Access to Astronomical Catalogues

← Click to display the menu
J/ApJ/606/664       MAMBO sources near NTT Deep Field       (Dannerbauer+, 2004)

The faint counterparts of MAMBO millimeter sources near the New Technology Telescope Deep Field. Dannerbauer H., Lehnert M.D., Lutz D., Tacconi L., Bertoldi F., Carilli C., Genzel R., Menten K.M. <Astrophys. J., 606, 664-682 (2004)> =2004ApJ...606..664D
ADC_Keywords: Radio sources ; Infrared sources ; Redshifts ; Photometry Keywords: galaxies: formation - galaxies: high-redshift - galaxies: starburst - infrared: galaxies - submillimeter Abstract: We discuss identifications for 18 sources from our Max-Planck- Millimeter-Bolometer (MAMBO) 1.2mm survey of the region surrounding the NTT Deep Field. We have obtained accurate positions from Very Large Array 1.4GHz interferometry, and in a few cases IRAM millimeter interferometry, and have also made deep BVRIzJK imaging at ESO. Description: The NTT Deep Field was observed at 1.4GHz with the VLA in 2001 April and May for 15hr in the B configuration (10 km maximum baseline). Standard wide-field imaging mode was employed (50MHz total bandwidth, with two polarizations and 16 spectral channels). We use the BVRIK imaging of a field centered on the NDF that is described in Paper I, Dannerbauer et al. (2002ApJ...573..473D). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 117 23 NDF MAMBO sources and associated 1.4GHz radio sources table2.dat 111 82 Optical/near-infrared objects close to the interferometric positions
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 17 A17 --- [DLL2002] Source designation, MM JHHMMSS-DDMM.m 19- 20 I2 --- MAMBO ? Short number on the original MAMBO NDF source list, MAMBO NTT-MM NN in Simbad 22- 23 I2 h RAh MAMBO 1.2mm Right ascension (J2000.0) 25- 26 I2 min RAm MAMBO 1.2mm Right ascension (J2000.0) 28- 32 F5.2 s RAs MAMBO 1.2mm Right ascension (J2000.0) 34 A1 --- DE- MAMBO 1.2mm Declination sign (J2000.0) 35- 36 I2 deg DEd MAMBO 1.2mm Declination (J2000.0) 38- 39 I2 arcmin DEm MAMBO 1.2mm Declination (J2000.0) 41- 44 F4.1 arcsec DEs MAMBO 1.2mm Declination (J2000.0) 46 A1 --- l_S1.2mm Limit flag on S1.2mm 47- 49 F3.1 mJy S1.2mm MAMBO 1.2mm peak flux density 51- 53 F3.1 mJy e_S1.2mm rms uncertainty on S1.2mm 54 A1 --- n_S1.2mm [a] Note on S1.2mm (1) 56- 57 I2 h RAVh VLA 1.4GHz Right ascension (J2000.0) 59- 60 I2 min RAVm VLA 1.4GHz Right ascension (J2000.0) 62- 66 F5.2 s RAVs VLA 1.4GHz Right ascension (J2000.0) 68- 71 F4.2 s e_RAVs rms uncertainty on RAVs 73 A1 --- DEV- VLA 1.4GHz Declination sign (J2000.0) 74- 75 I2 deg DEVd VLA 1.4GHz Declination (J2000.0) 77- 78 I2 arcmin DEVm VLA 1.4GHz Declination (J2000.0) 80- 83 F4.1 arcsec DEVs VLA 1.4GHz Declination (J2000.0) 85- 87 F3.1 arcsec e_DEVs rms uncertainty on DEVs 89- 91 I3 uJy S.14GHz ? VLA 1.4GHz peak flux density 93- 95 F3.1 arcsec Sep ? Separation between MAMBO and VLA positions 97-101 F5.3 --- Prob ? Probability that the association is a chance coincidence 103 A1 --- Qual [gu] Quality flag for good (g) and uncertain (u) radio sources (2) 105-117 A13 --- Com Comments
Note (1): The source MM J120534-0738.3 appears to be extended and may be multiple or smeared. For consistency with the other sources, we list its peak flux, which is effectively a lower limit to the true flux. The source was included because of a reliable detection in total flux and a 1.4GHz counterpart. Note (2): To declare the quality of a radio source good, two criteria have to be fulfilled: (1) Source does not disappear in the "background-subtracted" radio map, and (2) no eye-catching clustering of greater than 40µJy peaks in the adjacent region.
