TY - JOUR A1 - Taal, H. Rob A1 - St Pourcain, Beate A1 - Thiering, Elisabeth A1 - Das, Shikta A1 - Mook-Kanamori, Dennis O. A1 - Warrington, Nicole M. A1 - Kaakinen, Marika A1 - Kreiner-Moller, Eskil A1 - Bradfield, Jonathan P. A1 - Freathy, Rachel M. A1 - Geller, Frank A1 - Guxens, Monica A1 - Cousminer, Diana L. A1 - Kerkhof, Marjan A1 - Timpson, Nicholas J. A1 - Ikram, M. Arfan A1 - Beilin, Lawrence J. A1 - Bonnelykke, Klaus A1 - Buxton, Jessica L. A1 - Charoen, Pimphen A1 - Chawes, Bo Lund Krogsgaard A1 - Eriksson, Johan A1 - Evans, David M. A1 - Hofman, Albert A1 - Kemp, John P. A1 - Kim, Cecilia E. A1 - Klopp, Norman A1 - Lahti, Jari A1 - Lye, Stephen J. A1 - McMahon, George A1 - Mentch, Frank D. A1 - Mueller-Nurasyid, Martina A1 - O'Reilly, Paul F. A1 - Prokopenko, Inga A1 - Rivadeneira, Fernando A1 - Steegers, Eric A. P. A1 - Sunyer, Jordi A1 - Tiesler, Carla A1 - Yaghootkar, Hanieh A1 - Breteler, Monique M. B. A1 - Debette, Stephanie A1 - Fornage, Myriam A1 - Gudnason, Vilmundur A1 - Launer, Lenore J. A1 - van der Lugt, Aad A1 - Mosley, Thomas H. A1 - Seshadri, Sudha A1 - Smith, Albert V. A1 - Vernooij, Meike W. A1 - Blakemore, Alexandra I. F. A1 - Chiavacci, Rosetta M. A1 - Feenstra, Bjarke A1 - Fernandez-Banet, Julio A1 - Grant, Struan F. A. A1 - Hartikainen, Anna-Liisa A1 - van der Heijden, Albert J. A1 - Iniguez, Carmen A1 - Lathrop, Mark A1 - McArdle, Wendy L. A1 - Molgaard, Anne A1 - Newnham, John P. A1 - Palmer, Lyle J. A1 - Palotie, Aarno A1 - Pouta, Annneli A1 - Ring, Susan M. A1 - Sovio, Ulla A1 - Standl, Marie A1 - Uitterlinden, Andre G. A1 - Wichmann, H-Erich A1 - Vissing, Nadja Hawwa A1 - DeCarli, Charles A1 - van Duijn, Cornelia M. A1 - McCarthy, Mark I. A1 - Koppelman, Gerard H. A1 - Estivill, Xavier A1 - Hattersley, Andrew T. A1 - Melbye, Mads A1 - Bisgaard, Hans A1 - Pennell, Craig E. A1 - Widen, Elisabeth A1 - Hakonarson, Hakon A1 - Smith, George Davey A1 - Heinrich, Joachim A1 - Jarvelin, Marjo-Riitta A1 - Jaddoe, Vincent W. V. A1 - Adair, Linda S. A1 - Ang, Wei A1 - Atalay, Mustafa A1 - van Beijsterveldt, Toos A1 - Bergen, Nienke A1 - Benke, Kelly A1 - Berry, Diane J. A1 - Bradfield, Jonathan P. A1 - Charoen, Pimphen A1 - Coin, Lachlan A1 - Cousminer, Diana L. A1 - Das, Shikta A1 - Davis, Oliver S. P. A1 - Elliott, Paul A1 - Evans, David M. A1 - Feenstra, Bjarke A1 - Flexeder, Claudia A1 - Frayling, Tim A1 - Freathy, Rachel M. A1 - Gaillard, Romy A1 - Geller, Frank A1 - Groen-Blokhuis, Maria A1 - Goh, Liang-Kee A1 - Guxens, Monica A1 - Haworth, Claire M. A. A1 - Hadley, Dexter A1 - Hebebrand, Johannes A1 - Hinney, Anke A1 - Hirschhorn, Joel N. A1 - Holloway, John W. A1 - Holst, Claus A1 - Hottenga, Jouke Jan A1 - Horikoshi, Momoko A1 - Huikari, Ville A1 - Hypponen, Elina A1 - Iniguez, Carmen A1 - Kaakinen, Marika A1 - Kilpelainen, Tuomas O. A1 - Kirin, Mirna A1 - Kowgier, Matthew A1 - Lakka, Hanna-Maaria A1 - Lange, Leslie A. A1 - Lawlor, Debbie A. A1 - Lehtimaki, Terho A1 - Lewin, Alex A1 - Lindgren, Cecilia A1 - Lindi, Virpi A1 - Maggi, Reedik A1 - Marsh, Julie A1 - Middeldorp, Christel A1 - Millwood, Iona A1 - Mook-Kanamori, Dennis O. A1 - Murray, Jeffrey C. A1 - Nivard, Michel A1 - Nohr, Ellen Aagaard A1 - Ntalla, Ioanna A1 - Oken, Emily A1 - O'Reilly, Paul F. A1 - Palmer, Lyle J. A1 - Panoutsopoulou, Kalliope A1 - Pararajasingham, Jennifer A1 - Prokopenko, Inga A1 - Rodriguez, Alina A1 - Salem, Rany M. A1 - Sebert, Sylvain