intern","Merged from goescholar"],["dc.rights","CC BY 4.0"],["dc.rights.uri","https://creativecommons.org/licenses/by/4.0"],["dc.subject.ddc","570"],["dc.title","Non-invasive genotyping with a massively parallel sequencing panel for the detection of SNPs in HPA-axis genes"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]