cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.17909/t9d30c
title: Bianchi, Conti, Shiao (BCS) Catalog of Unique GALEX Sources ("BCSCAT")

description: The GALEX spacecraft operated for over 10 years and surveyed nearly the entire sky during its lifetime. The telescope observed in both FUV (1344-1786 Angstroms) and NUV (1771-2831 Angstroms) simultaneously until May 2009, when the FUV detector failed. The NUV detector continued to operate until June 2013, when GALEX was retired and the mission ended. The standard GALEX data products at MAST include visit and coadd image files, as well as a source catalog produced by the GALEX reduction pipeline called the 'MCAT'. The MCAT consists of over 200 million source measurements, but, since it was run on each tile, there are multiple measurements of the same source due to tile overlaps and different surveys (AIS, MIS, DIS, Guest Investigator, etc.) To rectify the situation, Bianchi et al. have constructed a catalog of unique sources: one based on All-Sky Imaging Survey (AIS) tiles, and another based on Medium-Sky Imaging Survey (MIS) tiles.  These catalogs are homogeneous in depth and quality, and are optimal for cross-matching GALEX UV fluxes with data in other bands (e.g., for source selection combining optical or IR data), or for Galactic and extragalactic population studies.
DOI: 10.17909/t9gw2p
title: Hubble Space Telescope ACS Mosaic Images of M82 ("M82")

description: In March 2006, the Hubble Heritage Team obtained a large 4-color mosaic image of the M82 with the Advanced Camera for Surveys (ACS) onboard the Hubble Space Telescope (HST). See 10776 PI: Matt Mountain) for details.  The resulting color composite image was released to the community on April 24, 2006 to celebrate Hubble's 16th anniversary. Since the M82 mosaics produced by the Hubble Heritage Team represent a significant investment of expert processing beyond the standard archival products, these drizzle-combined FITS have now been released as a High-Level Science Product via MAST.
DOI: 10.17909/t9mk5z
title: Hubble Ultra Deep Field Follow-on

description: PI Massimo Stiavelli and colleagues obtained an HST cycle 14 program 10632 titled Searching for galaxies at z&gt;6.5 in the Hubble Ultra Deep Field(also known as UDF05). The program was conceived as a follow-on program to the Hubble Ultra Deep Field (HUDF) and was designed to obtain deep ACS (F606W, F775W, F850LP) imaging in the area of the original HUDF NICMOS parallel fields. In addition, deep NICMOS (F110W, F160W) images within the original HUDF field were made as simultaneous parallel observations.
DOI: 10.17909/t9rc7w
title: The HST Treasury Program on the Orion Nebula Cluster ("ORION")

description: The Orion Nebula hosts the richest cluster of young pre-main-sequence stars within 1 kpc from the Sun and therefore represents an ideal laboratory to understand the process of star formation.  The 'ORION' HLSP is an HST Treasury Program on the Orion Nebula cluster (GO-10246, PI M. Robberto) that has obtained deep multi-color photometry of thousand of sources well into the brown-dwarf regime, complemented by a rich set of ancillary data from ground-based observatories.
DOI: 10.17909/t9w30q
title: GALEX Unique Source Catalogs ("GCAT")

description: GALEX undertook a number of surveys covering large areas of the sky at a variety of depths. However, making use of this large data set can be difficult because the standard GALEX database contains all of the detected sources, which include many duplicate observations of the same sources, as well as numerous spurious low signal-to-noise sources. At the same time, the sky footprint associated with GALEX observations has not been well defined or presented in an easily usable format. Seibert et al. have constructed three catalogs of GALEX unique source measurements; namely the GALEX All-Sky Survey Source Catalog (GASC), the GALEX Medium Imaging Survey Catalog (GMSC), and the Kepler GCAT. The team's intention is that these catalogs will provide the primary reference catalog useful for matching GALEX measurements with other large surveys of the sky at other wavelengths.
DOI: 10.3886/e62128v1
title: Is the general factor of personality based on evaluative responding? Experimental manipulation of item-popularity in personality inventories