A1 - Siitonen, Niina A1 - Sovio, Ulla A1 - St Pourcain, Beate A1 - Strachan, David P. A1 - Sunyer, Jordi A1 - Taal, H. Rob A1 - Teo, Yik-Ying A1 - Thiering, Elisabeth A1 - Tiesler, Carla A1 - Uitterlinden, Andre G. A1 - Valcarcel, Beatriz A1 - Warrington, Nicole M. A1 - White, Scott A1 - Willemsen, Gonneke A1 - Yaghootkar, Hanieh A1 - Zeggini, Eleftheria A1 - Boomsma, Dorret I. A1 - Cooper, Cyrus A1 - Estivill, Xavier A1 - Gillman, Matthew A1 - Grant, Struan F. A. A1 - Hakonarson, Hakon A1 - Hattersley, Andrew T. A1 - Heinrich, Joachim A1 - Hocher, Berthold A1 - Jaddoe, Vincent W. V. A1 - Jarvelin, Marjo-Riitta A1 - Lakka, Timo A. A1 - McCarthy, Mark I. A1 - Melbye, Mads A1 - Mohlke, Karen L. A1 - Dedoussis, George V. A1 - Ong, Ken K. A1 - Pearson, Ewan R. A1 - Pennell, Craig E. A1 - Price, Thomas S. A1 - Power, Chris A1 - Raitakari, Olli T. A1 - Saw, Seang-Mei A1 - Scherag, Andre A1 - Simell, Olli A1 - Sorensen, Thorkild I. A. A1 - Timpson, Nicholas J. A1 - Widen, Elisabeth A1 - Wilson, James F. A1 - Ang, Wei A1 - van Beijsterveldt, Toos A1 - Bergen, Nienke A1 - Benke, Kelly A1 - Berry, Diane J. A1 - Bradfield, Jonathan P. A1 - Charoen, Pimphen A1 - Coin, Lachlan A1 - Cousminer, Diana L. A1 - Das, Shikta A1 - Elliott, Paul A1 - Evans, David M. A1 - Frayling, Tim A1 - Freathy, Rachel M. A1 - Gaillard, Romy A1 - Groen-Blokhuis, Maria A1 - Guxens, Monica A1 - Hadley, Dexter A1 - Hottenga, Jouke Jan A1 - Huikari, Ville A1 - Hypponen, Elina A1 - Kaakinen, Marika A1 - Kowgier, Matthew A1 - Lawlor, Debbie A. A1 - Lewin, Alex A1 - Lindgren, Cecilia A1 - Marsh, Julie A1 - Middeldorp, Christel A1 - Millwood, Iona A1 - Mook-Kanamori, Dennis O. A1 - Nivard, Michel A1 - O'Reilly, Paul F. A1 - Palmer, Lyle J. A1 - Prokopenko, Inga A1 - Rodriguez, Alina A1 - Sebert, Sylvain A1 - Sovio, Ulla A1 - St Pourcain, Beate A1 - Standl, Marie A1 - Strachan, David P. A1 - Sunyer, Jordi A1 - Taal, H. Rob A1 - Thiering, Elisabeth A1 - Tiesler, Carla A1 - Uitterlinden, Andre G. A1 - Valcarcel, Beatriz A1 - Warrington, Nicole M. A1 - White, Scott A1 - Willemsen, Gonneke A1 - Yaghootkar, Hanieh A1 - Boomsma, Dorret I. A1 - Estivill, Xavier A1 - Grant, Struan F. A. A1 - Hakonarson, Hakon A1 - Hattersley, Andrew T. A1 - Heinrich, Joachim A1 - Jaddoe, Vincent W. V. A1 - Jarvelin, Marjo-Riitta A1 - McCarthy, Mark I. A1 - Pennell, Craig E. A1 - Power, Chris A1 - Timpson, Nicholas J. A1 - Widen, Elisabeth A1 - Ikram, M. Arfan A1 - Fornage, Myriam A1 - Smith, Albert V. A1 - Seshadri, Sudha A1 - Schmidt, Reinhold A1 - Debette, Stephanie A1 - Vrooman, Henri A. A1 - Sigurdsson, Sigurdur A1 - Ropele, Stefan A1 - Coker, Laura H. A1 - Longstreth, W. T. A1 - Niessen, Wiro J. A1 - DeStefano, Anita L. A1 - Beiser, Alexa A1 - Zijdenbos, Alex P. A1 - Struchalin, Maksim A1 - Jack, Clifford R. A1 - Nalls, Mike A. A1 - Au, Rhoda A1 - Hofman, Albert A1 - Gudnason, Haukur A1 - van der Lugt, Aad A1 - Harris, Tamara B. A1 - Meeks, William M. A1 - Vernooij, Meike W. A1 - van Buchem, Mark A. A1 - Catellier, Diane A1 - Gudnason, Vilmundur A1 - Windham, B. Gwen A1 - Wolf, Philip A. A1 - van Duijn, Cornelia M. A1 - Mosley, Thomas H. A1 - Schmidt, Helena A1 - Launer, Lenore J. A1 - Breteler, Monique M. B. A1 - DeCarli, Charles T1 - Common variants at 12q15 and 12q24 are associated with infant head circumference JF - Nature genetics N2 - To identify genetic variants associated with head circumference in infancy, we