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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00003839naa a2200673 4500
001oai:DiVA.org:su-147007
003SwePub
008170929s2017 | |||||||||||000 ||eng|
0247 a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1470072 URI
0247 a https://doi.org/10.3847/1538-4357/aa81cc2 DOI
040 a (SwePub)su
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
1001 a Pirzkal, Norbert4 aut
2451 0a FIGS-Faint Infrared Grism Survey :b Description and Data Reduction
264 c 2017-09-01
264 1b American Astronomical Society,c 2017
338 a print2 rdacarrier
520 a The Faint Infrared Grism Survey (FIGS) is a deep Hubble Space Telescope (HST) WFC3/IR (Wide Field Camera 3 Infrared) slitless spectroscopic survey of four deep fields. Two fields are located in the Great Observatories Origins Deep Survey-North (GOODS-N) area and two fields are located in the Great Observatories Origins Deep Survey-South (GOODS-S) area. One of the southern fields selected is the Hubble Ultra Deep Field. Each of these four fields were observed using the WFC3/G102 grism (0.8 mu m-1.15 mu m continuous coverage) with a total exposure time of 40 orbits (approximate to 100 kilo-seconds) per field. This reaches a 3 sigma continuum depth of approximate to 26 AB magnitudes and probes emission lines to similar to 10(-17) erg s(-1) cm(-2). This paper details the four FIGS fields and the overall observational strategy of the project. A detailed description of the Simulation Based Extraction (SBE) method used to extract and combine over 10,000 spectra of over 2000 distinct sources brighter than m(F105W) = 26.5 mag is provided. High fidelity simulations of the observations is shown to significantly improve the background subtraction process, the spectral contamination estimates, and the final flux calibration. This allows for the combination of multiple spectra to produce a final high quality, deep, 1D spectra for each object in the survey.
650 7a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng
653 a galaxies: general
653 a surveys
653 a techniques: spectroscopic
7001 a Malhotra, Sangeeta4 aut
7001 a Ryan, Russell E.4 aut
7001 a Rothberg, Barry4 aut
7001 a Grogin, Norman4 aut
7001 a Finkelstein, Steven L.4 aut
7001 a Koekemoer, Anton M.4 aut
7001 a Rhoads, James4 aut
7001 a Larson, Rebecca L.4 aut
7001 a Christensen, Lise4 aut
7001 a Cimatti, Andrea4 aut
7001 a Ferreras, Ignacio4 aut
7001 a Gardner, Jonathan P.4 aut
7001 a Gronwall, Caryl4 aut
7001 a Hathi, Nimish P.4 aut
7001 a Hibon, Pascale4 aut
7001 a Joshi, Bhavin4 aut
7001 a Kuntschner, Harald4 aut
7001 a Meurer, Gerhardt R.4 aut
7001 a O'Connell, Robert W.4 aut
7001 a Östlin, Göranu Stockholms universitet,Institutionen för astronomi4 aut0 (Swepub:su)ostlin
7001 a Pasquali, Anna4 aut
7001 a Pharo, John4 aut
7001 a Straughn, Amber N.4 aut
7001 a Walsh, Jeremy R.4 aut
7001 a Watson, Darach4 aut
7001 a Windhorst, Rogier A.4 aut
7001 a Zakamska, Nadia L.4 aut
7001 a Zirm, Andrew4 aut
7102 a Stockholms universitetb Institutionen för astronomi4 org
7730 t Astrophysical Journald : American Astronomical Societyg 846:1q 846:1x 0004-637Xx 1538-4357
8564 u https://repository.arizona.edu/bitstream/10150/625750/1/Pirzkal_2017_ApJ_846_84.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-147007
8564 8u https://doi.org/10.3847/1538-4357/aa81cc

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