Classical and Quantum Gravity

Resonant mass detectors: present status
pp. 1227-1235(9)
Author: Astone P.

Japanese large-scale interferometers
pp. 1237-1245(9)
Authors: Kuroda K.; Ohashi M.; Miyoki S.; Ishizuka H.; Taylor C.T.; Yamamoto K.; Miyakawa O.; Fujimoto M-K.; Kawamura S.; Takahashi R.; Yamazaki T.; Arai K.; Tatsumi D.; Ueda A.; Fukushima M.; Sato S.; Shintomi T.; Yamamoto A.; Suzuki T.; Saito Y.; Haruyama T.; Sato N.; Higashi Y.; Uchiyama T.; Tomaru T.; Tsubono K.; Ando M.; Takamori A.; Numata K.; Ueda K-I.; Yoneda H.; Nakagawa K.; Musha M.; Mio N.; Moriwaki S.; Somiya K.; Araya A.; Kanda N.; Telada S.; Sasaki M.; Tagoshi H.; Nakamura T.; Tanaka T.; Ohara K.

Gravitational radiation from the r-mode instability
pp. 1247-1253(7)
Authors: Owen B.J.; Lindblom L.

Gravitational waves from rotating strained neutron stars
pp. 1255-1265(11)
Author: Jones D.I.

Gravitational waves from inspiralling binary black holes
pp. 1267-1278(12)
Author: Buonanno A.

Making maps with LISA
pp. 1279-1283(5)
Author: Cornish N.J.

Radiation-balanced simulations for binary inspiral
pp. 1285-1290(6)
Authors: Whelan J.T.; Beetle C.; Landry W.; Price R.H.

Gravitational waves from relativistic rotational core collapse in axisymmetry
pp. 1291-1296(6)
Authors: Dimmelmeier H.; Font J.A.; Müller E.

Gravitational radiation from black hole binaries in globular clusters
pp. 1297-1302(6)
Author: Benacquista M.J.

Statistical characteristics of a stochastic background of gravitational waves from neutron star formation
pp. 1303-1307(5)
Authors: Coward D.; Burman R.; Blair D.

Gamma-ray bursts: calorimetry on echoes in gravitational waves
pp. 1309-1315(7)
Authors: Putten M.H.P.M.v.; Levinson A.

Black-hole galactic nuclei: a high-energy perspective
pp. 1317-1319(3)
Authors: Boldt E.; Levinson A.; Loewenstein M.

Gravitational waves from rotating neutron stars and evaluation of fast chirp transform techniques
pp. 1321-1326(6)
Author: Strohmayer T.E.

A study of the gravitational wave form from pulsars
pp. 1327-1334(8)
Authors: Valluri S.R.; Drozd J.J.; Chishtie F.A.; Biggs R.G.; Davison M.; Dhurandhar S.V.; Sathyaprakash B.S.

Background of gravitational waves from pre-galactic black hole formation
pp. 1335-1342(8)
Authors: Araujo J.C.N.d.; Miranda O.D.; Aguiar O.D.

On the sole influence of plane gravitational waves on the magnitude of the gradient of a scalar field
pp. 1343-1349(7)
Author: Melek M.

Non-Dopplerian cosmological redshift parameters in a model of graviton-dusty universe
pp. 1351-1354(4)
Author: Ivanov M.A.

Bounding the graviton mass with binary pulsar observations
pp. 1355-1360(6)
Authors: Sutton P.J.; Finn L.S.

Influence of gravitational lensing on sources of gravitational radiation
pp. 1361-1366(6)
Authors: Zakharov A.F.; Baryshev Y.V.

