J/PASJ/57/881   Imaging of high-redshift Lyman alpha emitters  (Yamada+, 2005)

An intermediate-band imaging survey for high-redshift Lyman alpha emitters: the Mahoroba-11. Yamada S.F., Sasaki S.S., Sumiya R., Umeda K., Shioya Y., Ajiki M., Nagao T., Murayama T., Taniguchi Y. <Publ. Astron. Soc. Jap., 57, 881-903 (2005)> =2005PASJ...57..881Y 2005PASJ...57..881Y
ADC_Keywords: Surveys ; Photometry, UBVRI ; Photometry, Cousins Keywords: cosmology: early universe - cosmology: observations - galaxies: evolution - galaxies: formation Abstract: We present results of our intermediate-band optical imaging survey for high-z Lyα emitters (LAEs) using the prime focus camera, Suprime-Cam, on the 8.2m Subaru telescope. In our survey, we used eleven filters: four broad-band filters (B, RC, i', and z') and seven intermediate-band filters covering from 500nm to 720nm. We call this imaging program the Mahoroba-11. The seven intermediate-band filters were selected from a series of IA filters, which is the Suprime-Cam intermediate-band filter system, whose spectral resolution is R=23. Our survey was made in a 34'x27' sky area in the Subaru XMM-Newton Deep Survey Field. We found 409 IA-excess objects, which provided us with a large photometric sample of strong emission-line objects. Applying the photometric redshift method to this sample, we obtained a new sample of 198 LAE candidates at 3<z<5. We found no evidence for evolutions of the number density and the star-formation rate density (SFRD) for LAEs with logL(Lyα)(erg/s)>42.67 between z∼3 and z∼5. Description: Deep and wide-field B-, RC-, i'-, and z'-band imaging data of a southward 30'x24' area in the Subaru/XMM-Newton Deep Survey Field (the SXDS field) centered at RA=02:18:00, DE=-05:12:00 (J2000.0) were obtained using the Suprime-Cam on the 8.2m Subaru telescope during a period between 2000 August and 2002 January by the SXDS team. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 79 11 Journal of observations table3.dat 90 198 Catalog of LAE (Lyα emitter) candidates table4.dat 69 198 Properties of LAE candidates -------------------------------------------------------------------------------- See also: J/A+A/431/793 : Ly-alpha emitters around MRC 0316-257 (Venemans+, 2005) J/PASJ/57/165 : SDF : Ly-alpha emitters (Taniguchi+, 2005) B/subaru : Log of Subaru Prime Focus Camera Exposures (ADAC NAOJ, 2006) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- Filter Filter name 7- 10 I4 0.1nm lambdac Central wavelength of the filter band 12- 15 I4 0.1nm FWHM FWHM of the filter band 17- 68 A52 --- Obs Observation dates 70- 74 I5 s IntTime Total integration time 76- 79 F4.1 mag magLim Limiting magnitude (in AB mag) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- [YSS2005] Object designation, IANNN NNNNNN (G1) 14- 18 F5.2 arcmin DRA Offset in right ascension (2) 20- 24 F5.2 arcmin DDE Offset in declination (2) 26 A1 --- l_Bmag Limit flag on Bmag 27- 30 F4.1 mag Bmag B (436.4±100.8nm) magnitude (3) 32 A1 --- l_Rcmag Limit flag on Rcmag 33- 36 F4.1 mag Rcmag Cousins R (641.0±157.6nm) magnitude (3) 38 A1 --- l_i'mag Limit flag on i'mag 39- 42 F4.1 mag i'mag i' (758.9±153.5nm) magnitude (3) 44 A1 --- l_z'mag Limit flag on z'mag 45- 48 F4.1 mag z'mag z' (902.4±140.9nm) magnitude (3) 50 A1 --- l_IA527mag Limit flag on IA527mag 51- 54 F4.1 mag IA527mag IA527 (527.2±24.2nm) magnitude (3) 56 A1 --- l_IA574mag Limit flag on IA574mag 57- 60 F4.1 mag IA574mag IA574 (574.3±27.1nm) magnitude (3) 62 A1 --- l_IA598mag Limit flag on IA598mag 63- 66 F4.1 mag IA598mag IA598 (600.0±29.4nm) magnitude (3) 68 A1 --- l_IA624mag Limit flag on IA624mag 69- 72 F4.1 mag IA624mag IA624 (622.6±29.9nm) magnitude (3) 74 A1 --- l_IA651mag Limit flag on IA651mag 75- 78 F4.1 mag IA651mag IA651 (650.2±32.2nm) magnitude (3) 80 A1 --- l_IA679mag Limit flag on IA679mag 81- 84 F4.1 mag IA679mag IA679 (678.8±33.6nm) magnitude (3) 86 A1 --- l_IA709mag Limit flag on IA709mag 87- 90 F4.1 mag IA709mag IA709 (708.2±31.8nm) magnitude (3) -------------------------------------------------------------------------------- Note (2): Offset from RA=02:18:00, DE=-05:12:00 (J2000.0). Note (3): AB magnitude in a 2" diameter; the filter characteristics are detailed in table1.dat -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- [YSS2005] Object designation, IANNN NNNNNN (G1) 14- 19 F6.1 0.1nm EWobs Observed equivalent width of Lyα line 21- 26 F6.1 0.1nm EWrest Rest-frame equivalent width 28- 35 E8.3 mW/m2 F(Lya) Lyα flux 37- 44 E8.3 10-7W L(Lya) Lyα luminosity 46- 53 E8.3 10-7W/Hz L(UV) Monochromatic UV luminosity 55- 59 F5.1 mag MUV Absolute UV magnitude 61- 64 F4.1 solMass/yr SFR(Lya) Lyα star formation rate 66- 69 F4.1 solMass/yr SFR(UV) UV star formation rate -------------------------------------------------------------------------------- Global notes: Note (G1): Object are designated as IANNN NNNNN, where IANNN is the name of the IA filter, and NNNNNN a sequential number for the corresponding IANNN image. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 29-Jun-2006
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