The spectro point spread function for GAIA
(2002) In Astrophysics and Space Science 280(1-2). p.51-56- Abstract
- We discuss the point spread function for the Spectro instrument based on realistic effects of the time delayed integration, transverse image motion and pixelization, but assuming rather small wave front errors. Stars brighter than 10 mag, which will saturate the CCD, may be observed photometrically using the image wings, but the central wavelengths will be slightly shifted towards the red.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/118558
- author
- Fabricius, C and Lindegren, Lennart LU
- organization
- publishing date
- 2002
- type
- Contribution to journal
- publication status
- published
- subject
- in
- Astrophysics and Space Science
- volume
- 280
- issue
- 1-2
- pages
- 51 - 56
- publisher
- Springer
- external identifiers
-
- wos:000175634300007
- scopus:0141680637
- ISSN
- 0004-640X
- DOI
- 10.1023/A:1015587924410
- language
- English
- LU publication?
- yes
- id
- b2a15a85-da52-4c51-921b-233afe65ffe7 (old id 118558)
- date added to LUP
- 2016-04-04 11:36:20
- date last changed
- 2024-01-13 01:24:09
@article{b2a15a85-da52-4c51-921b-233afe65ffe7, abstract = {{We discuss the point spread function for the Spectro instrument based on realistic effects of the time delayed integration, transverse image motion and pixelization, but assuming rather small wave front errors. Stars brighter than 10 mag, which will saturate the CCD, may be observed photometrically using the image wings, but the central wavelengths will be slightly shifted towards the red.}}, author = {{Fabricius, C and Lindegren, Lennart}}, issn = {{0004-640X}}, language = {{eng}}, number = {{1-2}}, pages = {{51--56}}, publisher = {{Springer}}, series = {{Astrophysics and Space Science}}, title = {{The spectro point spread function for GAIA}}, url = {{http://dx.doi.org/10.1023/A:1015587924410}}, doi = {{10.1023/A:1015587924410}}, volume = {{280}}, year = {{2002}}, }