Search for gravitational wave bursts by the network of resonant detectors
pp. 1367-1375(9)
Authors: Astone P.; Baggio L.; Busby D.; Bassan M.; Blair D.G.; Bonaldi M.; Bonifazi P.; Carelli P.; Cerdonio M.; Coccia E.; Conti L.; Cosmelli C.; D'Antonio S.; Fafone V.; Falferi P.; Fortini P.; Frasca S.; Hamilton W.O.; Heng I.S.; Ivanov E.N.; Johnson W.W.; Locke C.R.; Marini A.; Mauceli E.; McHugh M.P.; Mezzena R.; Minenkov Y.; Modena I.; Modestino G.; Moleti A.; Ortolan A.; Pallottino G.V.; Pizzella G.; Prodi G.A.; Quintieri L.; Rocchi A.; Rocco E.; Ronga F.; Salemi F.; Santostasi G.; Taffarello L.; Terenzi R.; Tobar M.E.; Vedovato G.; Vinante A.; Visco M.; Vitale S.; Zendri J.P.; Collaboration .G.E.

The GEO 600 gravitational wave detector
pp. 1377-1387(11)
Authors: Willke B.; Aufmuth P.; Aulbert C.; Babak S.; Balasubramanian R.; Barr B.W.; Berukoff S.; Bose S.; Cagnoli G.; Casey M.M.; Churches D.; Clubley D.; Colacino C.N.; Crooks D.R.M.; Cutler C.; Danzmann K.; Davies R.; Dupuis R.; Elliffe E.; Fallnich C.; Freise A.; Goßler S.; Grant A.; Grote H.; Heinzel G.; Heptonstall A.; Heurs M.; Hewitson M.; Hough J.; Jennrich O.; Kawabe K.; Kötter K.; Leonhardt V.; Lück H.; Malec M.; McNamara P.W.; McIntosh S.A.; Mossavi K.; Mohanty S.; Mukherjee S.; Nagano S.; Newton G.P.; Owen B.J.; Palmer D.; Papa M.A.; Plissi M.V.; Quetschke V.; Robertson D.I.; Robertson N.A.; Rowan S.; Rüdiger A.; Sathyaprakash B.S.; Schilling R.; Schutz B.F.; Senior R.; Sintes A.M.; Skeldon K.D.; Sneddon P.; Stief F.; Strain K.A.; Taylor I.; Torrie C.I.; Vecchio A.; Ward H.; Weiland U.; Welling H.; Williams P.; Winkler W.; Woan G.; Zawischa I.

Performance of a 1200 m long suspended Fabry-Perot cavity
pp. 1389-1397(9)
Authors: Freise A.; Casey M.M.; Gossler S.; Grote H.; Heinzel G.; Lück H.; Robertson D.I.; Strain K.A.; Ward H.; Willke B.; Hough J.; Danzmann K.

Data acquisition and detector characterization of GEO600
pp. 1399-1407(9)
Authors: Kötter K.; Aulbert C.; Babak S.; Balasubramanian R.; Berukoff S.; Bose S.; Churches D.; Colacino C.N.; Cutler C.; Danzmann K.; Davies R.; Dupuis R.; Freise A.; Grote H.; Heinzel G.; Hewitson M.; Hough J.; Lück H.; Malec M.; Mohanty S.D.; Mukherjee S.; Nagano S.; Papa M.A.; Robertson D.; Sathyaprakash B.S.; Schutz B.F.; Sintes A.M.; Strain K.A.; Taylor I.J.; Vecchio A.; Ward H.; Weiland U.; Willke B.; Woan G.

Current status of TAMA
pp. 1409-1419(11)
Authors: Ando M.; collaboration t.T.

Commissioning of the LIGO detectors
pp. 1429-1435(7)
Author: Sigg D.

A robust and coherent network statistic for detecting gravitational waves from inspiralling compact binaries in non-Gaussian noise
pp. 1437-1442(6)
Author: Bose S.

Coincidence analysis in gravitational wave experiments
pp. 1443-1448(6)
Authors: Astone P.; Antonio S.D.; Pizzella G.

LISA and gravitational-wave stochastic backgrounds
pp. 1449-1455(7)
Author: Vecchio A.

Parametric adaptive filtering and data validation in the bar GW detector AURIGA
pp. 1457-1464(8)
Authors: Ortolan A.; Baggio L.; Cerdonio M.; Prodi G.A.; Vedovato G.; Vitale S.

