TY - JOUR
T1 - Discovery of a z = 7.452 High Equivalent Width Lyα Emitter from the Hubble Space Telescope Faint Infrared Grism Survey
AU - Figs Team, The
AU - Larson, Rebecca L.
AU - Finkelstein, Steven L.
AU - Pirzkal, Norbert
AU - Ryan, Russell
AU - Tilvi, Vithal
AU - Malhotra, Sangeeta
AU - Rhoads, James
AU - Finkelstein, Keely
AU - Jung, Intae
AU - Christensen, Lise
AU - Cimatti, Andrea
AU - Ferreras, Ignacio
AU - Grogin, Norman
AU - Koekemoer, Anton M.
AU - Hathi, Nimish
AU - O'Connell, Robert
AU - Östlin, Göran
AU - Pasquali, Anna
AU - Pharo, John
AU - Rothberg, Barry
AU - Windhorst, Rogier
N1 - Funding Information:
This work is based on observations made with the NASA/ ESA Hubble Space Telescope, obtained [from the Data Archive] at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program #13779. Processing of this data was done using the Texas Advanced Computing Center (TACC). R.L. and S.F. acknowledge support provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. R.L. also acknowledges support from the National Science Foundation through the MPS-GRSV program under grant number 1707552. I.J. acknowledges support from the NASA Headquarters under the NASA Earth and Space Science Fellowship Program—Grant 80NSSC17K0532. A.C. acknowledges the grants ASI n.I/023/12/0 “Attivitá relative alla fase B2/C per la missione Euclid” and PRIN MIUR 2015 “Cosmology and Fundamental Physics: Illuminating the Dark Universe with Euclid.” L.C. is supported by grant ID DFF-4090-00079. This work was supported by grants HST GO-13779.* from STScI, which is operated by AURA for NASA under contract NAS 5-26555. R.A.W. acknowledges support from NASA JWST Interdisciplinary Scientist grants NAG5-12460 and NNX14AN10G from GSFC. Facilities: HST, Spitzer. Software: IDL, Python, EAZY, BPZ, SourceExtractor.
Publisher Copyright:
© 2018. The American Astronomical Society. All rights reserved.
PY - 2018/5/10
Y1 - 2018/5/10
N2 - We present the results of an unbiased search for Lyα emission from continuum-selected 5.6 < z < 8.7 galaxies. Our data set consists of 160 orbits of G102 slitless grism spectroscopy obtained with the Hubble Space Telescope(HST)/WFC3 as part of the Faint Infrared Grism Survey (FIGS; PI: Malhotra), which obtains deep slitless spectra of all sources in four fields, and was designed to minimize contamination in observations of previously identified high-redshift galaxy candidates. The FIGS data can potentially spectroscopically confirm the redshifts of galaxies, and as Lyα emission is resonantly scattered by neutral gas, FIGS can also constrain the ionization state of the intergalactic medium during the epoch of reionization. These data have sufficient depth to detect Lyα emission in this epoch, as Tilvi et al. have published the FIGS detection of previously known Lyα emission at z = 7.51. The FIGS data use five separate roll angles of HST to mitigate the contamination by nearby galaxies. We created a method that accounts for and removes the contamination from surrounding galaxies and also removes any dispersed continuum light from each individual spectrum. We searched for significant (>4σ) emission lines using two different automated detection methods, free of any visual inspection biases. Applying these methods on photometrically selected high-redshift candidates between 5.6 < z < 8.7, we find two emission lines, one previously published by Tilvi et al., (2016) and a new line at 1.028 μm, which we identify as Lyα at z = 7.452 ± 0.003. This newly spectroscopically confirmed galaxy has the highest Lyα rest-frame equivalent width (EWLyα) yet published at z > 7 (140.3 ± 19.0 -).
AB - We present the results of an unbiased search for Lyα emission from continuum-selected 5.6 < z < 8.7 galaxies. Our data set consists of 160 orbits of G102 slitless grism spectroscopy obtained with the Hubble Space Telescope(HST)/WFC3 as part of the Faint Infrared Grism Survey (FIGS; PI: Malhotra), which obtains deep slitless spectra of all sources in four fields, and was designed to minimize contamination in observations of previously identified high-redshift galaxy candidates. The FIGS data can potentially spectroscopically confirm the redshifts of galaxies, and as Lyα emission is resonantly scattered by neutral gas, FIGS can also constrain the ionization state of the intergalactic medium during the epoch of reionization. These data have sufficient depth to detect Lyα emission in this epoch, as Tilvi et al. have published the FIGS detection of previously known Lyα emission at z = 7.51. The FIGS data use five separate roll angles of HST to mitigate the contamination by nearby galaxies. We created a method that accounts for and removes the contamination from surrounding galaxies and also removes any dispersed continuum light from each individual spectrum. We searched for significant (>4σ) emission lines using two different automated detection methods, free of any visual inspection biases. Applying these methods on photometrically selected high-redshift candidates between 5.6 < z < 8.7, we find two emission lines, one previously published by Tilvi et al., (2016) and a new line at 1.028 μm, which we identify as Lyα at z = 7.452 ± 0.003. This newly spectroscopically confirmed galaxy has the highest Lyα rest-frame equivalent width (EWLyα) yet published at z > 7 (140.3 ± 19.0 -).
KW - galaxies: distances and redshifts
KW - galaxies: high-redshift
KW - line: identification
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U2 - 10.3847/1538-4357/aab893
DO - 10.3847/1538-4357/aab893
M3 - Article
AN - SCOPUS:85047217550
SN - 0004-637X
VL - 858
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 94
ER -