J/ApJS/244/40    A3COSMOS. I. ALMA continuum photometry catalogs    (Liu+, 2019)

Automated mining of the ALMA archive in the COSMOS field (A3COSMOS). I. Robust ALMA continuum photometry catalogs and stellar mass and star formation properties for ∼700 galaxies at z=0.5-6. Liu D., Lang P., Magnelli B., Schinnerer E., Leslie S., Fudamoto Y., Bondi M., Groves B., Jimenez-Andrade E., Harrington K., Karim A., Oesch P.A., Sargent M., Vardoulaki E., Badescu T., Moser L., Bertoldi F., Battisti A., da Cunha E., Zavala J., Vaccari M., Davidzon I., Riechers D., Aravena M. <Astrophys. J. Suppl. Ser., 244, 40 (2019)> =2019ApJS..244...40L 2019ApJS..244...40L
ADC_Keywords: Galaxy catalogs; Photometry, millimetric/submm; Redshifts Keywords: galaxies: evolution ; galaxies: ISM ; galaxies: photometry ; galaxies: star formation ; submillimeter: galaxies ; techniques: photometric Abstract: The rich information on (sub)millimeter dust continuum emission from distant galaxies in the public Atacama Large Millimeter/submillimeter Array (ALMA) archive is contained in thousands of inhomogeneous observations from individual PI-led programs. To increase the usability of these data for studies deepening our understanding of galaxy evolution, we have developed automated mining pipelines for the ALMA archive in the COSMOS field (A3COSMOS) that efficiently exploit the available information for large numbers of galaxies across cosmic time and keep the data products in sync with the increasing public ALMA archive: (a) a dedicated ALMA continuum imaging pipeline, (b) two complementary photometry pipelines for both blind source extraction and prior source fitting, (c) a counterpart association pipeline utilizing the multiwavelength data available (including quality assessment based on machine-learning techniques), (d) an assessment of potential (sub)millimeter line contribution to the measured ALMA continuum, and (e) extensive simulations to provide statistical corrections to biases and uncertainties in the ALMA continuum measurements. Application of these tools yields photometry catalogs with ∼1000 (sub)millimeter detections (spurious fraction ∼8%-12%) from over 1500 individual ALMA continuum images. Combined with ancillary photometric and redshift catalogs and the above quality assessments, we provide robust information on redshift, stellar mass, and star formation rate for ∼700 galaxies at redshifts 0.5-6 in the COSMOS field (with undetermined selection function). The ALMA photometric measurements and galaxy properties are released publicly within our blind extraction, prior fitting, and galaxy property catalogs, plus the images. Description: The pointings of all public Atacama Large Millimeter/submillimeter Array (ALMA) data for the COSMOS field as of 2018 January 2 is shown in Figure 2, overlaid on the Herschel Space Observatory Photodetector Array Camera and Spectrometer (PACS) 100um image. The sum of the primary beam area of these observations reaches 164arcmin2. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file blind.dat 219 1134 The "blind"-extraction photometry catalog; all sources with S/N_peak>5.40 in the ALMA continuum data (see Section 2.2) prior.dat 251 1277 The "prior"-fitting photometry catalog; known sources in deep optical/near-infrared/radio catalogs which have S/N_peak>4.35 in the ALMA continuum data (see Section 2.4) catalog.dat 207 669 *A3COSMOS final galaxy catalog (see Section 4) fits/* . 