description: No summary available for this study.
DOI: 10.3886/e62131v1
title: Is the general factor of personality based on evaluative responding? Experimental manipulation of item-popularity in personality inventories

description: No summary available for this study.
DOI: 10.17909/t92p4n
title: EUVE Spectral Atlas of Stars ("EUVEATLAS")

description: A table containing EUVE (Extreme Ultraviolet Explorer Data) spectra of 94 stars selected by Craig et al. (1997). The list is roughly representative of the sample of stars by the EUVE project during its lifetime (1992-January 2001).

The EUVEATLAS contains EUVE (Extreme Ultraviolet Explorer Data) spectra of 94 stars selected by Craig et al. (1997). The list is roughly representative of the sample of stars by the EUVE project during its lifetime (1992-January 2001). These spectra were taken whenever possible with all the three bandpasses, short- (SW; 70-190 Angstroms), medium- (MW; 140-380  Angstroms), and long-wavelength (LW; 280-760 Angstroms). The spectral resolutions for these cameras are 0.5, 1, and 2 Angstroms, respectively.  The stars are organized in a table by spectral type and by subcategories within each type.  It is important to point out that the spectra in this atlas were only the best available at the time of the compilation. In some cases, longer exposures were made after the atlas was constructed (late in the mission lifetime) and are available in the HEASARC/MAST archives.
DOI: 10.17909/t93k59
title: Mosaics of the Carina Nebula ("CARINA")

description: In early February 2010, mosaic images of the Herbig-Haro 901 and 902 (hereafter just HH 901) star formation sites were obtained using both the visible (UVIS) and infrared (IR) channels of the new Wide Field camera 3 (WFC3).  The new WFC3 observations include four pointings in a 2x2 mosaic pattern, with small dithers within each pointing to fill the gaps between the two CCD chips, and allow for the rejection of cosmic rays and detector artifacts. A mosaic image was also obtained for a parallel field, using the Advanced Camera for Surveys.  In 2005, a 43-orbit investment of Hubble observing time was awarded (HST proposals 10241 and 10475), to study the Carina Nebula in the light of Hydrogen-alpha. Although these observations cover only a small central part of the entire nebula, it resulted in one of the largest contiguous ACS images ever collected. Most of the observations are part of a large mosaic, centered on the star clusters Trumpler 14 and Trumpler 16.  Many smaller nearby fields were also imaged, including the spectacular Herbig-Haro object HH666 and the nearby NGC 3324.  In 2008, the Hubble Heritage Team also obtained WFPC2 mosaic data for NGC 3324 (HST proposal 11800) with the [O III] and [S II] filters (F502N and F673N).
DOI: 10.17909/t96c7x
title: HST Time Series of gamma Cas GHRS Observations ("GHRS_GAMMACAS")

description: GHRS_GAMMACAS is an ultraviolet grayscale timeseries of difference spectra for gamma Cas in the neighborhood of the SiIV resonance lines. 

The spectral data were recorded for over 21 hours while gamma Cas was in HST's continuous viewing zone on 1996 March 14-15 using the GHRS 2 arcsecond Large Science Aperture (LSA).  The observations covered 1045 out of a total of 1280 minutes. The data were obtained at a cadence of one spectrum per second in the ACCUM mode (8100 counts per second per pixel) with the G160M grating and were later rebinned to 1 spectrum per minute. The ACCUM mode permitted only a modest resolution (30 km/s) but provided the ability to integrate fluxes unobstructed by an aperture and construct a pseudo-continuum light curve from 'non-line pixels'. The spectral range covers approximately 1382--1417 Angstroms.

