J/ApJ/736/18   Lyman-continuum emission at z∼3 in SSA22 field   (Nestor+, 2011)

Narrowband imaging of escaping Lyman-continuum emission in the SSA22 field. Nestor D.B., Shapley A.E., Steidel C.C., Siana B. <Astrophys. J., 736, 18 (2011)> =2011ApJ...736...18N 2011ApJ...736...18N
ADC_Keywords: Galaxies, optical ; Redshifts ; Surveys ; Photometry ; Ultraviolet Keywords: cosmology: observations - diffuse radiation - galaxies: high-redshift - intergalactic medium Abstract: We present the results of an ultradeep, narrowband imaging survey for Lyman-continuum (LyC) emission at z∼3 in the SSA22a field. We employ a custom narrowband filter centered at λ=3640Å (NB3640), which probes the LyC region for galaxies at z≥3.06. We also analyze new and archival NB4980 imaging tuned to the wavelength of the Lyα emission line at z=3.09, and archival broadband B, V, and R images of the non-ionizing UV continuum. Our NB3640 images contain 26 z≥3.06 Lyman break galaxies (LBGs) as well as a set of 130 Lyα emitters (LAEs), identified by their excess NB4980 flux relative to the BV continuum. Six LBGs and 28 LAEs are detected in the NB3640 image. LBGs appear to span a range of NB3640-R colors, while LAEs appear bimodal in their NB3640-R properties. We estimate average UV-to-LyC flux density ratios. Description: The NB3640 imaging data were collected,using the blue side of the Keck Low Resolution Imaging Spectrometer (LRIS), on 2005 August 6-7 and 2008 June 2-4 (UT). During the 2005 August run, the red side of LRIS was simultaneously used to collect NB4980 data. The pointing center of the LRIS imaging field was RA(J2000)=22:17:28.8, DE(J2000)=+00:14:36, and the area of the final trimmed stacks is 5.5'x7.6'. Narrowband images were calibrated onto the AB system and were also corrected for a Galactic extinction of E(B-V)=0.08. We augmented the LRIS data set with both narrowband and broadband archival imaging data taken with Suprime-Cam on the Subaru Telescope. Broadband B- and V-band images were obtained on 2003 September 21 (UT; PI: Hu). We constructed a BV continuum image by first smoothing the V-band image so that the B and V image point-spread functions (PSFs) were matched, and then scaling the PSF-matched images to the same zeropoint. We then executed: BV=0.44B+0.56V, with the weights determined by the relative wavelengths of the broadband and NB4980 filters. Finally, for detailed rest-frame UV (non-ionizing) continuum morphologies of our SSA22a targets, we assembled archival Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) imaging of the field, taken with the F814W filter. See section 2 for further explanations. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4.dat 79 6 Photometry for LBGs (Lyman Break galaxies) with NB3640 Detections table5.dat 85 28 Photometry for LAEs (Lyman Alpha Eimitters) with NB3640 Detections table9.dat 67 20 Photometry for LBGs without NB3640 Detections table10.dat 72 102 Photometry for LAEs without NB3640 Detections -------------------------------------------------------------------------------- See also: B/hst : HST Archived Exposures Catalog (STScI, 2007) J/MNRAS/401/1521 : Stellar masses of LBGs at z∼3 (Magdis+, 2010) J/A+A/498/13 : Lyman-α emitters from redshifts z∼2-3 (Nilsson+, 2009) J/ApJ/705/639 : Sizes of Lyman alpha emitters at z=3.1 (Bond+, 2009) J/ApJ/592/728 : Lyman break galaxies at redshift z∼3 (Steidel+, 2003) J/PASJ/53/653 : SSA 22 field NIR imaging (Tamura+, 2001) J/ApJ/519/1 : Lyman-break galaxies at z ≳ 4 (Steidel+, 1999) Byte-by-byte Description of file: table[49].