De Angeli, F. ; Weiler, M. ; Montegriffo, P. ; Evans, D. W. ; Riello, M. ; Andrae, R. ; Carrasco, J. M. ; Busso, G. ; Burgess, P. W. ; Cacciari, C. ; Davidson, M. ; Harrison, D. L. ; Hodgkin, S. T. ; Jordi, C. ; Osborne, P. J. ; Pancino, E. ; Altavilla, G. ; Barstow, M. A. ; Bailer-Jones, C. A. L. ; Bellazzini, M. ; Brown, A. G. A. ; Castellani, M. ; Cowell, S. ; Delchambre, L. ; De Luise, F. ; Diener, C. ; Fabricius, C. ; Fouesneau, M. ; Fremat, Y. ; Gilmore, G. ; Giuffrida, G. ; Hambly, N. C. ; Hidalgo, S. ; Holland, G. ; Kostrzewa-Rutkowska, Z. ; van Leeuwen, F. ; Lobel, A. ; Marinoni, S. ; Miller, N. ; Pagani, C. ; Palaversa, L. ; Piersimoni, A. M. ; Pulone, L. ; Ragaini, S. ; Rainer, M. ; Richards, P. J. ; Rixon, G. T. ; Ruz-Mieres, D. ; Sanna, N. ; Sarro, L. M. ; Rowell, N. ; Sordo, R. ; Walton, N. A. ; Yoldas, A.

published in Astronomy & Astrophysics, 674, pp. A2 (28pp) (2023)

Abstract: Context. Blue (BP) and Red (RP) Photometer low-resolution spectral data is one of the exciting new products in Gaia Data Release 3 (Gaia DR3). These data have also been used to derive astrometry and integrated photometry in Gaia Early Data Release 3 and astrophysical parameters and Solar System Object reflectance spectra in Gaia DR3. Aims. In this paper we give an overview of the processing techniques that allow converting satellite raw data of multiple transits per source into combined spectra calibrated onto an internal reference system, resulting in low-resolution BP and RP mean spectra.We describe how we overcome challenges due to the complexity of the on-board instruments and to the various observation strategies. Furthermore, we show highlights from the scientific validation of the results. This work covers the internal calibration of BP/RP spectra onto a self-consistent mean instrument, while the calibration of the BP/RP spectra to the absolute reference system of physical flux and wavelength is covered in Montegriffo, P. et al. (2022a). This should be seen as an essential companion to this paper. Methods. We calibrate about 65 billion individual transit spectra onto the same mean BP/RP instrument through a series of calibration steps, including background subtraction, calibration of the CCD geometry and an iterative procedure for the calibration of CCD eciency as well as variations of the line-spread function and dispersion across the focal plane and in time. The calibrated transit spectra are then combined for each source in terms of an expansion into continuous basis functions. We discuss the configuration of these basis functions. Results. Time-averaged mean spectra covering the optical to near-infrared wavelength range [330; 1050] nm are published for approximately 220 million objects. Most of these are brighter than G = 17:65 but some BP/RP spectra are published for sources down to G = 21:43. Their signal-to-noise ratio varies significantly over the wavelength range covered and with magnitude and colour of the observed objects, with sources around G = 15 having S/N above 100 in some wavelength ranges. The top-quality BP/RP spectra are achieved for sources with magnitudes 9 < G < 12, having S/N reaching 1000 in the central part of the RP wavelength range. Scientific validation suggests that the internal calibration was generally successful. However, there is some evidence for imperfect calibrations at the bright end G < 11, where calibrated BP/RP spectra can exhibit systematic flux variations that exceed their estimated flux uncertainties. We also report that due to long-range noise correlations, BP/RP spectra can exhibit wiggles when sampled in pseudo-wavelength. Conclusions. The Gaia DR3 data products are the expansion coefficients and corresponding covariance matrices for BP and RP separately. Users are encouraged to work with the data in this format, with full covariance information showing that correlations between coefficients are typically very low. Documentation and instructions on how to access and use BP/RP spectral data from the archive are also provided.

Keyword(s): catalogs ; surveys ; instrumentation: photometers; spectrographs ; techniques: photometric; spectroscopy
DOI: 10.1051/0004-6361/202243680
Links: link; link2
Funding: Gaia PRODEX/Gaia PRODEX/Gaia PRODEX