Several instrumental effects had to be removed to obtain the final spectra. These effects included included fixed pattern noise artifacts from the detector, differential spacecraft velocities, and shifts of the spectrum in both detector coordinates caused by changes in the Geomagnetic field (so-called 'GIMP') as the spacecraft traced its orbit. Photometric variations 140 pixels to the red of the Si IV line complex were removed and are presented as a separate data file. Finally, a maximum-spectrum template was obtained from the spectra by submtracting the maximum flux at each pixel from each spectrum of the time series. The data shown are from difference spectra from that template in units of continuum = 1. The spectra were taken as part of a simultaneous campaign with the RXTE satellite and contemporaneously with IUE and optical observations two months earlier.
DOI: 10.17909/t9b59v
title: A Detailed Far-UV Spectral Atlas of O Main Sequence Stars ("FUVOSTARS")

description: The Far-UV Spectral Atlas of O Stars (Smith 2012) contains high resolution data in the far-UV wavelength region (defined here as the range 930-1188 Angstroms) for 25 O stars in the Galaxy and Magellanic clouds between spectral types O2 and O9.5, obtained from the MAST FUSE data archives. The star list consists of three parallel spectral type sequences, Galactic main sequence (luminosity classes III-I), Galactic supergiants, and low metallicity stars in the Small or Large Magellanic clouds.  FITS data files of 25 stars are provided, comprised of merged spectra in each of the two FUSE detector sides, each representing the spectrum sampled in the original wavelength sampling (0.075 Angstroms).  Of these stars, six spectral templates were chosen for detailed study.  The identified lines are all the photospheric and Interstellar Medium atomic and molecular features in the far-UV spectrum. These lists were compiled from line synthesis of model atmospheres appropriate to the stars' spectral types from a theoretical and empirical set of line libraries.  The atlas spectra are enhanced with respect to the data in the MAST archives, first, in that wavelength irregularities for the FUSE Side 1 and Side 2 spectra have been removed to the extent possible and corrections made for the stars' radial velocities. The spectra were then resampled to restore the wavelength zeropoints and increments of the original spectra. Second, the depressed fluxes in the FUSE 1B LiF detector segment due to the primary 'worm' have been corrected by means of the quasi-continuum fluxes in the 2A LiF segment.
DOI: 10.17909/t9fw2c
title: A Detailed Far-UV Spectral Atlas of B Main Sequence Stars ("FUVBSTARS")

description: The Far-UV Spectral Atlas of B stars (Smith 2010) contains high resolution data in the far-UV wavelength region (defined here as the range 949-1225 Angstroms) for 10 B stars near the main sequence. The spectrum for type B0 is taken, with permission from the author, from the still classic Copernicus satellite atlas of tau Scorpii (Rogerson and Upson 1977). For all other types the spectra were obtained from the MAST/FUSE data archives (Far Ultraviolet Spectroscopic Explorer) in the range 949-1188 Angstroms, and from the archives of either the HST/STIS or IUE archives for wavelengths above 1188 Angstroms.  Whenever both data sources were available the STIS spectrum was selected.  With respect to the data in the MAST archives, the altas spectra are enhanced, first, in that wavelength irregularities for the FUSE Side 1 and Side 2 spectra have been removed to the greatest extent possible and corrections made for the stars' radial velocities. The spectra were then resampled to restore the wavelength zeropoints and increments of the original spectra. Second, the depressed fluxes in the FUSE 1B LiF detector segment due to the primary 'worm' have been corrected by means of the quasi-continuum fluxes in the 2A LiF segment. Third, a star/ISM flag vector was added to the FITS files to designate those wavelengths for which the fluxes are dominated by local molecular hydrogen lines.
DOI: 10.17909/t9qc7k
title: Brightest of Reionizing Galaxies ("BORG")