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- ID Source identification 10- 11 I2 h RAh [22] Hour of right ascension (J2000) 13- 14 I2 min RAm [17] Minute of right ascension (J2000) 16- 20 F5.2 s RAs Second of right ascension (J2000) 22 A1 --- DE- [+] Sign of declination (J2000) 23 I1 deg DEd [0] Degree of declination (J2000) 25- 26 I2 arcmin DEm Arcminute of declination (J2000) 28- 31 F4.1 arcsec DEs Arcsecond of declination (J2000) 33- 38 F6.4 --- zem [3.07/3.30]? Lyα emission redshift 40- 45 F6.4 --- zabs [3.06/3.29]? Interstellar absorption redshift 47- 51 F5.2 mag Rmag [23.49/25.2] R-band AB magnitude 53- 57 F5.2 mag [3640] ? Narrow-band 3640 magnitude (only for table 4) 59- 61 F3.1 arcsec delR ? Spatial offset between the centroids of R-band and NB3640 emission (only for table 4) 63 A1 --- l_FUV/Fo Limit flag on FUV/Fo 64- 67 F4.1 --- FUV/Fo [1.4/29.2] Observed ratio in non-ionizing UV and LyC emission (G1) 69- 71 F3.1 --- e_FUV/Fo ? FUV/Fo uncertainty 73- 75 F3.1 --- FUV/Fc ? Ratio of non-ionizing UV continuum and LyC emission (only for table 4) (G2) 77- 79 F3.1 --- e_FUV/Fc ? FUV/Fc uncertainty -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat table10.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Seq Source number (003-118 for table 5; 001-130 for table 10) 4 A1 --- f_Seq [c-i] Individual notes (1) 6- 7 I2 h RAh [22] Hour of right ascension (J2000) 9- 10 I2 min RAm [17] Minute of right ascension (J2000) 12- 16 F5.2 s RAs Second of right ascension (J2000) 18 A1 --- DE- [+] Sign of declination (J2000) 19 I1 deg DEd [0] Degree of declination (J2000) 21- 22 I2 arcmin DEm Arcminute of declination (J2000) 24- 27 F4.1 arcsec DEs Arcsecond of declination (J2000) 29- 33 F5.2 mag [4980] [23/26.49] Keck/LRIS NB4980 magnitude 35 A1 --- l_BV-4980 Limit flag on BV-4980 36- 39 F4.2 mag BV-4980 [0.71/2.68] BV-NB4980 color index 41 A1 --- l_EW0 Limit flag on EW0 42- 44 I3 0.1nm EW0 [19/400] Lyα rest equivalent width estimated from BV-NB4980 color index 46 A1 --- l_Rmag Limit flag on Rmag 47- 51 F5.2 mag Rmag [23.92/27] R-band AB magnitude 53- 57 F5.2 mag [3640] ? Narrow-band 3640 magnitude (only for table 5) 59- 61 F3.1 arcsec delR ? Spatial offset between the centroids of R and NB3640 emission (only for table 5) 62 A1 --- f_delR [e] e: offset determined from the centroid of BV detection 64- 66 F3.1 arcsec delLya ? Spatial offset between the centroids of Lyα and NB3640 emission (only for table 5) 68 A1 --- l_FUV/Fo Limit flag on FUV/Fo 69- 72 F4.1 --- FUV/Fo [0.5/22.4]? Observed ratio in non-ionizing UV and LyC emission (G1) 74- 76 F3.1 --- e_FUV/Fo ? FUV/Fo uncertainty 78 A1 --- l_FUV/Fc Limit flag on FUV/Fc 79- 81 F3.1 --- FUV/Fc ? Ratio of non-ionizing UV continuum and LyC emission (G2) 83- 85 F3.1 --- e_FUV/Fc ? FUV/Fc uncertainty -------------------------------------------------------------------------------- Note (1): Flag as follows: c = LBG D3 (<SAS-LBG SSA22a-D3> in Simbad), zem=3.086. d = LBG C4 (<SAS-LBG SSA22a-C4> in Simbad), zem=3.076. e = LBG MD23 (<SAS-LBG SSA22a-MD23> in Simbad), zem=3.092. f = LBG C28 (<SAS-LBG SSA22a-C28> in Simbad), zem=3.076. g = LBG candidate C9 (<SAS-LBG SSA22a-C9> in Simbad). h = LBG M28 (<SAS-LBG SSA22a-M28> in Simbad), zem=3.094. i = LBG candidate M13 (<SAS-LBG SSA22a-M13> in Simbad). -------------------------------------------------------------------------------- Global notes: Note (G1): Observed ratio in non-ionizing UV and LyC emission; inferred from the NB3640-R color (for tables 4 and 5). This value has not been corrected for either contamination by foreground sources or IGM absorption. Note (G2): Corrected for both foreground contamination and IGM absorption. -------------------------------------------------------------------------------- Nomenclature notes: In tables 4 and 9, IDs come from Steidel et al., 2003, Cat. J/ApJ/592/728, <SAS-LBG SSA22a-AANN> or <SAS-LBG SSA22a-aug96AANN> in Simbad. History: From electronic version of the journal
(End) Emmanuelle Perret [CDS] 06-Dec-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line