Network sensitivity to geographical configuration
pp. 1465-1470(6)
Authors: Searle A.C.; Scott S.M.; McClelland D.E.

Towards a data and detector characterization robot for gravitational wave detectors
pp. 1471-1476(6)
Authors: Mohanty S.D.; Mukherjee S.

Computational cost for detecting inspiralling binaries using a network of laser interferometric detectors
pp. 1477-1483(7)
Authors: Pai A.; Bose S.; Dhurandhar S.

A technique to modulate the signature of a stochastic gravitational wave background
pp. 1485-1492(8)
Authors: Lazzarini A.; Finn L.S.

A method for the detection of gravitational waves from inspiralling compact binaries using a fast chirp transform
pp. 1493-1498(6)
Authors: Charlton P.R.; Anderson S.B.; Blackburn J.K.; Edlund J.; Jenet F.A.; Lazzarini A.; Prince T.A.; Tinto M.; Wen L.

The online data filters for Explorer and Nautilus
pp. 1499-1505(7)
Author: D'Antonio S.

Extended hierarchical search (EHS) algorithm for detection of gravitational waves from inspiralling compact binaries
pp. 1507-1512(6)
Authors: Sengupta A.S.; Dhurandhar S.V.; Lazzarini A.; Prince T.

Median based line tracker (MBLT): model independent and transient preserving line removal from interferometric data
pp. 1513-1519(7)
Author: Mohanty S.D.

Progress on stochastic background search codes for LIGO
pp. 1521-1527(7)
Authors: Whelan J.T.; Anderson W.G.; Casquette M.; Díaz M.C.; Heng I.S.; McHugh M.; Romano J.D.; Jr C.W.T.; Trejo R.M.; Vecchio A.

A procedure for noise uncoupling in laser interferometry
pp. 1529-1536(8)
Authors: Barone F.; Calloni E.; Rosa R.D.; Eleuteri A.; Milano L.; Qipiani K.

Network data analysis server (NDAS) prototype development
pp. 1537-1540(4)
Authors: Márka S.; Mours B.; Williams R.

IGEC toolbox for coincidence search
pp. 1541-1546(6)
Authors: Baggio L.; Cerdonio M.; Heng I.S.; Ortolan A.; Prodi G.A.; Rocco E.; Vedovato G.; Vitale S.

Dual recycling for GEO 600
pp. 1547-1553(7)
Authors: Heinzel G.; Freise A.; Grote H.; Strain K.; Danzmann K.

Development of a suspended-mass RSE interferometer using third harmonic demodulation
pp. 1555-1560(6)
Authors: Miyakawa O.; Somiya K.; Heinzel G.; Kawamura S.

Variable reflectivity signal mirrors and signal response measurements
pp. 1561-1568(8)
Authors: Vine G.d.; Shaddock D.A.; McClelland D.E.

Laser-interferometer gravitational-wave optical-spring detectors
pp. 1569-1574(6)
Authors: Buonanno A.; Chen Y.

Advanced LIGO optical configuration and prototyping effort
pp. 1575-1584(10)
Author: Weinstein A.

Results from the Stanford 10 m Sagnac interferometer
pp. 1585-1589(5)
Authors: Beyersdorf P.T.; Byer R.L.; Fejer M.M.

Seismic isolation for Advanced LIGO
pp. 1591-1597(7)
Authors: Abbott R.; Adhikari R.; Allen G.; Cowley S.; Daw E.; DeBra D.; Giaime J.; Hammond G.; Hammond M.; Hardham C.; How J.; Hua W.; Johnson W.; Lantz B.; Mason K.; Mittleman R.; Nichol J.; Richman S.; Rollins J.; Shoemaker D.; Stapfer G.; Stebbins R.

Improvement of the vibration isolation system for TAMA300
pp. 1599-1604(6)
Authors: Takahashi R.; Arai K.; collaboration t.T.