description: The Brightest of Reionizing Galaxies (BoRG) observations were first obtained in HST Cycle 17 in program GO 11700 (PI: Michele Trenti) and continued in Cycle 19 with program GO 12572 (PI: Michele Trenti). BoRG is an ongoing pure-parallel program that obtains WFC3 imaging in four filters (F606W, F098M, F125W, F160W) on random sightlines at high Galactic latitudes (|b| &gt; 30 degrees). BoRG also assimilates data from the similar Hubble Infrared Pure Parallel Imaging Extragalactic Survey (HIPPIES) pure-parallel program (GO 11702; PI: Yan) as well as the coordinated parallel observations acquired as part of the Cosmic Origins Spectrograph (COS) GTO program (GO 11519, 11520, 11524, 11528, 11530, 11533, 11534, 11541, 12024, and 12025).
DOI: 10.17909/t9v30d
title: Space Telescope A901/902 Galaxy Evolution Survey ("STAGES")

description: STAGES is a a large area (~0.5x0.5 degree) survey of the complex Abell 901(a,b)/902 multiple-cluster system at z=0.165. An 80-tile imaging mosaic in F606W was conducted in Cycle 13 under GO program 10395 (PI: M. Gray).  With multiwavelength data available from COMBO-17, HST, Spitzer, XMM-Newton, GALEX, 2dF and GMRT the survey goals include simultaneously linking galaxy morphology with other observables such as age, star-formation rate, nuclear activity, and stellar mass.  The data products available at MAST include the reduced HST/ACS images for each of the 80 tiles in the F606W ACS mosaic, as well as postage stamps for all objects in the field and the complete output of GALFIT profile fitting.
DOI: 10.17909/t9zw21
title: A Hubble Space Telescope Gallery of Merging Galaxies ("MERGGAL")

description: The HST 18th anniversary press release contains a large gallery of interacting and merging galaxies. In association with this press release, seven of these objects have been made available as MAST High-Level Science Products (HLSP).  These data were originally acquired under HST programs 6276, 10592, 11091, 11092, 11095, 11956, and 11994.
DOI: 10.14457/kmitl.res.2013.35
title: การใช้สารสกัดชาเขียวเพื่อเพิ่มคุณภาพและยืดอายุ การเก็บรักษาในหมูหวาน
DOI: 10.14457/kmitl.res.2014.50
title: ปัจจัยเชิงสาเหตุที่สนับสนุนความตั้งใจของผู้ใช้ในการใช้งานฐานข้อมูลวิชาการออนไลน์ในมหาวิทยาลัย
DOI: 10.14457/kmitl.res.2014.51
title: ความแตกต่างเชิงพฤติกรรมระหว่างกลุ่มบุคคลในการซื้อสินค้าหรือใช้บริการการพาณิชย์อิเล็กทรอนิกส์
DOI: 10.17909/t95c7m
title: VLA-A Array AL218 Texas Survey Source Snapshots ("AL218")

description: The VLA-A Texas Survey consists of a sample of objects extracted in 1989 by Ray Lucas and Kenneth Chambers from the earlier Texas Interferometer 365 MHz Survey of radio sources covering a strip of sky from approximately -35.5 degrees declination to +71.5 degrees declination, and complete to flux densities of 0.25 Jy, with positional accuracies of ~1 arcsecond in RA and DEC. The Lucas and Chambers sample from 1989, which comprises the VLA-A Texas Survey is a subset of 71 sources drawn from the area of one optical Schmidt sky survey plate (covering ~6.5x6.5 degrees), Region S861, centered at approximately RA=190.640822109, DEC=-0.273834224277 (J2000), from the UK Schmidt SRC-J Survey. The Region S861 was initially chosen because it represented the combination of the deepest UK Schmidt plate material (the best optical survey material available at the time of our sample definition in 1989) and the highest galactic latitude, thereby emphasizing the extragalactic nature of the survey and also maximizing the likelihood of having more optical detections. Much more recently, the area of this plate has been covered by a number of important sky surveys including 2MASS, NRAO VLA FIRST, and the Sloan Digital Sky Survey (SDSS). In particular, the availability of the Sloan Survey data provides 5-band ugriz color information at optical wavelengths, to a depth of g,r=22.2.
DOI: 10.17909/t9959j
title: Wide Field Camera 3 Early Release Science Program

