LEADER 01056nam--2200373---450- 001 990003134070203316 005 20080730112502.0 035 $a000313407 035 $aUSA01000313407 035 $a(ALEPH)000313407USA01 035 $a000313407 100 $a20080730d1976----km-y0itay50------ba 101 $aita 102 $aIT 105 $a||||||||001yy 200 1 $a<> ceramica orientale, africana e precolombiana$fRoberto Bosi 210 $aFaenza$cFaenza editrice$dc1976 215 $aP. 275-416, [16] p. di tav.$cill.$d27 cm. 410 0$12001 454 1$12001 461 1$1001-------$12001 606 0 $aCeramiche orientali 606 0 $aCeramiche africane 606 0 $aCeramiche precolombiane 676 $a738.09 700 1$aBOSI,$bRoberto$038451 801 0$aIT$bsalbc$gISBD 912 $a990003134070203316 951 $aS VII a 29$b97 DLM$cS VII a 959 $aBK 969 $aDILAM 979 $aDILAM$b90$c20080730$lUSA01$h1125 996 $aCeramica orientale, africana e precolombiana$91016779 997 $aUNISA LEADER 03259nam 22005655 450 001 9910300555003321 005 20260910160522.0 010 $a3-319-90957-6 024 7 $a10.1007/978-3-319-90957-8 035 $a(CKB)4100000004243978 035 $a(DE-He213)978-3-319-90957-8 035 $a(MiAaPQ)EBC5396664 035 $a(PPN)227399374 035 $a(EXLCZ)994100000004243978 100 $a20180516d2018 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aExomoons to Galactic Structure $eHigh Precision Studies with the Microlensing and Transit Methods /$fby Supachai Awiphan 205 $a1st ed.. 2018. 210 1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2018. 215 $a1 online resource (XXVI, 187 p. 72 illus., 54 illus. in color.) 225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 311 08$a3-319-90956-8 327 $aIntroduction -- TTV and Transmission Spectroscopy of GJ3470b -- Detectability of Habitable Exomoons -- Microlensing Maps of the Galaxy -- Besan¸Con Model Simulations of MOA-II -- Summary and Future Works. 330 $aThis book presents three major studies covering exomoon and exoplanet detection and characterisation. Firstly, it reports the observations and analysis of the atmosphere of the hot Neptune GJ3470b, one of the lowest-mass planets with a measured atmosphere, using transmission spectroscopy techniques. The result provided improved measurements of Rayleigh scattering in the atmosphere and the first limits on additional planetary companions in the system. The second part discusses modeling a Kepler-like satellite?s ability of a to detect exomoons by looking for transit timing variations and transit duration variations, demonstrating how exomoons can unambiguously be identified from such data.Lastly, the book examines the development of a state-of-the-art Galactic microlensing simulator, which has been made publicly available. It was used to compare with the largest published sample of microlensing events from the MOA-II survey. 410 0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 606 $aAstronomy$vObservations 606 $aAstronomy?Observations 606 $aPlanetary science 606 $aExobiology 606 $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014 606 $aPlanetary Sciences$3https://scigraph.springernature.com/ontologies/product-market-codes/P22060 606 $aAstrobiology$3https://scigraph.springernature.com/ontologies/product-market-codes/P22057 615 0$aAstronomy 615 0$aAstronomy?Observations. 615 0$aPlanetary science. 615 0$aExobiology. 615 14$aAstronomy, Observations and Techniques. 615 24$aPlanetary Sciences. 615 24$aAstrobiology. 676 $a520 700 $aAwiphan$4aut$4http://id.loc.gov/vocabulary/relators/aut$02018393 701 $a Supachai.$02018394 906 $aBOOK 912 $a9910300555003321 996 $aExomoons to Galactic Structure$94809925 997 $aUNINA