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J/AJ/136/2136    HST/ACS Atlas of Great Orion Nebula proplyds     (Ricci+, 2008)

The Hubble Space Telescope/Advanced Camera for Surveys atlas of protoplanetary disks in the Great Orion Nebula. Ricci L., Robberto M., Soderblom D.R. <Astron. J., 136, 2136-2151 (2008)> =2008AJ....136.2136R
ADC_Keywords: H II regions ; Nebulae ; Cross identifications ; Atlases Keywords: ISM: individual (Orion Nebula) - ISM: jets and outflows - planetary systems: protoplanetary disks - reflection nebulae - stars: formation - stars: pre-main sequence Abstract: We present the atlas of protoplanetary disks in the Orion Nebula based on the Wide Field Channel of the Advanced Camera for Surveys (ACS/WFC) images obtained for the Hubble Space Telescope (HST) Treasury Program on the Orion Nebula Cluster. The observations have been carried out in five photometric filters nearly equivalent to the standard B, V, Hα, I, and z passbands. Our master catalog lists 178 externally ionized protoplanetary disks (proplyds), 28 disks seen only in absorption against the bright nebular background (silhouette disks), eight disks seen only as dark lanes at the midplane of extended polar emission (bipolar nebulae or reflection nebulae), and five sources showing jet emission with no evidence of either external ionized gas emission or dark silhouette disks. Description: The images have been extracted from the large dataset (520 images) of ACS/WFC observations executed between 2004 November and 2005 April. The ACS/WFC survey has covered an area of about 450arcmin2, centered about 4' southwest of the Trapezium cluster. In data subdirectory, every file name has the structure: object name+"_"+filter+".fits", where object name is the name of the object as reported in the paper and filter is the HST/ACS photometric filter of the image. These images are astrometrically correct, i.e. field distortion has been removed. The fits headers contain the correct astrometric information (WCS) and return absolutely calibrated coordinates. In these drizzled images the pixel values are in counts per second, and an estimate in magnitudes of the photometry of a source can be directly extracted by m=-2.5Log(F)+ZP, where m is the magnitude of the source in the passband of interest, F is the observed flux of the source in counts per second in that passband, and ZP is the passband zero-point magnitude in a certain photometric system. In the paper, Table 2 lists the zero-point magnitudes derived by the Photometric Calibration of the HST/ACS camera (Sirianni et al., 2005PASP..117.1049S) in the VEGAMAG, ABMAG and STMAG standard photometric systems for the filters used by our survey. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 95 219 Circumstellar disks from the HST/ACS Treasury Program list.dat 31 1335 List of images in "data" subdirectory data/* 0 1335 Images of sources in 5 HST filters
See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) J/AJ/111/846 : Orion HST survey (O'Dell+ 1996) J/ApJS/160/319 : COUP: observations and source lists (Getman+, 2005) Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Object identification (NNNN-NNNN) (G1) 10 I1 h RAh Hour of Right Ascension (J2000) 12- 13 I2 min RAm Minute of Right Ascension (J2000) 15- 19 F5.2 s RAs Second of Right Ascension (J2000) 21 A1 --- DE- Sign of the Declination (J2000) 22 I1 deg DEd Degree of Declination (J2000) 24- 25 I2 arcmin DEm Arcminute of Declination (J2000) 27- 31 F5.2 arcsec DEs Arcsecond of Declination (J2000) 33- 40 A8 --- [OW94] O'Dell catalogs identification (1) 42- 49 A8 --- [BOM2000] Bally et al. (2000AJ....119.2919B)/Smith et al. (2005AJ....129..382S) identification 51- 53 I3 --- JW ? ID in Jones & Walker (1988AJ.....95.1755J) 55- 57 I3 --- PSH ? ID in Prosser et al. (1994ApJ...421..517P) 59- 62 I4 --- [AD95] ? ID in Ali & DePoy (1995AJ....109..709A) 64- 80 A17 --- 2MASS ID in 2MASS (Cutri et al. 2003, Cat. II/246) 82- 85 I4 --- COUP ? ID in COUP (Getman et al. 2005, Cat. J/ApJS/160/319) 87- 88 A2 --- Type Source type (2) 90- 95 A6 --- Note Additional note(s) (3)
Note (1): O'Dell & Wen 1994ApJ...436..194O, O'Dell & Wong 1996, Cat. J/AJ/111/846, and O'Dell 2001AJ....122.2662O. Note (2): Source type as follows: i = ionized disk seen in emission d = dark disk seen only in silhouette rn = reflection nebulae with no external ionized gas emission j = jet emission with no evidence of neither ionized disk nor silhouette disk Note (3): Additional notes as follows: J = jet RN = reflection nebula EO = disk seen nearly edge-on FO = disk seen nearly face-on B = binary system
Byte-by-byte Description of file: list.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Object identification (NNNN-NNNN) (G1) 11- 31 A21 --- FileName Name of the image in subdirectory data
Global notes: Note (G1): Sources identified as <[RRS2008] NNNN-NNNN> in Simbad: * NNNN-NNN : MSSs-MSS (position: 5 3M SS.s -5 2M SS) * NNN-NNN : SSs-MSS (position: 5 35 SS.s -5 2M SS) * NNN-NNNN : SSs-MMSS (position: 5 35 SS.s -5 MM SS) * NNNN-NNNN : MSSs-MMSS (position: 5 3M SS.s -5 MM SS)
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 20-May-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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