performed a meta-analysis of seven genome-wide association studies (GWAS) (N = 10,768 individuals of European ancestry enrolled in pregnancy and/or birth cohorts) and followed up three lead signals in six replication studies (combined N = 19,089). rs7980687 on chromosome 12q24 (P = 8.1 x 10(-9)) and rs1042725 on chromosome 12q15 (P = 2.8 x 10(-10)) were robustly associated with head circumference in infancy. Although these loci have previously been associated with adult height(1), their effects on infant head circumference were largely independent of height (P = 3.8 x 10(-7) for rs7980687 and P = 1.3 x 10(-7) for rs1042725 after adjustment for infant height). A third signal, rs11655470 on chromosome 17q21, showed suggestive evidence of association with head circumference (P = 3.9 x 10(-6)). SNPs correlated to the 17q21 signal have shown genome-wide association with adult intracranial volume(2), Parkinson's disease and other neurodegenerative diseases(3-5), indicating that a common genetic variant in this region might link early brain growth with neurological disease in later life. Y1 - 2012 U6 - https://doi.org/10.1038/ng.2238 SN - 1061-4036 VL - 44 IS - 5 SP - 532 EP - + PB - Nature Publ. Group CY - New York ER - TY - JOUR A1 - Read, Betsy A. A1 - Kegel, Jessica A1 - Klute, Mary J. A1 - Kuo, Alan A1 - Lefebvre, Stephane C. A1 - Maumus, Florian A1 - Mayer, Christoph A1 - Miller, John A1 - Monier, Adam A1 - Salamov, Asaf A1 - Young, Jeremy A1 - Aguilar, Maria A1 - Claverie, Jean-Michel A1 - Frickenhaus, Stephan A1 - Gonzalez, Karina A1 - Herman, Emily K. A1 - Lin, Yao-Cheng A1 - Napier, Johnathan A1 - Ogata, Hiroyuki A1 - Sarno, Analissa F. A1 - Shmutz, Jeremy A1 - Schroeder, Declan A1 - de Vargas, Colomban A1 - Verret, Frederic A1 - von Dassow, Peter A1 - Valentin, Klaus A1 - Van de Peer, Yves A1 - Wheeler, Glen A1 - Dacks, Joel B. A1 - Delwiche, Charles F. A1 - Dyhrman, Sonya T. A1 - Glöckner, Gernot A1 - John, Uwe A1 - Richards, Thomas A1 - Worden, Alexandra Z. A1 - Zhang, Xiaoyu A1 - Grigoriev, Igor V. A1 - Allen, Andrew E. A1 - Bidle, Kay A1 - Borodovsky, M. A1 - Bowler, C. A1 - Brownlee, Colin A1 - Cock, J. Mark A1 - Elias, Marek A1 - Gladyshev, Vadim N. A1 - Groth, Marco A1 - Guda, Chittibabu A1 - Hadaegh, Ahmad A1 - Iglesias-Rodriguez, Maria Debora A1 - Jenkins, J. A1 - Jones, Bethan M. A1 - Lawson, Tracy A1 - Leese, Florian A1 - Lindquist, Erika A1 - Lobanov, Alexei A1 - Lomsadze, Alexandre A1 - Malik, Shehre-Banoo A1 - Marsh, Mary E. A1 - Mackinder, Luke A1 - Mock, Thomas A1 - Müller-Röber, Bernd A1 - Pagarete, Antonio A1 - Parker, Micaela A1 - Probert, Ian A1 - Quesneville, Hadi A1 - Raines, Christine A1 - Rensing, Stefan A. A1 - Riano-Pachon, Diego Mauricio A1 - Richier, Sophie A1 - Rokitta, Sebastian A1 - Shiraiwa, Yoshihiro A1 - Soanes, Darren M. A1 - van der Giezen, Mark A1 - Wahlund, Thomas M. A1 - Williams, Bryony A1 - Wilson, Willie A1 - Wolfe, Gordon A1 - Wurch, Louie L. T1 - Pan genome of the phytoplankton Emiliania underpins its global distribution JF - Nature : the international weekly journal of science N2 - Coccolithophores have influenced the global climate for over 200 million years(1). These marine phytoplankton can account for 20 per cent of total carbon fixation in some systems(2). They form blooms that can occupy hundreds of thousands of square kilometres and are distinguished by their elegantly sculpted calcium carbonate