description: ~210 orbits of Director's Discretionary time to the WFC3 SOC for challenging science programs designed to test key capabilities of both the UVIS and IR channels.
DOI: 10.17909/t9dw22
title: Hubble Ultra Deep Field 2012 ("HUDF12")

description: The Hubble Ultra Deep Field 2012 program (HUDF12: Ellis et al. 2013; Koekemoer et al. 2013) is a large HST program awarded 128 orbits (HST Program ID 12498; PI: R. Ellis), designed to probe the contribution of early galaxies to cosmic reionization.  Specifically, these observations quadruple the exposure time of F105W on the UDF main field by adding 72 new orbits to data obtained previously in program ID 11563 (PI: G. Illingworth; see Bouwens et al. 2011), as well as providing 30 orbits in the completely new F140W filter, and providing an additional 26 orbits of depth in the F160W filter.
DOI: 10.17909/t9jp40
title: HST/NICMOS Paschen-alpha Survey of the Galactic Center ("HPSGC")

description: The HPSGC survey maps out a region of 2253 pc^2 (416 arcmin^2) around the central supermassive black hole (Sgr A*) in the 1.87 and 1.90 micron narrow bands with a spatial resolution of 0.01 pc (0.2 arcsec full width at half-maximum) at a distance of 8 kpc.
DOI: 10.17909/t9t596
title: FUSE Atlas Of Magellanic OB Stars ("FUSE_MAGOB")

description: This catalog serves data for 47 OB stars in the Large and Small Magellanic Clouds (see Walborn et al. 2002). This spectral atlas covers essentially the same spectral type and luminosity ranges in the FUSE_GALOB HLSP. The same observing configuration was used as for the other atlas. However, for this atlas the data have been rebinned to steps of 0.25 Angstroms. The primary difference is that the spectra are less attenuated below 1000 Angstroms by Galactic ISM and H2 extinction. The continuum is fully rectified (flat) and normalized to unity, bringing the conditioning of FUSE data to its fullest potential for immediate analysis purposes.
DOI: 10.17909/t9ww2d
title: Hubble Deep Field South ("HDF_SOUTH")

description: A second Hubble Deep Field campaign was carried out between late September and October of 1998.  The field is located in the Southern Continuous Viewing Zone.  As was the case for HDF-N, approximately 150 consecutive orbits were devoted to a single telescope pointing. Additional flanking field observations were made surrounding the deep STIS, WFPC2 and NICMOS fields.  The raw, pipeline calibrated and reprocessed data were released to the community on November 23, 1998. The rationale for undertaking a second deep field campaign followed from the wealth of information that has come out of HDF-N, and from the desire to provide a point of focus for similar studies of the distant universe from southern-hemisphere facilities. The wide public access to the HDF-N data stimulated extensive followup observations across the electromagnetic spectrum, both from major ground-based observatories and from other satellites.
DOI: 10.17909/t9xw2q
title: Cosmic Evolution Survey ("COSMOS")

description: COSMOS (P.I. Nicholas Scoville) is an HST Treasury Program to survey a two square degree equatorial field, centered on RA=10:00:28.6 and DEC=+02:12:21.0 with the ACS in the I band of the VIMOS equatorial field. Parallel observations with WFPC2 and NICMOS were also obtained. Several HST programs are associated with this project: (9822; 9999; 10092; 10337; 10702). The team has also assembled several publically available ancillary datasets including optical spectra, deep XMM and VLA imaging, ground-based optical/IR imaging, UV imaging from GALEX and IR data from SIRTF. MAST has archived the ACS, WFPC2, NICMOS and GALEX science products from the COSMOS project.
DOI: 10.17909/t90p41
title: Grism-ACS Program for Extragalactic Science ("GRAPES")

