J/ApJS/263/27           CLAMATO DR2 redshift catalog           (Horowitz+, 2022)

Second Data Release of the COSMOS Lyα Mapping and Tomography Observations: the first 3D maps of the detailed cosmic web at 2.05<z<2.55. Horowitz B., Lee K.-G., Ata M., Muller T., Krolewski A., Prochaska J.X., Hennawi J.F., White M., Schlegel D., Rich R.M., Nugent P.E., Suzuki N., Kashino D., Koekemoer A.M., Lemaux B.C. <Astrophys. J. Suppl. Ser., 263, 27 (2022)> =2022ApJS..263...27H 2022ApJS..263...27H
ADC_Keywords: Intergalactic medium; Galaxies, spectra; QSOs; Redshifts; Optical; Surveys Keywords: Intergalactic medium ; Extragalactic astronomy ; Intergalactic filaments ; Intergalactic gas ; Voids ; High-redshift galaxy clusters ; Galaxy clusters ; Lyman alpha forest ; Spectroscopy ; Redshift surveys ; Surveys ; Hubble Space Telescope Abstract: We present the second data release of the COSMOS Lyα Mapping And Tomography Observations Survey conducted with the Low Resolution Imaging Spectrometer on the Keck I telescope. This project used Lyα forest absorption in the spectra of faint star-forming galaxies and quasars at z∼2-3 to trace neutral hydrogen in the intergalactic medium. In particular, we use 320 objects over a footprint of ∼0.2deg2 to reconstruct the absorption field at 2.05<z<2.55 at ∼2h-1Mpc resolution. We apply a Wiener filtering technique to the observed data to reconstruct three-dimensional (3D) maps of the field over a volume of 4.1x105h-3Mpc3. In addition to the filtered flux maps, for the first time we infer the underlying dark matter field through a forward-modeling framework from a joint likelihood of galaxy and Lyα forest data, finding clear examples of the detailed cosmic web consisting of cosmic voids, sheets, filaments, and nodes. In addition to traditional figures, we present a number of interactive 3D models to allow exploration of the data and qualitative comparisons to known galaxy surveys. We find that our inferred overdensities are consistent with those found from galaxy fields. We will make all our reduced spectra, extracted Lyα forest pixel data, and reconstructed tomographic maps publicly available upon publication. Description: The COSMOS Lyα Mapping And Tomography Observations (CLAMATO) survey observations were carried out using the Low Resolution Imaging Spectrometer (LRIS) spectrograph on the Keck I telescope at Maunakea, Hawai'i. The observations described in this paper were carried out in 2014-2020 via a total time allocation of 20.5 nights. CLAMATO focused on the LRIS blue channel covering the range of 3700Å<λ<4400Å (R∼1100), which corresponds to the rest frame Lyα at 2.1≲zα≲2.6. From the 32 unique slit-masks observed in the 2014-2020 CLAMATO campaign, we reduced and extracted 600 spectra from the blue channel. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 103 600 The COSMOS Lyα Mapping And Tomography Observations (CLAMATO) Data Release 2 redshift catalog sp/* . 619 Indiviual reduced spectra from LRIS-Blue in FITS format -------------------------------------------------------------------------------- See also: II/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007) J/ApJS/172/70 : zCOSMOS-bright catalog (Lilly+, 2007) J/ApJ/675/49 : High-redshift QSOs in the SWIRE survey (Siana+, 2008) J/ApJ/690/1236 : COSMOS photometric redshift catalog (Ilbert+, 2009) J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016) J/ApJS/225/27 : 3D-HST Survey: grism spectra master catalog (Momcheva+, 2016) J/ApJ/828/21 : ZFIRE v1.0 data release (Nanayakkara+, 2016) J/ApJ/861/60 : z∼2.3 cosmic voids in the COSMOS field (Krolewski+, 2018) J/ApJS/237/31 : CLAMATO DR1: 3D Lyα forest tomography (Lee+, 2018) J/AJ/160/37 : IGM opacity from Lyman-break galaxies (Monzon+, 2020) http://zenodo.org/record/7524313 : Data products for CLAMATO DR2 Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 30 A30 --- FileName Name of the FITS file in subdirectory "sp" (1) 32- 38 I7 --- Seq [403/34729] CLAMATO ID number (<[LKW2018] NNNNN> in Simbad) 40- 44 F5.2 mag gmag [20.12/25.3] Subaru g+ AB magnitude (2) 46- 49 F4.1 --- q_zspec [-3/4] Redshift confidence grade (4=very secure, 3=secure, 2=probable, 1=insecure, 0=unidentified spectrum) (3) 51- 55 F5.3 --- zspec [0/3.52] Spectroscopic redshift as determined from CLAMATO spectrum 57 I1 --- QSO [0/1] QSO flag (1 if QSO (19 occurrences); 0 if non-QSO) 59- 67 F9.5 deg RAdeg [149.4/150.5] Right Ascension (J2000) (2) 69- 75 F7.5 deg DEdeg [1.7/2.5] Declination (J2000) (2) 77- 80 F4.1 --- SN1 [0/35.7]?=-9 Estimated (median) Lyα-forest S/N at 2.05<z<2.15 82- 85 F4.1 --- SN2 [0/42.2]?=-9 Estimated (median) Lyα-forest S/N at 2.15<z<2.35 87- 90 F4.1 --- SN3 [0/49.2]?=-9 Estimated (median) Lyα-forest S/N at 2.35<z<2.55 92- 95 F4.1 --- SNRed [-0.3/64.6]?=-9 Estimated S/N over restframe 1250Å-1350Å 97 I1 --- Tomo [0/1] Flag on whether sightline was used in tomographic map (0 for no, 1 for yes) 99- 103 I5 s Texp [7200/53100] Exposure time on the spectrum, in seconds (aggregate) -------------------------------------------------------------------------------- Note (1): Spectrum filename as given in the spec_v0.tar.gz archive on Zenodo: doi:10.5281/zenodo.5842842 (v2 on doi:10.5281/zenodo.7524313). Note (2): Source positions and magnitudes from Capak+ 2007, II/284 Note (3): Redshift confidence grade, similar to that described in Lilly+ 2007, J/ApJS/172/70 but without fractional grades. See also Lee+ 2018, J/ApJS/237/31 (CLAMATO DR1). -------------------------------------------------------------------------------- History: From electronic version of the journal for Table 1. Reduced spectra downloaded at: http://zenodo.org/record/7524313 References: Lee et al. DR1. 2018ApJS..237...31L 2018ApJS..237...31L Cat. J/ApJS/237/31
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 27-Jan-2023
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