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J/ApJ/692/422       MAMBO observations of SWIRE sources        (Lonsdale+, 2009)

MAMBO 1.2 mm observations of luminous starbursts at z ∼ 2 in the SWIRE fields. Lonsdale C.J., Polletta M.DEL C., Omont A., Shupe D., Berta S., Zylka R., Siana B., Lutz D., Farrah D., Smith H.E., Lagache G., De Breuck C., Owen F., Beelen A., Weedman D., Franceschini A., Clements D., Tacconi L., Afonso-Luis A., Perez-Fournon I., Cox P., Bertoldi F. <Astrophys. J., 692, 422-442 (2009)> =2009ApJ...692..422L
ADC_Keywords: Photometry, ugriz ; Redshifts ; Galaxies, IR ; Extinction ; Photometry, millimetric/submm Keywords: cosmology: observations - galaxies: formation - galaxies: starburst - galaxies: high-redshift - infrared: galaxies - submillimeter Abstract: We report on-off pointed MAMBO observations at 1.2mm of 61 Spitzer-selected star-forming galaxies from the Spitzer Wide Area Infrared Extragalactic Legacy survey (SWIRE). The sources are selected on the basis of bright 24um fluxes (F24um>0.4mJy) and of stellar dominated near-infrared spectral energy distributions in order to favor z∼2 starburst galaxies. The average 1.2mm flux for the whole sample is 1.5±0.2mJy. Our analysis focuses on 29 sources in the Lockman Hole field where the average 1.2mm flux (1.9±0.3mJy) is higher than in other fields (1.1±0.2mJy). The analysis of the multiwavelength spectral energy distributions indicates that these sources are starburst galaxies with far-infrared luminosities from 1012 to 1013.3L, and stellar masses of ∼0.2-6x1011M. Compared to submillimeter selected galaxies (SMGs), the SWIRE-MAMBO sources are among those with the largest 24um/1.2mm flux ratios. The origin of such large ratios is investigated by comparing the average mid-infrared spectra and the stacked far-infrared spectral energy distributions of the SWIRE-MAMBO sources and of SMGs. Description: Observations were spread over the pool observing sessions at the Institut de Radioastronomie Millimetrique (IRAM) 30m telescope in fall/winter 2005/2006, using the 117 element version of the Max Planck Millimeter Bolometer (MAMBO) array operating at a wavelength of 1.2mm (250GHz). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 105 61 Basic properties of the SWIRE-MAMBO sample table2.dat 64 61 Optical and infrared data of the SWIRE-MAMBO sample table4.dat 25 113 *Best-fit templates and photometric redshifts for the 61 SWIRE objects
Notes on table4.dat: The solutions are listed in order of χ2.
See also: II/290 : SWIRE Photometric Redshift Catalogue (Rowan-Robinson+, 2008) II/255 : SWIRE ELAIS N1 Source Catalogs (Surace+, 2004) J/MNRAS/401/294 : Optical identification of XMM-LSS sources (Stalin+, 2010) J/ApJ/703/1778 : Spitzer sources in SWIRE/XMM/ELAIS-S1 field (Sacchi+, 2009) J/A+A/490/879 : XMM-LSS field optical identifications (Tasse+, 2008) J/AJ/136/1889 : 20cm observations of deep Swire Field (Owen+, 2008) J/A+A/467/565 : z=1-3 ULIRGs from the Spitzer SWIRE survey (Berta+, 2007) J/MNRAS/371/1891 : GOODS ELAIS-N1 24um flux densities (Rodighiero+, 2006) http://irsa.ipac.caltech.edu/data/SPITZER/SWIRE/ : SWIRE data access Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 3 A3 --- Field Field (G1) 5- 6 I2 --- Seq Running sequence number (G1) 8 A1 --- l_S/N [<] Limit on S/N detection 9 I1 --- S/N Signal detection (signal at Nσ) 11 A1 --- --- [S] 12- 30 A19 --- SWIRE SWIRE identification (JHHMMSS.ss+DDMMSS.s) (1) 