description: GRAPES is a project which was conducted in the Hubble Ultra-Deep Field (HUDF) during HST Cycle 12, over the period 2004 September to 2005 January. Sangeeta Malhotra is the PI for proposal 9793 for which 40 orbits were allocated. Slitless spectra in the Ultra-Deep Field were obtained with the Advanced Camera for Surveys (ACS) with the Wide Field Camera (WFC) over the field of 204x204 arcsec. The G800L grism provides slitless spectra with a dispersion of about 40 Angstroms per pixel.  The release constitutes 1400 1D extracted spectra from the GRAPES dataset that were selected to have i &lt; 27.0 mag.
DOI: 10.17909/t94g6z
title: STIS Next Generation Spectral Library ("STISNGSL")

description: The Next Generation Spectral Library (NGSL) consists of spectra for 374 stars, all observed in the same way, and all spectra covering the spectral range, ~0.2-1.0 microns, at a resolving power R ~1000.  As part of HST proposal AR 10659, the team worked to derive a wavelength-dependent correction to the slit throughput as a function of offset from the slit center, delivering Version 1 of the NGSL to MAST as an HLSP.  In HST proposal GO/CAL 11652, the team derived an improved slit-throughput correction based on post-SM4 observations of a standard star (BD+75D325), which was stepped across the slit.  In HST proposal AR 11755, the team incorporated the observed slit-throughput corrections in this new version of the Next Generation Spectral Library.
DOI: 10.17909/t98597
title: Catalogs of B-, V-, and i-band Dropout Sources ("DROPOUTS")

description: Beckwith et al. (2006) have prepared catalogs of dropout sources for the GOODS North, GOODS South, and the Hubble Ultra Deep fields based on the original projects source catalogs.
DOI: 10.17909/t9d01q
title: GOODS NICMOS Archival Data ("GOODSNIC")

description: As a part of the HST 10937 Archival Research proposal, PI Rychard Bouwens and colleagues retrieved and process nearly all NICMOS Camera 3 F110W and F160W data taken over the GOODS North and South fields.  All data were process using the NICMOS data reduction pipeline 'NICRED'. The NICRED pipeline includes nine processing steps from basic calibration to generating final co-added registered mosaics. Among these nine steps are procedures for successfully handling three of the most common NICMOS anomalies: electronic ghosting, the pedestal effect and cosmic-ray persistence.
DOI: 10.17909/t9hp4p
title: A Catalog and Atlas of Cataclysmic Variables ("CVCAT")

description: The Catalog and Atlas of Cataclysmic Variables (2001, PASP 113, 764) is a web-based version of the team's previously published catalogs (Downes and Shara 1993, PASP 105, 127; Downes, Webbink, and Shara 1997, PASP 109, 345). The data in this version supersedes that in the published catalogs, and contains the latest information on the objects. The catalog was frozen on February 1, 2006, and no new information will be added.
DOI: 10.17909/t9r59k
title: A Comprehensive UV Spectral Linelist of White Dwarf G191-B2B

description: A team led by Simon Preval have created one of the most complete UV linelists of a white dwarf. Co-adding over 150 spectra from both HST STIS and FUSE, the team was able to identify nearly 950 absorption lines with equivalent widths as small as a few mÅ.
DOI: 10.17909/t9s59w
title: Ultra Deep Field NICMOS-Treasury

description: Images and catalog of the Near-Infrared Camera and Multi-Object Spectrometer Ultra Deep Field (NICMOS UDF) Treasury program.
DOI: 10.17909/t9w012
title: Probing Evolution And Reionization Spectroscopically ("PEARS")

description: PEARS is an HST program that was conducted in the GOODS North and GOODS South fields using the Advanced Camera for Surveys in Cycle 14. Observations were made during the period 2005 August 8 to 2006 February 17.  Slitless spectra over both fields were obtained with the ACS Wide Field Camera (WFC) and the G800L grism over the 204x204 arcsec detector area. Short F606W images were also obtained to align to the GOODS astrometry and to provide the zero point of the slitless spectra. The G800L grism provides slitless spectra with a dispersion of about 40 Angstroms per pixel. The grism first order covers 5500-10500 Angstroms, with a peak sensitivity around 7500 Angstroms.