Anatomy of the TAMA SAS seismic attenuation system
pp. 1605-1614(10)
Authors: Márka S.; Takamori A.; Ando M.; Bertolini A.; Cella G.; DeSalvo R.; Fukushima M.; Iida Y.; Jacquier F.; Kawamura S.; Nishi Y.; Numata K.; Sannibale V.; Somiya K.; Takahashi R.; Tariq H.; Tsubono K.; Ugas J.; Viboud N.; Wang C.; Yamamoto H.; Yoda T.

Mirror suspension system for the TAMA SAS
pp. 1615-1621(7)
Authors: Takamori A.; Ando M.; Bertolini A.; Cella G.; DeSalvo R.; Fukushima M.; Iida Y.; Jacquier F.; Kawamura S.; Márka S.; Nishi Y.; Numata K.; Sannibale V.; Somiya K.; Takahashi R.; Tariq H.; Tsubono K.; Ugas J.; Viboud N.; Yamamoto H.; Yoda T.; Wang C.

The VIRGO suspensions
pp. 1623-1629(7)
Author: Braccini T.V.C..b.S.

The inertial damping of the VIRGO superattenuator and the residual motion of the mirror
pp. 1631-1637(7)
Author: Losurdo T.V.C..b.G.

Using Euler buckling springs for vibration isolation
pp. 1639-1645(7)
Authors: Winterflood J.; Barber T.; Blair D.G.

Application of a high-performance damping metal to gravitational wave detectors
pp. 1647-1654(8)
Authors: Mio N.; Tanji T.; Moriwaki S.

Silica research in Glasgow
pp. 1655-1662(8)
Authors: Barr B.W.; Cagnoli G.; Casey M.M.; Clubley D.; Crooks D.R.M.; Danzmann K.; Ellife E.J.; Goßler S.; Grant A.; Grote H.; Heptonstall A.; Hough J.; Jennrich O.; Lück H.; McIntosh S.A.; Newton G.P.; Palmer D.A.; Plissi M.V.; Robertson D.I.; Robertson N.A.; Rowan S.; Skeldon K.D.; Sneddon P.; Strain K.A.; Torrie C.I.; Ward H.; Willems P.A.; Willke B.; Winkler W.

Mechanical quality factor of mirror substrates for VIRGO
pp. 1663-1668(6)
Authors: Amico P.; Bosi L.; Carbone L.; Gammaitoni L.; Punturo M.; Travasso F.; Vocca H.

Fused silica suspension for the VIRGO optics: status and perspectives
pp. 1669-1674(6)
Authors: Amico P.; Bosi L.; Carbone L.; Gammaitoni L.; Punturo M.; Travasso F.; Vocca H.

Status of the low frequency facility experiment
pp. 1675-1682(8)
Authors: Bracci L.; Calamai G.; Cuoco E.; Dominici P.; Fabbroni L.; Guidi G.; Losurdo G.; Martelli F.; Mazzoni M.; Stanga R.; Vetrano F.; Porzio A.; Ricciardi I.; Solimeno S.; Ballardin G.; Braccini S.; Bradaschia C.; Casciano C.; Cavalieri R.; Cecchi R.; Cella G.; Dattilo V.; Virgilio A.D.; Fazzi M.; Ferrante I.; Fidecaro F.; Frasconi F.; Gennaro G.; Giazotto A.; Holloway L.; Penna P.L.; Lomtadze T.; Nenci F.; Nicolosi L.; Lelli F.; Paoletti F.; Pasqualetti A.; Passaquieti R.; Passuello D.; Poggiani R.; Raffaelli F.; Taddei R.; Viceré A.; Zhang Z.; Frasca S.; Majorana E.; Palomba C.; Perciballi M.; Puppo P.; Rapagnani P.; Ricci F.

High dynamic range flexure transfer function measurement
pp. 1683-1687(5)
Authors: Slagmolen B.J.J.; Brokmann X.; Shaddock D.A.; Gray M.B.; McClelland D.E.

Study of the thermal noise caused by inhomogeneously distributed loss
pp. 1689-1696(8)
Authors: Yamamoto K.; Otsuka S.; Ando M.; Kawabe K.; Tsubono K.