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 2 I2 --- MAMBO MAMBO number of the source (1) 3- 4 A2 --- m_MAMBO Optical/near-infrared source identification (1) 5 A1 --- n_MAMBO [*] *: suggested counterparts to millimeter sources 6 A1 --- f_MAMBO [a] Note on Source 03d (2) 7- 8 I2 h RAh Right ascension (J2000.0) 10- 11 I2 min RAm Right ascension (J2000.0) 13- 17 F5.2 s RAs Right ascension (J2000.0) 19 A1 --- DE- Declination sign (J2000.0) 20- 21 I2 deg DEd Declination (J2000.0) 23- 24 I2 arcmin DEm Declination (J2000.0) 26- 29 F4.1 arcsec DEs Declination (J2000.0) 31- 33 F3.1 arcsec Sep Separation between optical position and best interferometric position 35 A1 --- f_Bmag [~!] Note on Bmag (3) 36 A1 --- l_Bmag Limit flag on Bmag 37- 41 F5.2 mag Bmag B magnitude in a 2" aperture (4) 42 A1 --- n_Bmag [bde] Contaminated magnitude (5) 43 A1 --- f_Vmag [~!] Note on Vmag (3) 44 A1 --- l_Vmag Limit flag on Vmag 45- 49 F5.2 mag Vmag V magnitude in a 2" aperture (4) 50 A1 --- n_Vmag [bde] Contaminated magnitude (5) 51 A1 --- f_Rcmag [~!] Note on Rcmag (3) 52 A1 --- l_Rcmag Limit flag on Rcmag 53- 57 F5.2 mag Rcmag Cousins R magnitude in a 2" aperture (4) 58 A1 --- n_Rcmag [bde] Contaminated magnitude (5) 59 A1 --- f_Icmag [~!] Note on Icmag (3) 60 A1 --- l_Icmag Limit flag on Icmag 61- 65 F5.2 mag Icmag Cousins I magnitude in a 2" aperture (4) 66 A1 --- n_Icmag [bde] Contaminated magnitude (5) 67 A1 --- f_zmag [~!] Note on zmag (3) 68 A1 --- l_zmag Limit flag on zmag 69- 73 F5.2 mag zmag z magnitude in a 2" aperture (4) 74 A1 --- n_zmag [bd] Contaminated magnitude (5) 75 A1 --- f_Jmag [~!] Note on Jmag (3) 76 A1 --- l_Jmag Limit flag on Jmag 77- 81 F5.2 mag Jmag J magnitude in a 2" aperture (4) 83 A1 --- f_Kmag [~!] Note on Kmag (3) 84 A1 --- l_Kmag Limit flag on Kmag 85- 89 F5.2 mag Kmag K magnitude in a 2" aperture (4) 90 A1 --- n_Kmag [c] c: M. D. Lehnert et al. (2004), in prep. 92- 95 F4.2 --- zphot Optical/near-infrared photometric redshift 97-100 F4.2 --- E_zphot Error on zphot (upper limit) 102-105 F4.2 --- e_zphot Error on zphot (lower limit) 107-111 F5.3 --- Prob ? Probability of a chance coincidence with an object of the given K magnitude (07a: B) at the given separation
Note (1): The optical/near-infrared objects is designated with a combination of the short MAMBO number (Table 1) and a letter increasing with distance from the interferometric position. [DLL2004] MAMBO NTT-MM NNa in Simbad Note (2): (a) 03d is not detected in B, z, and K, but retained because of credible R and I detections Note (3): For the measurements in the individual bands, we indicate cases in which we consider the SExtractor aperture magnitudes more uncertain, since the object is only tentatively (~) or not (!) picked up by eye in the visual inspection. Note (4): All magnitudes are on the Vega system except for the z magnitudes, which are on the BD system (see text). Note (5): Notes as follows: b = Magnitude contaminated by 10a1. d = Magnitude contaminated by nearby foreground galaxy. e = Magnitude contaminated by nearby foreground star.
History: From electronic version of the journal References: Dannerbauer et al., Paper I 2002ApJ...573..473D
(End) James Marcout, Patricia Vannier [CDS] 02-Jul-2004
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

catalogue service