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Vaginal discharge among the primary school students and detection of the affection factors

Author: 10 ]
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A[ 2
A[ 34
Abernathy M[ 3 ]
ACERNESE Fausto
Allen B[ 6 ]
Andersson N[ 7 ]
Arun K[ 8 ]
BARONE Fabrizio
Barr B[ 3 ]
Barsuglia
Beker M[ 11 ]
Beveridge N[ 3 ]
Birindelli S[ 12 ]
Bose S[ 13 ]
Bosi L[ 1 ]
Braccini S[ 14 ]
Bradaschia C[ 14 ]
Bulik
By:Punturo
C[ 48
Calloni
Cella G[ 14 ]
Chelkowski S[ 21 ]
Chincarini A
Clark J[ 23 ]
Coccia
Colacino C[ 14 ]
Colas J[ 2 ]
Cumming A[ 3 ]
Cunningham L[ 3 ]
Cuoco E[ 2 ]
Danilishin S[ 26 ]
Danzmann K[ 6 ]
De Luca G[ 27 ]
De Salvo R[ 28 ]
Dent T[ 23 ]
Derosa
Di Fiore
Di Virgilio A[ 14 ]
Doets M[ 11 ]
E[ 24
E[ 4
EC[ 9
F[ 34
F[ 4
F[ 4
F[ 41
Fafone
Falferi
Flaminio R[ 31 ]
Franc J[ 31 ]
Frasconi F[ 14 ]
Freise A[ 21 ]
Fulda P[ 21 ]
G[ 34
Gair J[ 32 ]
Gemme G
Gennai A[ 21 ]
Giazotto
Glampedakis K[ 33 ]
Granata
Grote H[ 6 ]
Guidi
Hammond G[ 3 ]
Hannam M[ 36 ]
Harms J[ 37 ]
Heinert D[ 38 ]
Hendry M[ 3 ]
Heng I[ 3 ]
Hennes E[ 11 ]
Hild S[ 3 ]
Hough J[ 4 ]
Husa S[ 39 ]
Huttner S
Jones G[ 23 ]
Khalili F[ 40 ]
Kokeyama K[ 21 ]
Kokkotas K[ 33 ]
Krishnan B[ 39 ]
L[ 4
Lorenzini M[ 34 ]
Luck H[ 6 ]
M[ 1
M[ 9
M[ 9
Majorana E[ 41 ]
Mandel I[ 42 ]
Mandic V[ 37 ]
Martin I[ 3 ]
Michel C[ 31 ]
Minenkov
Morgado N[ 31 ]
Mosca
Mottin
Mours B[ 43 ]
Muller Ebhardt H[ 6 ]
Murray P[ 3 ]
Nawrodt R[ 3 ]
Nelson J[ 3 ]
Oshaughnessy R[ 44 ]
Ott CD[ 45 ]
P[ 29
P[ 41
P[ 48
Palomba C[ 41 ]
Paoli A[ 2 ]
Parguez G[ 2 ]
Pasqualetti A[ 2 ]
Passaquieti
Passuello D[ 14 ]
Pinard L[ 31 ]
Plastino
Poggiani
Popolizio P[ 2 ]
Prato M
Puppo P[ 41 ]
R[ 14
R[ 14
R[ 4
Rabeling D[ 11 ]
Rapagnani
Read J[ 39 ]
Regimbau T[ 12 ]
Rehbein H[ 6 ]
Reid S[ 3 ]
Rezzolla L[ 39 ]
Ricci
Richard F[ 2 ]
Rocchi A[ 24 ]
Rowan S[ 3 ]
Rudiger A[ 6 ]
S[ 4
Sassolas B[ 31 ]
Sathyaprakash B[ 23 ]
Schnabel R[ 6 ]
Schwarz
Seidel
Sintes A[ 39 ]
Somiya K[ 45 ]
Speirits F[ 3 ]
Strain K[ 3 ]
Strigin S[ 40 ]
Sutton P[ 23 ]
T[ 15
Tarabrin S[ 40 ]
V[ 24
Van den Brand J[ 11 ]
Van den Broeck C[ 23 ]
Van Leewen C[ 11 ]
Van Veggel M[ 3 ]
Vecchio A[ 21 ]
Veitch J[ 21 ]
Vetrano
Vicere
Vyatchanin S[ 40 ]
W[ 49
Willke B[ 6 ]
Woan G[ 3 ]
Y[ 24
Yamamoto K.
Publication venue
Publication date: 01/01/2009
Field of study

Large gravitational wave interferometric detectors, like Virgo and LIGO, demonstrated the capability to reach their design sensitivity, but to transform these machines into an effective observational instrument for gravitational wave astronomy a large improvement in sensitivity is required. Advanced detectors in the near future and third-generation observatories in more than one decade will open the possibility to perform gravitational wave astronomical observations from the Earth. An overview of the possible science reaches and the technological progress needed to realize a third-generation observatory are discussed in this paper. The status of the project Einstein Telescope (ET), a design study of a third-generation gravitational wave observatory, will be reported