Intrinsic losses in various kinds of fused silica
pp. 1697-1702(6)
Authors: Numata K.; Otsuka S.; Ando M.; Tsubono K.

Low loss niobium flexure suspension systems
pp. 1703-1708(6)
Authors: Ju L.; Blair D.G.; Bilenko I.; Paget D.

Cross-correlation studies with seismic noise
pp. 1709-1716(8)
Authors: Hoffmann H.; Winterflood J.; Cheng Y.; Blair D.G.

Towards measuring the off-resonant thermal noise of a pendulum mirror
pp. 1717-1721(5)
Authors: Leonhardt V.; Ribichini L.; Klövekorn P.; Willke B.; Lück H.; Danzmann K.

Tilt sensor and servo control system for gravitational wave detection
pp. 1723-1729(7)
Authors: Cheng Y.; Winterflood J.; Ju L.; Blair D.G.

Interferometry developments for LISA and SMART-2
pp. 1731-1737(7)
Authors: Jennrich O.; McNamara P.; Robertson D.; Rowan S.; Ward H.; Hough J.

Drag-free performance in a LISA mission with spherical proof masses
pp. 1739-1743(5)
Author: Lange B.

A Newton thrust-stand for LISA
pp. 1745-1750(6)
Authors: Merkowitz S.M.; Maghami P.G.; Sharma A.; Willis W.D.; Zakrzwski C.M.

Position sensors for LISA drag-free control
pp. 1751-1756(6)
Authors: Weber W.J.; Cavalleri A.; Dolesi R.; Fontana G.; Hueller M.; Vitale S.

Torsion pendulum facility for ground testing of gravitational sensors for LISA
pp. 1757-1765(9)
Authors: Hueller M.; Cavalleri A.; Dolesi R.; Vitale S.; Weber W.J.

The Cassini Ka-band gravitational wave experiments
pp. 1767-1773(7)
Author: Tinto M.

The GEO 600 laser system
pp. 1775-1781(7)
Authors: Zawischa I.; Brendel M.; Danzmann K.; Fallnich C.; Heurs M.; Nagano S.; Quetschke V.; Welling H.; Willke B.

High-power Nd:YAG lasers using stable-unstable resonators
pp. 1783-1792(10)
Authors: Mudge D.; Ostermeyer M.; Ottaway D.J.; Veitch P.J.; Munch J.; Hamilton M.W.

Method for compensation of thermally induced modal distortions in the input optical components of gravitational wave interferometers
pp. 1793-1801(9)
Authors: Mueller G.; Amin R.S.; Guagliardo D.; McFeron D.; Lundock R.; Reitze D.H.; Tanner D.B.

Adaptive thermal compensation of test masses in advanced LIGO
pp. 1803-1812(10)
Authors: Lawrence R.; Zucker M.; Fritschel P.; Marfuta P.; Shoemaker D.

An adaptive optics approach to the reduction of misalignments and beam jitters in gravitational wave interferometers
pp. 1813-1818(6)
Authors: Baker J.T.; Barone F.; Calloni E.; Rosa R.D.; Fiore L.D.; Eleuteri A.; Milano L.; Restaino S.; Quipiani K.

Double pass locking and spatial mode locking for gravitational wave detectors
pp. 1819-1824(6)
Authors: Cusack B.J.; Shaddock D.A.; Slagmolen B.J.J.; Vine G.d.; Gray M.B.; McClelland D.E.

LIGO sensing system performance
pp. 1825-1828(4)
Author: Landry M.

The VIRGO injection system
pp. 1829-1833(5)
Authors: Bondu F.; Brillet A.; Cleva F.; Heitmann H.; Loupias M.; Man C.N.; Trinquet H.; Collaboration t.V.

The modecleaner system and suspension aspects of GEO 600
pp. 1835-1842(8)
Authors: Gossler S.; Casey M.M.; Freise A.; Grote H.; Lück H.; McNamara P.; Plissi M.V.; Robertson D.I.; Robertson N.A.; Skeldon K.; Strain K.A.; Torrie C.I.; Ward H.; Willke B.; Hough J.; Danzmann K.

