activity
20042026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 17.2k across the 40 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

13 papers · 1 filter

astro-ph.IM2023★ 10 cited

Euclid preparation. XXIX. Water ice in spacecraft part I: The physics of ice formation and contamination

Euclid Collaboration, M. Schirmer, K. Thürmer +218

Molecular contamination is a well-known problem in space flight. Water is the most common contaminant and alters numerous properties of a cryogenic optical system. Too much ice mea…

astro-ph.IM2021★ 134 cited

Gaia Photometric Science Alerts

S. T. Hodgkin, D. L. Harrison, E. Breedt +108

Since July 2014, the Gaia mission has been engaged in a high-spatial-resolution, time-resolved, precise, accurate astrometric, and photometric survey of the entire sky. Aims: We pr…

astro-ph.IM2020★ 1.2k cited

Gaia Early Data Release 3: The astrometric solution

L. Lindegren, S. A. Klioner, J. Hernández +94

Gaia Early Data Release 3 (Gaia EDR3) contains results for 1.812 billion sources in the magnitude range G = 3 to 21 based on observations collected by the European Space Agency Gai…

astro-ph.IM2020★ 1k cited

Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

L. Lindegren, U. Bastian, M. Biermann +14

Gaia Early Data Release 3 (Gaia EDR3) gives trigonometric parallaxes for nearly 1.5 billion sources. Inspection of the EDR3 data for sources identified as quasars reveals that thei…

astro-ph.IM2020★ 64 cited

Gaia Early Data Release 3: Modelling and calibration of Gaia's point and line spread functions

N. Rowell, M. Davidson, L. Lindegren +18

Context: The unprecedented astrometric precision of the Gaia mission relies on accurate estimates of the locations of sources in the Gaia data stream. This is ultimately performed…

astro-ph.IM2019★ 17 cited

Expectations on the mass determination using astrometric microlensing by Gaia

J. Klüter, U. Bastian, J. Wambsganss

Context. Astrometric gravitational microlensing can be used to determine the mass of a single star (the lens) with an accuracy of a few percent. To do so, precise measurements of t…