32- 41 F10.6 deg RAdeg Right ascension in decimal degrees (J2000) 42- 50 F9.6 deg DEdeg Declination in decimal degrees (J2000) 52- 55 F4.2 --- z Photometric redshift 57 A1 --- f_z [c] c for spectroscopic z from IRS spectrum (2) 59- 63 F5.2 mJy F1.2mm MAMBO 1.2mm flux (250GHz) 65- 68 F4.2 mJy e_F1.2mm F1.2mm uncertainty 70 A1 --- l_F70 Limit flag on F70 71- 72 I2 mJy F70 Spitzer/MIPS 70um flux 74 I1 mJy e_F70 ? F70 uncertainty 76 A1 --- l_F160 Limit flag on F160 77- 79 I3 mJy F160 Spitzer/MIPS 160um flux 81 I1 mJy e_F160 ? F160 uncertainty 83- 87 F5.3 mJy F20cm ? VLA 20cm flux 89- 93 F5.3 mJy e_F20cm ? F20cm uncertainty 95-104 A10 --- Note Shape of the IRAS SED (3) 105 A1 --- f_Note [d] Flag for LH 10 (4)
Note (1): SJ stands for SWIRE J. SWIRE JHHMMSS.ss+DDMMSS.s is the official IAU source name for sources discovered in the SWIRE fields. Note (2): IRS spectra of LH sources are published in Weedman et al. (2006ApJ...653..101W), those of EN2 will be published in a future publication (C. J. Lonsdale et al. 2009, in preparation). Note (3): Notes about the IR spectrum: b2 = peak at 4.5um b3 = peak at 5.8um b4 = peak at 8.0um fl = flat IRAC SED IRS = sources with IRS observations B# = refers to the source ID in Weedman et al. (2006ApJ...653..101W) X = sources with X-ray coverage Note (4): X-ray source 425 in CLASX catalog (Yang et al. 2004, Cat. J/AJ/128/1501), F(0.4-8keV)=2.1x10-15erg/cm2/s (2.1aW/m2) and HR=-0.7.
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 3 A3 --- Field Field (G1) 5- 6 I2 --- Seq Running sequence number (G1) 8 A1 --- l_umag Limit flag on umag (5) 9- 13 F5.2 mag umag ? SWIRE u-band magnitude (Vega) (5) 15 A1 --- l_g'mag Limit flag on g'mag (5) 16- 20 F5.2 mag g'mag ? SWIRE g'-band magnitude (Vega) (5) 22 A1 --- l_r'mag Limit flag on r'mag (5) 23- 27 F5.2 mag r'mag SWIRE r'-band magnitude (Vega) (5) 29 A1 --- l_i'mag Limit flag on i'mag (5) 30- 34 F5.2 mag i'mag ? SWIRE i'-band magnitude (Vega) (5) 36 A1 --- l_zmag Limit flag on zmag (5) 37- 41 F5.2 mag zmag ? SWIRE z-band magnitude (Vega) (5) 43- 44 I2 uJy F3.6 Spitzer/IRAC 3.6um flux (5) 46 A1 --- l_F4.5 Limit flag on F4.5 (5) 47- 49 I3 uJy F4.5 Spitzer/IRAC 4.5um flux (5) 51 A1 --- l_F5.8 Limit flag on F5.8 (5) 52- 54 I3 uJy F5.8 Spitzer/IRAC 5.8um flux (5) 56 A1 --- l_F8.0 Limit flag on F8.0 (5) 57- 59 I3 uJy F8.0 Spitzer/IRAC 8.0um flux (5) 61- 64 I4 uJy F24 Spitzer/MIPS 24um flux (5)
Note (5): Typical uncertainties are ∼5% for the optical and the IRAC data, and 10% for MIPS. Upper limits correspond to 90% completeness in the optical and to 5σ in the infrared.
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 3 A3 --- Field Field (G1) 5- 6 I2 --- Seq Running sequence number (G1) 8- 12 F5.3 --- z Photometric redshift 14- 17 F4.2 --- AV Extinction 19- 25 A7 --- Tpl Best-fit template (1)
Note (1): All the "ce" templates are from the library in Chary & Elbaz (2001ApJ...556..562C), the others are from the library in Polletta et al. (2007, Cat. J/ApJ/663/81). The fits are shown in Figure 13.
Global notes: Note (G1): Fields are LH for Lockman-Hole, EN for ELAIS-N and XMM for XMM-LSS. The sources are ordered by field and signal-to-noise ratio at 1.2mm.
Nomenclature notes: These objects are <[LPO2009] Field Seq> in Simbad. History: From electronic version of the journal
(End) Emmanuelle Perret [CDS] 03-Mar-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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