Sensing and controls for power-recycling of TAMA300
pp. 1843-1848(6)
Authors: Arai K.; Collaboration T.

The automatic alignment system of GEO 600
pp. 1849-1855(7)
Authors: Grote H.; Heinzel G.; Freise A.; Gossler S.; Willke B.; Lück H.; Ward H.; Casey M.; Strain K.A.; Robertson D.; Hough J.; Danzmann K.

Interferometer signal detection system for the VIRGO experiment
pp. 1857-1863(7)
Author: Flaminio T.V.C..b.R.

Broadband Faraday isolator for gravitational wave detectors
pp. 1865-1870(6)
Authors: Parfenov V.A.; Parfenov V.A.

Improved sensitivity of NIOBÉ in 2001 and the search for anomalous cosmic ray events
pp. 1871-1875(5)
Authors: Coward D.; Blair D.; Clay R.; Mazzitelli G.

Properties of a monolithic sapphire parametric transducer: prospects of measuring the standard quantum limit
pp. 1877-1888(12)
Authors: Locke C.R.; Tobar M.E.; Ivanov E.N.

Allegro: noise performance and the ongoing search for gravitational waves
pp. 1889-1895(7)
Authors: Heng I.S.; Daw E.; Giaime J.; Hamilton W.O.; Mchugh M.P.; Johnson W.W.

Anomalous signals due to cosmic rays observed by the bar gravitational wave detector NAUTILUS
pp. 1897-1903(7)
Authors: Astone P.; Babusci D.; Bassan M.; Bonifazi P.; Coccia E.; D'Antonio S.; Fafone V.; Giordano G.; Marini A.; Minenkov Y.; Modena I.; Modestino G.; Moleti A.; Pallottino G.V.; Pizzella G.; Quintieri L.; Ronga F.; Terenzi R.; Visco M.

The EXPLORER gravitational wave antenna: recent improvements and performances
pp. 1905-1910(6)
Authors: Astone P.; Bassan M.; Bonifazi P.; Carelli P.; Castellano M.G.; Cavallari G.; Coccia E.; Cosmelli C.; D'Antonio S.; Fafone V.; Federici G.; Minenkov Y.; Modestino G.; Modena I.; Moleti A.; Pizzella G.; Pallottino G.V.; Quintieri L.; Rocchi A.; Ronga F.; Terenzi R.; Torrioli G.; Visco M.

The next science run of the gravitational wave detector NAUTILUS
pp. 1911-1917(7)
Authors: Astone P.; Babusci D.; Bassan M.; Bonifazi P.; Coccia E.; D'Antonio S.; Fafone V.; Giordano G.; Marini A.; Minenkov Y.; Modena I.; Modestino G.; Moleti A.; Pallottino G.V.; Pizzella G.; Quintieri L.; Rocchi A.; Ronga F.; Terenzi R.; Visco M.

First room temperature operation of the AURIGA optical readout
pp. 1919-1924(6)
Authors: Rosa M.D.; Baggio L.; Cerdonio M.; Conti L.; Galet G.; Marin F.; Ortolan A.; Prodi G.A.; Taffarello L.; Vedovato G.; Vitale S.; Zendri J-P.

Status report and near future prospects for the gravitational wave detector AURIGA
pp. 1925-1933(9)
Authors: Zendri J-P.; Baggio L.; Bignotto M.; Bonaldi M.; Cerdonio M.; Conti L.; Rosa M.D.; Falferi P.; Fortini P.L.; Inguscio M.; Marin A.; Marin F.; Mezzena R.; Ortolan A.; Prodi G.A.; Rocco E.; Salemi F.; Soranzo G.; Taffarello L.; Vedovato G.; Vinante A.; Vitale S.

MiniGRAIL progress report 2001: the first cooldown
pp. 1935-1941(7)
Authors: Waard A.d.; Gottardi L.; Frossati G.

