Updating SPIE references

GalagaBits · May 8, 2024 · 3f21e29 · 3f21e29
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Showing 1 changed file with 27 additions and 26 deletions.
diff --git a/paper/paper.bib b/paper/paper.bib
@@ -17,34 +17,35 @@ @article{gardner_james_2023
 	file = {Full Text PDF:/Users/galagabits/Zotero/storage/67WUHZBJ/Gardner et al. - 2023 - The James Webb Space Telescope Mission.pdf:application/pdf},
 }
 
-@article{doyon_jwst_2012,
-	title = {The {JWST} {Fine} {Guidance} {Sensor} ({FGS}) and {Near}-{Infrared} {Imager} and {Slitless} {Spectrograph} ({NIRISS})},
-	volume = {8442},
-	url = {https://ui.adsabs.harvard.edu/abs/2012SPIE.8442E..2RD},
-	doi = {10.1117/12.926578},
-	abstract = {The Fine Guidance Sensor (FGS) is one of the four science instruments on board the James Webb Space Telescope (JWST). FGS features two modules: an infrared camera dedicated to fine guiding of the observatory and a science camera module, the Near-Infrared Imager and Slitless Spectrograph (NIRISS) covering the wavelength range between 0.7 and 5.0 μm with a field of view of 2.2' X 2.2'. NIRISS has four observing modes: 1) broadband imaging featuring seven of the eight NIRCam broadband filters, 2) wide-field slitless spectroscopy at a resolving power of rv150 between 1 and 2.5 μm, 3) single-object cross-dispersed slitless spectroscopy enabling simultaneous wavelength coverage between 0. 7 and 2.5 μm at Rrv660, a mode optimized for transit spectroscopy of relatively bright (J {\textgreater} 7) stars and, 4) sparse aperture interferometric imaging between 3.8 and 4.8 μm enabling high contrast ("' 10-4) imaging of M {\textless} 8 point sources at angular separations between 70 and 500 milliarcsec. This paper presents an overview of the FGS/NIRISS design with a focus on the scientific capabilities and performance offered by NIRISS.},
-	urldate = {2023-11-14},
-	author = {Doyon, René and Hutchings, John B. and Beaulieu, Mathilde and Albert, Loic and Lafrenière, David and Willott, Chris and Touahri, Driss and Rowlands, Neil and Maszkiewicz, Micheal and Fullerton, Alex W. and Volk, Kevin and Martel, André R. and Chayer, Pierre and Sivaramakrishnan, Anand and Abraham, Roberto and Ferrarese, Laura and Jayawardhana, Ray and Johnstone, Doug and Meyer, Michael and Pipher, Judith L. and Sawicki, Marcin},
-	month = sep,
-	year = {2012},
-	note = {Conference Name: Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave
-ADS Bibcode: 2012SPIE.8442E..2RD},
-	pages = {84422R},
+@INPROCEEDINGS{doyon_jwst_2012,
+       author = {{Doyon}, Ren{\'e} and {Hutchings}, John B. and {Beaulieu}, Mathilde and {Albert}, Loic and {Lafreni{\`e}re}, David and {Willott}, Chris and {Touahri}, Driss and {Rowlands}, Neil and {Maszkiewicz}, Micheal and {Fullerton}, Alex W. and {Volk}, Kevin and {Martel}, Andr{\'e} R. and {Chayer}, Pierre and {Sivaramakrishnan}, Anand and {Abraham}, Roberto and {Ferrarese}, Laura and {Jayawardhana}, Ray and {Johnstone}, Doug and {Meyer}, Michael and {Pipher}, Judith L. and {Sawicki}, Marcin},
+        title = "{The JWST Fine Guidance Sensor (FGS) and Near-Infrared Imager and Slitless Spectrograph (NIRISS)}",
+    booktitle = {Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave},
+         year = 2012,
+       editor = {{Clampin}, Mark C. and {Fazio}, Giovanni G. and {MacEwen}, Howard A. and {Oschmann}, Jacobus M., Jr.},
+       series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
+       volume = {8442},
+        month = sep,
+          eid = {84422R},
+        pages = {84422R},
+          doi = {10.1117/12.926578},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2012SPIE.8442E..2RD},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
 }
 
-@article{marston_overview_2018,
-	title = {Overview of the {Mikulski} {Archive} for space telescopes for the {James} {Webb} {Space} {Telescope} data archiving},
-	volume = {10704},
-	url = {https://ui.adsabs.harvard.edu/abs/2018SPIE10704E..13M},
-	doi = {10.1117/12.2311973},
-	abstract = {In this paper we present the envisaged setup and changes to the current Mikulski Archive for Space Telescopes (MAST) configuration at the beginning of operations for the James Webb Space Telescope mission. The placing of the observatory at L2 and long periods of autonomous operations mean that observations can be split over several time periods or `visits'. Data are processed through standard science data reduction pipelines after arriving at the Space Telescope Science Institute (STScI). We describe how data from visits and pipeline processing lead to the data products that are to be stored in the archives. Most observations will require a number of exposures; we discuss the data associations that will formulate the highest level of pipeline products that will be available in the MAST archive for JWST. The JWST observatory has numerous spectroscopic modes, including integral field units and multiple object spectra which will distinguish it from the Hubble Space Telescope archive. We describe the expected data products and services. Finally, we discuss the links to data analysis software and archive products available for user reprocessing.},
-	urldate = {2023-11-14},
-	author = {Marston, A. and Hargis, J. and Levay, K. and Forshay, P. and Mullally, S. and Shaw, R.},
-	month = jul,
-	year = {2018},
-	note = {Conference Name: Observatory Operations: Strategies, Processes, and Systems VII
-ADS Bibcode: 2018SPIE10704E..13M},
-	pages = {1070413},
+@INPROCEEDINGS{marston_overview_2018,
+       author = {{Marston}, A. and {Hargis}, J. and {Levay}, K. and {Forshay}, P. and {Mullally}, S. and {Shaw}, R.},
+        title = "{Overview of the Mikulski Archive for space telescopes for the James Webb Space Telescope data archiving}",
+    booktitle = {Observatory Operations: Strategies, Processes, and Systems VII},
+         year = 2018,
+       series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
+       volume = {10704},
+        month = jul,
+          eid = {1070413},
+        pages = {1070413},
+          doi = {10.1117/12.2311973},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2018SPIE10704E..13M},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
 }
 
 @article{scargle_studies_1982,