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J/ApJ/696/785         Global SFR density over 0.7<z<1.9            (Shim+, 2009)

Global star formation rate density over 0.7<z<1.9. Shim H., Colbert J., Teplitz H., Henry A., Malkan M., McCarthy P., Yan L. <Astrophys. J., 696, 785-796 (2009)> =2009ApJ...696..785S
ADC_Keywords: Galaxies, spectra ; Redshifts ; Photometry, HST ; Infrared sources Keywords: galaxies: evolution - galaxies: high-redshift - galaxies: luminosity function, mass function - galaxies: starburst Abstract: We determine the global star formation rate (SFR) density at 0.7<z<1.9 using emission-line-selected galaxies identified in Hubble Space Telescope-Near Infrared Camera and Multi-Object Spectrograph (HST-NICMOS) grism spectroscopy observations. Observing in a pure parallel mode throughout HST Cycles 12 and 13, our survey covers ∼104arcmin2 from which we select 80 galaxies with likely redshifted Hα emission lines. In several cases, a somewhat weaker [OIII] doublet emission is also detected. Description: All of the data presented in this study have been obtained using camera 3 of NICMOS onboard HST, taken in the pure parallel mode with the G141 grism and the broadband F110W/F160W filters, between 2003 October and 2004 July (Cycle 12), 2004 July and 2005 January (Cycle 13). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 87 80 Emission-line objects from the NICMOS grism survey
See also: J/ApJ/677/169 : Hα galaxies at z=0.84 (Villar+, 2008) J/ApJS/175/128 : Hα emitting galaxies in COSMOS-2 field (Shioya+, 2008) J/AJ/127/2002 : Star Formation Rate of NFGS galaxies (Kewley+, 2004) J/ApJS/146/209 : STIS emission-line galaxies observations (Teplitz+, 2003) J/ApJ/549/820 : Hα flux of ACCG 114 galaxies (Couch+, 2001) J/A+A/379/798 : ELAIS Hα emitting galaxies (Pascual+, 2001) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 20 A20 --- [SCT2009] Object name (1) 22 A1 --- f_[SCT2009] [e] Near-edge objects (2) 24- 25 I2 h RAh Hour of right ascension (J2000) 27- 28 I2 min RAm Minute of right ascension (J2000) 30- 34 F5.2 s RAs Second of right ascension (J2000) 36 A1 --- DE- Declination sign (J2000) 37- 38 I2 deg DEd Degree of declination (J2000) 40- 41 I2 arcmin DEm Arcminute of declination (J2000) 43- 46 F4.1 arcsec DEs Arcsecond of declination (J2000) 48- 52 F5.3 --- z Spectroscopic redshift (3) 54- 59 F6.3 10-19W/m2 FHa Hα emission line flux (4) 61- 63 I3 0.1nm Wave Observed wavelength 65- 69 F5.2 mag F110W ? HST/NICMOS F110W AB magnitude (J-band) (5) 71- 75 F5.2 mag F160W ? HST/NICMOS F160W AB magnitude (H-band) (5) 77- 81 F5.2 [10-7W] logLHa Log of Hα luminosity (6) 83- 87 F5.1 Msun/yr SFR Star formation rate (6)
Note (1): We assign the suffix a, b, or c to identify different objects in one field. Note (2): 'e' indicates objects that do not have either F110W/F160W photometry are objects lying near the image edge. Due to the locations, we could not find these objects in the direct image despite of clear emission lines (not thought to be zero order) for these galaxies. All galaxies without F110W photometry do not have the corresponding F110W images, i.e., there is no F110W-dropouts or galaxies with very red (F110W-F160W) colors. Note (3): In general there is a systematic redshift determination error of Δz∼0.03. Also, there are a few cases where the emission-line object lies near the edge of the image. In these cases, the counterpart of the object is not found in the associated direct image, which causes a large uncertainty in wavelength calibration up to ∼0.1um. The redshift uncertainty for an object lying at the image edge is Δz∼0.15. Note (4): Since the [NII] and Hα lines are not resolved in the resolution of NICMOS grism, FHa represents f(Hα+[NII]). Expressed in 10-16erg/cm2/s. Note (5): F110W/F160W magnitudes are in AB magnitudes, MAG_AUTO from SExtractor (total magnitudes of the galaxies). The conversion between AB and Vega magnitudes are F110WVega=F110WAB-0.73; F160WVega=F160WAB-1.31 (derived using NICMOS zeropoints in Vega magnitude system at Note (6): Hα luminosity and the derived star formation rate are corrected for possible [NII] contamination in the measured Hα line flux: f(Hα)=0.71*f(Hα+[NII]).
History: From electronic version of the journal
(End) Emmanuelle Perret [CDS] 06-May-2011
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

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