exoskeletons (coccoliths), rendering them visible from space(3). Although coccolithophores export carbon in the form of organic matter and calcite to the sea floor, they also release CO2 in the calcification process. Hence, they have a complex influence on the carbon cycle, driving either CO2 production or uptake, sequestration and export to the deep ocean(4). Here we report the first haptophyte reference genome, from the coccolithophore Emiliania huxleyi strain CCMP1516, and sequences from 13 additional isolates. Our analyses reveal a pan genome (core genes plus genes distributed variably between strains) probably supported by an atypical complement of repetitive sequence in the genome. Comparisons across strains demonstrate that E. huxleyi, which has long been considered a single species, harbours extensive genome variability reflected in different metabolic repertoires. Genome variability within this species complex seems to underpin its capacity both to thrive in habitats ranging from the equator to the subarctic and to form large-scale episodic blooms under a wide variety of environmental conditions. Y1 - 2013 U6 - https://doi.org/10.1038/nature12221 SN - 0028-0836 SN - 1476-4687 VL - 499 IS - 7457 SP - 209 EP - 213 PB - Nature Publ. Group CY - London ER - TY - JOUR A1 - Ikram, M. Arfan A1 - Fornage, Myriam A1 - Smith, Albert V. A1 - Seshadri, Sudha A1 - Schmidt, Reinhold A1 - Debette, Stephanie A1 - Vrooman, Henri A. A1 - Sigurdsson, Sigurdur A1 - Ropele, Stefan A1 - Taal, H. Rob A1 - Mook-Kanamori, Dennis O. A1 - Coker, Laura H. A1 - Longstreth, W. T. A1 - Niessen, Wiro J. A1 - DeStefano, Anita L. A1 - Beiser, Alexa A1 - Zijdenbos, Alex P. A1 - Struchalin, Maksim A1 - Jack, Clifford R. A1 - Rivadeneira, Fernando A1 - Uitterlinden, Andre G. A1 - Knopman, David S. A1 - Hartikainen, Anna-Liisa A1 - Pennell, Craig E. A1 - Thiering, Elisabeth A1 - Steegers, Eric A. P. A1 - Hakonarson, Hakon A1 - Heinrich, Joachim A1 - Palmer, Lyle J. A1 - Jarvelin, Marjo-Riitta A1 - McCarthy, Mark I. A1 - Grant, Struan F. A. A1 - St Pourcain, Beate A1 - Timpson, Nicholas J. A1 - Smith, George Davey A1 - Sovio, Ulla A1 - Nalls, Mike A. A1 - Au, Rhoda A1 - Hofman, Albert A1 - Gudnason, Haukur A1 - van der Lugt, Aad A1 - Harris, Tamara B. A1 - Meeks, William M. A1 - Vernooij, Meike W. A1 - van Buchem, Mark A. A1 - Catellier, Diane A1 - Jaddoe, Vincent W. V. A1 - Gudnason, Vilmundur A1 - Windham, B. Gwen A1 - Wolf, Philip A. A1 - van Duijn, Cornelia M. A1 - Mosley, Thomas H. A1 - Schmidt, Helena A1 - Launer, Lenore J. A1 - Breteler, Monique M. B. A1 - DeCarli, Charles A1 - Adair, Linda S. A1 - Ang, Wei A1 - Atalay, Mustafa A1 - vanBeijsterveldt, Toos A1 - Bergen, Nienke A1 - Benke, Kelly A1 - Berry, Diane J. A1 - Coin, Lachlan A1 - Davis, Oliver S. P. A1 - Elliott, Paul A1 - Flexeder, Claudia A1 - Frayling, Tim A1 - Gaillard, Romy A1 - Groen-Blokhuis, Maria A1 - Goh, Liang-Kee A1 - Haworth, Claire M. A. A1 - Hadley, Dexter A1 - Hebebrand, Johannes A1 - Hinney, Anke A1 - Hirschhorn, Joel N. A1 - Holloway, John W. A1 - Holst, Claus A1 - Hottenga, Jouke Jan A1 - Horikoshi, Momoko A1 - Huikari, Ville A1 - Hypponen, Elina A1 - Kilpelainen, Tuomas O. A1 - Kirin, Mirna A1 - Kowgier, Matthew A1 - Lakka, Hanna-Maaria A1 - Lange, Leslie A. A1 - Lawlor, Debbie A. A1 - Lehtimaki, Terho A1 - Lewin, Alex A1 - Lindgren, Cecilia A1 - Lindi, Virpi A1 - Maggi, Reedik A1 - Marsh, Julie A1 - Middeldorp, Christel A1 - Millwood, Iona A1 - Murray, Jeffrey C. A1 - Nivard, Michel A1 - Nohr, Ellen Aagaard A1 - Ntalla, Ioanna A1 - Oken, Emily A1 - Panoutsopoulou, Kalliope A1 - Pararajasingham, Jennifer A1 - Rodriguez, Alina A1 - Salem, Rany M. A1 - Sebert, Sylvain A1 - Siitonen, Niina A1 - Strachan, David P. A1 - Teo, Yik-Ying A1 - Valcarcel, Beatriz A1 - Willemsen, Gonneke A1 - Zeggini, Eleftheria A1 - Boomsma, Dorret I. A1 - Cooper, Cyrus A1 - Gillman, Matthew A1 - Hocher, Berthold A1 - Lakka, Timo A. A1 - Mohlke, Karen L. A1 - Dedoussis, George V. A1 - Ong, Ken K. A1 - Pearson, Ewan R. A1 - Price, Thomas S. A1 - Power, Chris A1 - Raitakari, Olli T. A1 - Saw, Seang-Mei A1 - Scherag, Andre A1 - Simell, Olli A1 - Sorensen, Thorkild I. A. A1 - Wilson, James F. T1 - Common variants at 6q22 and 17q21 are associated with intracranial volume JF - Nature genetics N2 - During aging, intracranial volume remains unchanged and represents maximally attained brain size, while various interacting biological phenomena lead to brain volume loss. Consequently, intracranial volume and brain volume in late life reflect different genetic influences. Our genome-wide association study (GWAS) in 8,175 community-dwelling elderly persons did not reveal any associations at genome-wide significance (P < 5 x 10(-8)) for brain volume. In contrast, intracranial volume was significantly associated with two loci: rs4273712 (P = 3.4 x 10(-11)), a known height-associated locus on chromosome 6q22, and rs9915547 (P = 1.5 x 10(-12)), localized to the inversion on chromosome 17q21. We replicated the associations of these loci with intracranial volume in a separate sample of 1,752 elderly persons (P = 1.1 x 10(-3) for 6q22 and 1.2 x 10(-3) for 17q21). Furthermore, we also found suggestive associations of the 17q21 locus with head circumference in 10,768 children (mean age of 14.5 months). Our data identify two loci associated with head size, with the inversion at 17q21 also likely to be involved in attaining maximal brain size. Y1 - 2012 U6 - https://doi.org/10.1038/ng.2245 SN - 1061-4036 VL - 44 IS - 5 SP - 539 EP - + PB - Nature Publ. Group CY - New York ER - TY - JOUR A1 - Schaffenroth, Veronika A1 - Casewell, Sarah L. A1 - Schneider, D. A1 - Kilkenny, David A1 - Geier, Stephan A1 - Heber, Ulrich A1 - Irrgang, Andreas A1 - Przybilla, Norbert A1 - Marsh, Thomas R. A1 - Littlefair, Stuart P. A1 - Dhillon, Vik S. T1 - A quantitative in-depth analysis of the prototype sdB plus BD system SDSS J08205+0008 revisited in the Gaia era JF - Monthly notices of the Royal Astronomical Society N2 - Subdwarf B stars are core-helium-burning stars located on the extreme horizontal branch (EHB). Extensive mass loss on the red giant branch is necessary to form them. It has been proposed that substellar companions could lead to the required mass loss when they are engulfed in the envelope of the red giant star. J08205+0008 was the first example of a hot subdwarf star with a close, substellar companion candidate to be found. Here, we perform an in-depth re-analysis of this important system with much higher quality data allowing additional analysis methods. From the higher resolution spectra obtained with ESO-VLT/XSHOOTER, we derive the chemical abundances of the hot subdwarf as well as its rotational velocity. Using the Gaia parallax and a fit to the spectral energy distribution in the secondary eclipse, tight