J/MNRAS/454/2586     UWISH2 extended H2 emission line sources (Froebrich+, 2015)

Extended H2 emission line sources from UWISH2. Froebrich D., Makin S.V., Davis C.J., Gledhill T.M., Kim Y., Koo B.-C., Rowles J., Eisloffel J., Nicholas J., Lee J.J., Williamson J., Buckner A.S.M. <Mon. Not. R. Astron. Soc., 454, 2586-2605 (2015)> =2015MNRAS.454.2586F 2015MNRAS.454.2586F (SIMBAD/NED BibCode)
ADC_Keywords: Galactic plane ; H II regions ; Planetary nebulae ; Supernova remnants Keywords: stars: formation - H II regions - ISM: individual: Galactic Plane - ISM: jets and outflows - planetary nebulae: general - ISM: supernova remnants Abstract: We present the extended source catalogue for the UKIRT Wide Field Infrared Survey for H2 (UWISH2). The survey is unbiased along the inner Galactic Plane from l∼357° to l∼65° and |b|≤1.5° and covers 209deg2. A further 42.0 and 35.5deg2 of high dust column density regions have been targeted in Cygnus and Auriga. We have identified 33200 individual extended H2 features. They have been classified to be associated with about 700 groups of jets and outflows, 284 individual (candidate) planetary nebulae, 30 supernova remnants and about 1300 photodissociation regions. We find a clear decline of star formation activity (traced by H2 emission from jets and photodissociation regions) with increasing distance from the Galactic Centre. About 60 percent of the detected candidate planetary nebulae have no known counterpart and 25 percent of all supernova remnants have detectable H2 emission associated with them. Description: All data were acquired using the Wide Field Camera (WFCAM) on the United Kingdom Infrared Telescope (UKIRT), Mauna Kea, Hawaii. WFCAM houses four Rockwell Hawaii-II (HgCdTe 2048x2048-pixel) arrays spaced by 94 per cent in the focal plane. The pixel scale measures 0.4-arcsec, although microstepping is used to generate reduced mosaics with a 0.2-arcsec pixel scale and thereby fully sample the expected seeing. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tableb1.dat 107 284 Table listing all the PNe detected in our survey tablec1.dat 91 49 *Table listing all the images taken for the survey tabled1.dat 151 69 *Table listing all the extended H2 features in our survey -------------------------------------------------------------------------------- Note on tablec1.dat: This table is only an excerpt of the first few images. Note on tabled1.dat: This table is only an excerpt of the first few objects. -------------------------------------------------------------------------------- Byte-by-byte Description of file: tableb1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- --- [PNUWISH2] 11- 27 A17 --- PN_UWISH2 Source PN UWISH2 name (LLL.lllll+B.bbbbb) 29- 37 F9.5 deg RAdeg Right ascension of the geometric centre of the H2 emitting feature (J2000) 39- 47 F9.5 deg DEdeg Declination of the geometric centre of the H2 emitting feature (J2000) 49- 53 F5.1 arcsec Rad Radius around the central position enclosing all the H2 emission 55- 61 F7.2 arcsec+2 Area Area covered with H2 emission 63- 71 F9.2 10-19W/m2 Ftot Total flux of the PN 73- 80 F8.2 10-19W/m2 Fmed Median flux of the PN 82-107 A26 --- OName Other name (1) -------------------------------------------------------------------------------- Note (1): other known name/identifier or coinciding object (not necessarily a PN). New indicates objects that have so far not been recognized as PNe or PNe candidates in the literature. -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablec1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- Tile Tile name 15- 31 A17 --- Image Image name 33- 41 F9.5 deg RAdeg Right ascension of image centre (J2000) 43- 51 F9.5 deg DEdeg Declination of image centre (J2000) 53- 60 F8.5 deg GLON Galactic longitude of the image centre 62- 69 F8.5 deg GLAT Galactic latitude of the image centre 71- 74 F4.2 arcsec Seeing Seeing in the image 76- 80 F5.2 mag mapzp Magnitude zero-point 82- 86 F5.3 mag e_mapzp rms uncertainty on mapzp 88- 91 F4.2 10-19W/m2/arcsec2 Noise Noise -------------------------------------------------------------------------------- Byte-by-byte Description of file: tabled1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- --- [UWISH2_] 8- 24 A17 --- UWISH2 Source UWISH2 designation (LLL.lllll+B.bbbbb) 26- 34 F9.5 deg RAdeg Right ascension (J2000) 36- 44 F9.5 deg DEdeg Declination (J2000) 46- 51 F6.2 arcsec+2 Area Area of the H2 feature 53- 56 F4.1 arcsec Rad Radius of the H2 feature 58- 61 F4.2 10-19W/m2/arcsec2 Fmedsb Median surface brightness 63- 70 F8.2 10-19W/m2/arcsec2 Fmaxsb Maximum surface brightness 72- 75 F4.2 --- Fsigma One-pixel rms noise of the background 77- 84 F8.2 10-19W/m2 Ftot Total flux of the H2 feature 86- 89 F4.1 % DF/F Relative flux uncertainty due to photometric calibration 91 A1 --- Class [ujps] Classification code (1) 93-104 A12 --- Tile Tile name object is on 106-122 A17 --- Image Image name the object is on 124-151 A28 --- Group Name of group the object is associated with -------------------------------------------------------------------------------- Note (1): Classification code as follows: j = jet p = PN s = SNR u = unknown, most likely PDR -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 15-Jul-2016
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