1908 Continuum images in FITS format -------------------------------------------------------------------------------- Note on catalog.dat: The galaxy catalog contains only robustly detected galaxies with optical/near-infrared detections, so that each galaxy has a reasonably constrained, consistently fitted stellar mass, star formation rate and redshift. -------------------------------------------------------------------------------- Description of file: The three catalogs are available in their original FITS format on the FTP. See also: II/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007) VIII/103 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012) VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012) J/A+A/403/857 : VLA-VIRMOS Deep Field (Bondi+, 2003) J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003) J/ApJS/172/70 : zCOSMOS-bright catalog (Lilly+, 2007) J/AJ/136/2782 : Star formation efficiency in nearby galaxies (Leroy+, 2008) J/AJ/136/2563 : HI Nearby Galaxy Survey, THINGS (Walter+, 2008) J/ApJS/184/158 : Chandra COSMOS survey I. (Elvis+, 2009) J/ApJS/184/218 : The zCOSMOS 10k-bright spectroscopic sample (Lilly+, 2009) J/ApJS/188/384 : The VLA-COSMOS survey. IV. (Schinnerer+, 2010) J/MNRAS/415/3831 : AzTEC/ASTE source catalogue (Aretxaga+, 2011) J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011) J/MNRAS/411/102 : AzTEC/ASTE 1.1mm observations in the ADF-S (Hatsukade+ 2011) J/A+A/532/A90 : PACS Evolutionary Probe (PEP-DR1) catalogs (Lutz+, 2011) J/ApJ/742/61 : Phot. redshift of AGNs from XMM- and C-COSMOS (Salvato+ 2011) J/ApJ/761/140 : Spectroscopy of Herschel-SPIRE galaxies (Casey+, 2012) J/ApJS/201/30 : The Chandra COSMOS survey. III. (Civano+, 2012) J/A+A/544/A156 : UltraVISTA Catalogue Release DR1 (McCracken+, 2012) J/A+A/551/A100 : Panchromatic SED of Herschel sources (Berta+, 2013) J/A+A/556/A55 : Multi-color phot. of star-forming galaxies (Ilbert+, 2013) J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013) J/ApJ/768/74 : PHIBSS: CO obs. of star-forming galaxies (Tacconi+, 2013) J/MNRAS/441/1017 : Multiwavelength photometry of 34 galaxies (Rowlands+, 2014) J/ApJ/783/84 : ALMA obs. in 107 galaxies at z=0.2-2.5 (Scoville+, 2014) J/A+A/578/A11 : Spectrum of QSO XMMC 2028 (Brusa+, 2015) J/ApJ/812/43 : ALMA 870um obs. of HerMES galaxies (Bussmann+, 2015) J/ApJS/218/33 : Spitzer-CANDELS catalog within 5 deep fields (Ashby+, 2015) J/ApJS/219/8 : SFR for WISE + SDSS spectroscopic galaxies (Chang+, 2015) J/A+A/575/A40 : [OII] luminosity function (Comparat+, 2015) J/ApJ/806/110 : ALESS survey: SMGs in the ECDF-S data (da Cunha+, 2015) J/ApJS/220/12 : FMOS-COSMOS survey III. 0.7<z<2.5 galaxies (Silverman+, 2015) J/ApJ/819/62 : The COSMOS-Legacy Survey (CLS) catalog (Civano+, 2016) J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016) J/ApJ/817/34 : C-COSMOS Legacy sources multiwavelength cat. (Marchesi+, 2016) J/ApJ/828/21 : ZFIRE v1.0 data release (Nanayakkara+, 2016) J/ApJ/820/83 : ALMA galaxy data in the COSMOS survey field (Scoville+, 2016) J/ApJ/819/69 : [NII]205um emission in local luminous IR gal. (Zhao+, 2016) J/ApJ/830/51 : FourStar galaxy evolution survey (ZFOURGE) (Straatman+, 2016) J/ApJ/850/83 : DANCING-ALMA. I. submm/mm continuum sources (Fujimoto+, 2017) J/MNRAS/465/1789 : SCUBA-2 Cosmology Legacy Survey (Geach+, 2017) J/ApJ/841/111 : C3R2 survey: high-confidence z from DR1 (Masters+, 2017) J/ApJ/839/58 : ALMA submm galaxies multi-wavelength data (Simpson+, 2017) J/A+A/602/A1 : VLA-COSMOS 3 GHz Large Project (Smolcic+, 2017) J/A+A/600/A110 : VIMOS Ultra Deep Survey (VUDS) DR1 (Tasca+, 2017) J/ApJS/237/39 : Spitzer survey of UltraVISTA deep Stripes (Ashby+, 2018) J/ApJ/858/77 : DEIMOS 10K spectrosc. survey in COSMOS field (Hasinger+, 2018) J/ApJ/853/172 : "Super-deblended" dust emission in galaxies. I. (Liu+, 2018) J/A+A/625/A114 : Star-forming gal. over 0.35<z<2.25 (Jimenez-Andrade+, 2019) http://sites.google.com/view/a3cosmos/ : A3COSMOS home page Byte-by-byte Description of file: blind.