LISA Symposium 2026 - Parallel 5-A @LISAcommunity

Uploaded August 2026 | Updated September 2026, 3 hours ago

(Recorded on June 25, 2026)

16th LISA Symposium Parallel Sessions
Parallel 5-A: Instrument Performance

Presentations in this session:
00:00:25 - Optical Verification of the LISA Phase Detection System
Lea Bischof

00:15:50 - Space weather science investigations with LISA
Catia Grimani

00:31:40 - An ultra-stable testbed for verification of QPD signals performance in LISA
Alvise Pizzella

00:44:15 - Performance of the LISA Radiation Monitor and its Impact on the Mission and Beyond
Marina Orta Terre

00:59:45 - Performance Testing of the Engineering Development Unit (EDU) LISA Laser System
Joseph Hart

01:13:45 - LISA Charge Management Device: environmental testing for TRL6
Francesca Barbieri

Session Chair: Jake Slutsky

LISA Symposium XIV Parallel B Cosmology Part 2

Spectral separation of the Stochastic Gravitational wave Background

Disentangling the interplanetary magnetic field from the noise generated aboard LISA Pathfinder

Gravitational wave anisotropies as a probe of the inflationary particle content

Constraining two-spin effects in GW data with an augmented definition of the precessing spin ...

The effect of a constant velocity of the source on gravitational waves

Realistic Detection and Early Warning of Binary NS with Decihertz Gravitational-wave Observatories

$Thermo-elastic and thermo-optical effects on-board LISA Pathfinder Thermal gradients on board the LISA Pathfinder mission induced effects with a potential impact to perturb the main differential acceleration measurement between both free-falling test masses. Temperature gradients across the housing produced forces through three different effects, namely asymmetric outgassing, radiation pressure and radiometer effect. The latter is related to the residual gas pressure around the test mass and, therefore, allows the estimation of the Brownian noise contribution, one of the limiting noise contributions for a future observatory like LISA. In addition to thermal forces arising due to gradients around the proof mass, thermo-optical and thermo-elastic effects can also contribute to instrument noise. There were two places where such distortion could be critical. First, the optical window, i.e. the interface between the optical bench and the test mass. This optical element the only not bonded on the Zerodur optical bench was clamped in a Titanium ring and therefore was susceptible to mechanical stress or changes in the refractive index due to thermal gradients across the glass. The second location were the struts holding the optical bench inside the thermal shield acting as the main thermal link to the outside (thermally noisier) environment. Temperature changes in these structures induced net displacements or tilts of the bench with direct impact on the interferometer read-out. During the LISA Pathfinder mission we have carried out several experiments by which we characterized and quantified the previous effects. The aim of this presentation is to update the results about the impact of thermo-elastic and thermo-optical effects, that we have obtained by analyzing the experiments, on the main differential acceleration measurement. In the same way we want to give an estimate of the impact of these thermal effects for the LISA mission. Authors: PhD Francisco Rivas (Presenting) Universidad Loyola Andalucía, Sevilla, Spain$

Log power spectral density estimation using a smoothness prior with applications to separating ...