constraints to the radius of the hot subdwarf are derived. From a long-term photometric campaign, we detected a significant period decrease of -3.2(8) x 10(-12) dd(-1). This can be explained by the non-synchronized hot subdwarf star being spun up by tidal interactions forcing it to become synchronized. From the rate of period decrease we could derive the synchronization time-scale to be 4 Myr, much smaller than the lifetime on EHB. By combining all different methods, we could constrain the hot subdwarf to a mass of 0.39-0.50 M-circle dot and a radius of R-sdB = 0.194 +/- 0.008 R-circle dot, and the companion to 0.061-0.071 M-circle dot with a radius of R-comp = 0.092 +/- 0.005 R-circle dot, below the hydrogen-burning limit. We therefore confirm that the companion is most likely a massive brown dwarf. KW - stars: abundances KW - stars: atmospheres KW - stars: fundamental parameters KW - stars: horizontal branch KW - stars: low-mass KW - subdwarfs Y1 - 2020 U6 - https://doi.org/10.1093/mnras/staa3661 SN - 0035-8711 SN - 1365-2966 VL - 501 IS - 3 SP - 3847 EP - 3870 PB - Oxford Univ. Press CY - Oxford ER - TY - JOUR A1 - Schaffenroth, Veronika A1 - Barlow, Brad N. A1 - Geier, Stephan A1 - Vuckovic, Maja A1 - Kilkenny, D. A1 - Wolz, M. A1 - Kupfer, Thomas A1 - Heber, Ulrich A1 - Drechsel, H. A1 - Kimeswenger, S. A1 - Marsh, T. A1 - Wolf, M. A1 - Pelisoli, Ingrid Domingos A1 - Freudenthal, Joseph A1 - Dreizler, S. A1 - Kreuzer, S. A1 - Ziegerer, E. T1 - The EREBOS project: Investigating the effect of substellar and low-mass stellar companions on late stellar evolution Survey, target selection, and atmospheric parameters JF - Astronomy and astrophysics : an international weekly journal N2 - Eclipsing post-common-envelope binaries are highly important for resolving the poorly understood, very short-lived common-envelope phase of stellar evolution. Most hot subdwarfs (sdO/Bs) are the bare helium-burning cores of red giants that have lost almost all of their hydrogen envelope. This mass loss is often triggered by common-envelope interactions with close stellar or even substellar companions. Cool companions to hot subdwarf stars such as late-type stars and brown dwarfs are detectable from characteristic light-curve variations - reflection effects and often eclipses. In the recently published catalog of eclipsing binaries in the Galactic Bulge and in the Asteroid Terrestrial-impact Last Alert System (ATLAS) survey, we discovered 125 new eclipsing systems showing a reflection effect seen by visual inspection of the light curves and using a machine-learning algorithm, in addition to the 36 systems previously discovered by the Optical Gravitational Lesing Experiment (OGLE) team. The Eclipsing Reflection Effect Binaries from Optical Surveys (EREBOS) project aims at analyzing all newly discovered eclipsing binaries of the HW Vir type (hot subdwarf + close, cool companion) based on a spectroscopic and photometric follow up to derive the mass distribution of the companions, constrain the fraction of substellar companions, and determine the minimum mass needed to strip off the red-giant envelope. To constrain the nature of the primary we derived the absolute magnitude and the reduced proper motion of all our targets with the help of the parallaxes and proper motions measured by the Gaia mission and compared those to the Gaia white-dwarf candidate catalog. It was possible to