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 F14.10 deg RAdeg Right ascension of the ALMA emission (J2000) 16- 27 F12.10 deg DEdeg Declination of the ALMA emission (J2000) 29- 35 F7.4 mJy Fluxc [0.04/52.4] The fitted total flux with Gaussian source models, corrected for flux bias and PBA (Totalfluxpbcor) 37- 42 F6.4 mJy e_Fluxc [0.01/6.2] Fluxc uncertainty (ETotalflux_pbcor) (G1) 44- 49 F6.4 mJy s_Fluxc [0.009/5] Fluxc error but estimated from our own simulation statistics (ETotalfluxsimpbcor) 51- 55 F5.3 --- Pbcor [0.2/1] Primary beam attenuation (PBA) factor 57- 62 F6.3 arcsec Beam [8.6/64.6] ALMA 12m antenna's primary beam FWHM size at the observing frequency (Primary_beam) 64- 70 F7.4 mJy/beam FPk [0.02/27.6] Fitted ALMA continuum emission's peak flux, uncorrected for PBA (Peak_flux) 72- 77 F6.4 mJy/beam rms [0.005/1.8] Pixel rms noise in the continuum image (RMS_noise) 79- 85 F7.3 GHz Freq [90.2/671.5] Observing frequency, i.e., the center frequency of all collapsed spectral windows (Obs_frequency) 87- 94 F8.3 um lambda [446.4/3323.7] Observing wavelength =(2.99792458x105)/Freq (Obs_wavelength) 96-101 F6.3 arcsec FWHMa [0.1/3.9] Synthesized beam's major-axis FWHM size (Maj_beam) 103-108 F6.3 arcsec FWHMb [0.09/2.6] Synthesized beam's minor axis FWHM size (Min_beam) 110-116 F7.3 deg PA [-90/90] Synthesized beam's position angle; zero means to the north (PA_beam) 118-215 A98 --- FileName Name of the image FITS file in subdirectory fits (Image_file) 217 A1 --- Mult [MS] Flag= S (or M) means that the source is fitted with single (or multiple) Gaussian component(s) (Flag_multi) 219 I1 --- Flag [0/1] 0=reliable flux (Flaginconsistentflux) (G2) -------------------------------------------------------------------------------- Byte-by-byte Description of file: prior.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 I7 --- ID A3COSMOS master catalog identification number (G3) 9- 15 I7 --- OID ID number in "Ref" (ID_PriorCat) 17- 28 A12 --- Ref The reference of the prior catalog in which the source is first included (RefIDPriorCat) (1) 30- 40 F11.7 deg RAdeg Right ascension of the ALMA emission (J2000) 42- 50 F9.7 deg DEdeg Declination of the ALMA emission (J2000) 52- 58 F7.4 mJy Fluxc [0.04/55.6] The fitted total flux with Gaussian source models, corrected for flux bias and PBA (Totalfluxpbcor) 60- 65 F6.4 mJy e_Fluxc [0.01/6.2] Fluxc uncertainty (ETotalflux_pbcor) (G1) 67- 72 F6.4 mJy s_Fluxc [0.01/5.7] Fluxc error but estimated from our own simulation statistics (ETotalfluxsimpbcor) 74- 78 F5.3 --- Pbcor [0.2/1] Primary beam attenuation (PBA) factor 80- 85 F6.3 arcsec Beam [8.6/64.6] ALMA 12m antenna's primary beam FWHM size at the observing frequency (Primary_beam) 87- 93 F7.4 mJy/beam FPk [0.02/27.6] Fitted ALMA continuum emission's peak flux, uncorrected for PBA (Peak_flux) 95-100 F6.4 mJy/beam rms [0.005/1.8] Pixel rms noise in the continuum image (RMS_noise) 102-108 F7.3 GHz Freq [90.1/671.5] Observing frequency, i.e., the center frequency of all collapsed spectral windows (Obs_frequency) 110-117 F8.3 um lambda [446.4/3325.5] Observing wavelength =(2.99792458x105)/Freq (Obs_wavelength) 119-123 F5.3 arcsec FWHMa [0.1/3.9] Synthesized beam's major-axis FWHM size (Maj_beam) 125-129 F5.3 arcsec FWHMb [0.09/2.6] Synthesized beam's minor axis FWHM size (Min_beam) 131-137 F7.3 deg PA [-90/90] Synthesized beam's position angle; zero means to the north (PA_beam) 139-236 A98 --- FileName Name of the image FITS file in subdirectory fits (Image_file) 238-243 F6.3 --- Chi2 [0.01/48.2] The reduced χ2 of galfit prior source fitting, measured from the residual image for each source with an aperture of 1.0" in diameter (Galfitreducedchi_square) 245 I1 --- Bound [0/1] Flag=1 means that the fitted source major-axis FWHM size reaches the upper boundary of 3.0" and should be used with caution (Flagsizeupper_boundary) 247 I1 --- Flag [0/1] 0=Reliable flux (Flaginconsistentflux) (G2) 249 I1 --- CPA [0/1] Unreliable counterpart outlier flag; see Section 4.2 (FlagoutlierCPA) 251 I1 --- SED [0/1] SED-excess outlier flag; see Section 4.4 (FlagoutlierSED) -------------------------------------------------------------------------------- Note (1): Reference as