Development of a transducer for MiniGrail
pp. 1943-1948(6)
Authors: Gottardi L.; Waard A.d.; Frossati G.

The status of the Brazilian spherical detector
pp. 1949-1953(5)
Authors: Aguiar O.D.; Andrade L.A.; Filho L.C.; Costa C.A.; Araújo J.C.N.d.; Neto E.C.d.R.; Souza S.T.d.; Fauth A.C.; Frajuca C.; Frossati G.; Furtado S.R.; Furtado V.G.S.; Magalhães N.S.; Jr R.M.M.; Matos E.S.; Meliani M.T.; Melo J.L.; Miranda O.D.; Jr N.F.O.; Ribeiro K.L.; Salles K.B.M.; Stellati C.; Jr W.F.V.

Response of spherical gravitational wave antenna modes to high-energy cosmic ray particles
pp. 1955-1960(6)
Authors: Jr R.M.M.; Magalhães N.S.; Aguiar O.D.; Frajuca C.

Transducers for the Brazilian gravitational wave detector `Mario Schenberg'
pp. 1961-1965(5)
Authors: Frajuca C.; Ribeiro K.L.; Andrade L.A.; Jr W.F.V.; Melo J.L.; Aguiar O.D.; Magalhaes N.S.

A proposal for improving the noise floor of the gravitational wave antenna Niobè
pp. 1967-1972(6)
Authors: Ribeiro K.L.; Ivanov E.N.; Blair D.G.; Tobar M.E.; Aguiar O.D.; Frajuca C.

Fast cooling techniques for gravitational wave antennas
pp. 1973-1978(6)
Authors: Furtado S.R.; Aguiar O.D.

A 200 two-stage dc SQUID amplifier for resonant gravitational wave detectors
pp. 1979-1984(6)
Authors: Vinante A.; Bonaldi M.; Cerdonio M.; Falferi P.; Mezzena R.; Prodi G.A.; Vitale S.

Vibration isolation support design for the SCHENBERG detector
pp. 1985-1989(5)
Authors: Melo J.L.; Jr W.F.V.; Aguiar O.D.

Noise measurements and optimization of the high sensitivity capacitive transducer of AURIGA
pp. 1991-1996(6)
Authors: Marin A.; Bignotto M.; Bonaldi M.; Cerdonio M.; Falferi P.; Mezzena R.; Prodi G.A.; Soranzo G.; Taffarello L.; Vinante A.; Vitale S.; Zendri J-P.

The cross-coupled interferometer for gravitational wave detection
pp. 1997-2004(8)
Author: Mueller G.

Extension of gravity-wave interferometer operation to low frequencies
pp. 2005-2011(7)
Authors: Drever R.W.P.; Augst S.J.

A wideband and sensitive GW detector for kHz frequencies: the dual sphere
pp. 2013-2019(7)
Authors: Conti L.; Cerdonio M.; Bignotto M.; Bonaldi M.; Jr W.D.; Falferi P.; Heidmann A.; Lobo J.A.; Marin F.; Ortolan A.; Pinard M.; Prodi G.A.; Taffarello L.; Vitale S.; Zendri J-P.

Path-finding towards a cryogenic interferometer for LIGO
pp. 2021-2027(7)
Author: DeSalvo R.

Hollow sphere: a flexible multimode gravitational wave antenna
pp. 2029-2034(6)
Author: Lobo J.A.

Thermal and excess noise in suspension fibres
pp. 2035-2038(4)
Authors: Bilenko I.A.; Braginsky V.B.; Markova N.Y.

Test mass damping associated with electrostatic actuator
pp. 2039-2043(5)
Authors: Mitrofanov V.P.; Styazhkina N.A.; Tokmakov K.V.

Thermal lensing in cryogenic sapphire substrates
pp. 2045-2049(5)
Authors: Tomaru T.; Suzuki T.; Miyoki S.; Uchiyama T.; Taylor C.T.; Yamamoto A.; Shintomi T.; Ohashi M.; Kuroda K.