derive the nature of a subset of our targets, for which observed spectra are available, by measuring the atmospheric parameter of the primary, confirming that less than 10% of our systems are not sdO/Bs with cool companions but are white dwarfs or central stars of planetary nebula. This large sample of eclipsing hot subdwarfs with cool companions allowed us to derive a significant period distribution for hot subdwarfs with cool companions for the first time showing that the period distribution is much broader than previously thought and is ideally suited to finding the lowest-mass companions to hot subdwarf stars. The comparison with related binary populations shows that the period distribution of HW Vir systems is very similar to WD+dM systems and central stars of planetary nebula with cool companions. In the future, several new photometric surveys will be carried out, which will further increase the sample of this project, providing the potential to test many aspects of common-envelope theory and binary evolution. KW - binaries: eclipsing KW - brown dwarfs KW - binaries: spectroscopic KW - binaries: close KW - subdwarfs KW - surveys Y1 - 2019 U6 - https://doi.org/10.1051/0004-6361/201936019 SN - 1432-0746 VL - 630 PB - EDP Sciences CY - Les Ulis ER - TY - JOUR A1 - Fusillo, Nicola Pietro Gentile A1 - Tremblay, Pier-Emmanuel A1 - Gänsicke, Boris T. A1 - Manser, Christopher J. A1 - Cunningham, Tim A1 - Cukanovaite, Elena A1 - Hollands, Mark A1 - Marsh, Thomas A1 - Raddi, Roberto A1 - Jordan, Stefan A1 - Toonen, Silvia A1 - Geier, Stephan A1 - Barstow, Martin A1 - Cummings, Jeffrey D. T1 - A Gaia Data Release 2 catalogue of white dwarfs and a comparison with SDSS JF - Monthly notices of the Royal Astronomical Society N2 - We present a catalogue of white dwarf candidates selected from the second data release of Gaia (DR2). We used a sample of spectroscopically confirmed white dwarfs from the Sloan Digital Sky Survey (SDSS) to map the entire space spanned by these objects in the Gaia Hertzsprung–Russell diagram. We then defined a set of cuts in absolute magnitude, colour, and a number of Gaia quality flags to remove the majority of contaminating objects. Finally, we adopt a method analogous to the one presented in our earlier SDSS photometric catalogues to calculate a probability of being a white dwarf (PWD) for all Gaia sources that passed the initial selection. The final catalogue is composed of 486641 stars with calculated PWD from which it is possible to select a sample of ≃260000 high-confidence white dwarf candidates in the magnitude range 8 < G < 21. By comparing this catalogue with a sample of SDSS white dwarf candidates, we estimate an upper limit in completeness of 85 per cent for white dwarfs with G ≤ 20 mag and Teff >7000 K, at high Galactic latitudes (|b| > 20°). However, the completeness drops at low Galactic latitudes, and the magnitude limit of the catalogue varies significantly across the sky as a function of Gaia’s scanning law. We also provide the list of objects within our sample with available SDSS spectroscopy. We use this spectroscopic sample to characterize the observed structure of the white dwarf distribution in the H–R diagram. KW - catalogues KW - surveys KW - white dwarfs Y1 - 2018 U6 - https://doi.org/10.1093/mnras/sty3016 SN - 0035-8711 SN - 1365-2966 VL - 482 IS - 4 SP - 4570 EP - 4591 PB - Oxford Univ. Press CY - Oxford ER -