follows: Ashby2018 = UltraVISTA Ultra-deep Stripes (SMUVS; Ashby et al. 2018, J/ApJS/237/39) (135 occurrences) Capak2007 = i-band catalog; Capak et al. 2007, II/284 (5 occurrences) Davidzon2017 = Photometric catalog; Davidzon et al. 2017A&A...605A..70D 2017A&A...605A..70D (19 occurrences) Laigle2016 = COSMOS2015 catalog; Laigle+ 2016, J/ApJS/224/24 (1050 occurrences) LeFloch2009 = COSMOS mid-IR catalog; Le Floc'h et al. 2009ApJ...703..222L 2009ApJ...703..222L (2 occurrences) Muzzin2013 = K-band catalog; Muzzin et al. 2013, J/ApJ/777/18 (44 occurrences) Sanders2007 = IRAC catalog; Sanders et al. 2007ApJS..172...86S 2007ApJS..172...86S (7 occurrences) Smolcic2017 = VLA catalog; Smolcic et al. 2017, J/A+A/602/A1 (15 occurrences) -------------------------------------------------------------------------------- Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 I7 --- ID [168767/1389517] A3COSMOS master catalog identification number (G3) 9- 22 F14.10 deg RAdeg Right ascension of the ALMA emission (J2000) 24- 35 F12.10 deg DEdeg Declination of the ALMA emission (J2000) 37- 42 F6.4 --- z [0.3/7.3] SED best-fit redshift from the list of prior redshifts 44 A1 --- f_z p: photometric or s: spectroscopic 46- 48 I3 --- q_z [1/212]? Quality flag "Qz" for dzLiu or S17 50- 54 A5 --- r_z Reference for z (1) 56- 82 A27 --- zPrior Prior redshifts in the literature (z_prior) 84-171 A88 --- r_zPrior References of zPrior (Refzprior) (2) 173-181 E9.4 Msun Mstar [2.7e+9/8.4e+12] Stellar mass from our SED fitting (M_star) (3) 183-191 E9.4 Lsun Ldust [9.3e+10/3.9e+13] Infrared 8-1000u luminosity from dust (L_dust) (3) 193-200 F8.3 Msun/yr SFR [9.3/3890.5] SFR integrated from SFH (3) 202-207 F6.3 Gyr-1 sSFR [0.1/35] Specific SFR from SFH; SFR/Mstarx109 -------------------------------------------------------------------------------- Note (1): Reference as follows: L16 = Laigle+ 2016, J/ApJS/224/24 (COSMOS2015) dzLiu = "dzliu_known" in r_zPrior; the source has the spectroscopic redshift confirmed in our A3COSMOS data cube analysis with at least one S/N>6 spectral line (Section 4.5; D. Liu et al. 2019, in preparation). S17 = Salvato+ 2017: COSMOS spec-z catalog compiled by M. Salvato et al. (available in the COSMOS collaboration; version 07SEP2017 with 103,964 rows) S11c = Salvato+ 2011, J/ApJ/742/61 Chandra catalog S11x = Salvato+ 2011, J/ApJ/742/61 XMM catalog D17 = Delvecchio+ 2017A&A...602A...3D 2017A&A...602A...3D D17b = Davidzon+ 2017A&A...605A..70D 2017A&A...605A..70D J18 = Jin+ 2018ApJ...864...56J 2018ApJ...864...56J Note (2): The photo-z is inconsistent with any previous redshift by >0.15x(1+z) difference. Note (3): Stellar mass, luminosity and SFR from our SED fitting at redshift z; assumed Chabrier (2003PASP..115..763C 2003PASP..115..763C) IMF. -------------------------------------------------------------------------------- Global notes: Note (G1): Error in "Totalfluxpbcor", provided by photometry pipelines based on Condon (1997PASP..109..166C 1997PASP..109..166C) simulation statistics and equations. Note (G2): Inconsistent-flux outliers, described in Section 2.5. Flag=1 means that the source has >5σ inconsistent total fluxes from our prior and blind photometry Note (G3): A3COSMOS master catalog ID (version 20170426), which equals Laigle+ (2016, J/ApJS/224/24) COSMOS2015 catalog ID when ID≤1182108. -------------------------------------------------------------------------------- History: From electronic version of the journal for the three catalogs. FITS continuum images downloaded at: http://irsa.ipac.caltech.edu/data/COSMOS/images/a3cosmos/ References: Liu et al. Paper I. 2019ApJS..244...40L 2019ApJS..244...40L This catalog Liu et al. Paper II. 2019ApJ...887..235L 2019ApJ...887..235L Fudamoto et al. Paper III. 2020MNRAS.491.4724F 2020MNRAS.491.4724F
(End) Emmanuelle Perret [CDS] 09-Mar-2020
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