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1. Wide-field Survey around Local Group Dwarf Spheroidal Galaxy Leo II: Spatial Distribution of Stellar Content

Author

Komiyama, Yutaka, Doi, Mamoru, Furusawa, Hisanori, Hamabe, Masaru, Imi, Katsumi, Kimura, Masahiko, Miyazaki, Satoshi, Nakata, Fumiaki, Okada, Norio, Okamura, Sadanori, Ouchi, Masami, Sekiguchi, Maki, Shimasaku, Kazuhiro, Yagi, Masafumi, and Yasuda, Naoki

Subjects
Astrophysics
Abstract

We carried out a wide-field V, I imaging survey of the Local Group dwarf spheroidal galaxy Leo II using the Subaru Prime Focus Camera on the 8.2-m Subaru Telescope. The survey covered an area of 26.67 x 26.67 arcmin^2, far beyond the tidal radius of Leo II (8.63 arcmin), down to the limiting magnitude of V ~26, which is roughly 1 mag deeper than the turn-off point of the main sequence stars of Leo II. Radial number density profiles of bright and faint red giant branch (RGB) stars were found to change their slopes at around the tidal radius, and extend beyond the tidal radius with shallower slopes. A smoothed surface brightness map of Leo II suggests the existence of a small substructure of globular cluster luminosity beyond the tidal radius. We investigated the properties of the stellar population by means of the color-magnitude diagram. The horizontal branch (HB) morphology index shows a radial gradient in which red HB stars are more concentrated than blue HB stars, which is common to many Local Group dwarf spheroidal galaxies. The color distribution of RGB stars around the mean RGB sequence shows a larger dispersion at the center than in the outskirts, indicating a mixture of stellar populations at the center and a more homogeneous population in the outskirts. Based on the age estimation using subgiant branch (SGB) stars, we found that although the major star formation took place ~8 Gyr ago, a considerable stellar population younger than 8 Gyr is found at the center; such a younger population is insignificant in the outskirts., Comment: Accepted for publication in AJ

Published
2007
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2. Discovery of a Large Scale Clumpy Structure around the Lynx Supercluster at z~1.27

Author

Nakata, Fumiaki, Kodama, Tadayuki, Shimasaku, Kazuhiro, Doi, Mamoru, Furusawa, Hisanori, Hamabe, Masaru, Kimura, Masahiko, Komiyama, Yutaka, Miyazaki, Satoshi, Okamura, Sadanori, Ouchi, Masami, Sekiguchi, Maki, Ueda, Yoshihiro, Yagi, Masafumi, and Yasuda, Naoki

Subjects
Astrophysics
Abstract

We report the discovery of a probable large scale structure composed of many galaxy clumps around the known twin clusters at z=1.26 and z=1.27 in the Lynx region. Our analysis is based on deep, panoramic, and multi-colour imaging (26.4'x24.1') in VRi'z'-bands with the Suprime-Cam on the 8.2m Subaru telescope. This unique, deep and wide-field imaging data-set allows us for the first time to map out the galaxy distribution in the highest redshift supercluster known. We apply a photometric redshift technique to extract plausible cluster members at z~1.27 down to i'=26.15 (5sigma) corresponding to \~M*+2.5 at this redshift. From the 2-D distribution of these photometrically selected galaxies, we newly identify seven candidates of galaxy groups or clusters where the surface density of red galaxies is significantly high (>5sigma), in addition to the two known clusters. These candidates show clear red colour-magnitude sequences consistent with a passive evolution model, which suggests the existence of additional high density regions around the Lynx superclusters., Comment: 6 pages, 5 figures, accepted for publication in MNRAS

Published
2004
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3. Subaru Prime Focus Camera -- Suprime-Cam --

Author

Miyazaki, Satoshi, Komiyama, Yutaka, Sekiguchi, Maki, Okamura, Sadanori, Doi, Mamoru, Furusawa, Hisanori, Hamabe, Masaru, Imi, Katsumi, Kimura, Masahiki, Nakata, Fumiaki, Okada, Norio, Ouchi, Masami, Shimasaku, Kazuhiro, Yagi, Masafumi, and Yasuda, Naoki

Subjects
Astrophysics
Abstract

We have built an 80-mega pixels (10240 X 8192) mosaic CCD camera, called Suprime-Cam, for the wide-field prime focus of the 8.2 m Subaru telescope. Suprime-Cam covers a field of view 34' X 27', a unique facility among the the 8-10 m class telescopes, with a resolution of 0.''202 per pixel. The focal plane consists of ten high-resistivity 2k X 4k CCDs developed by MIT Lincoln Laboratory, which are cooled by a large stirling-cycle cooler. The CCD readout electronics was designed to be scalable, which allows the multiple read-out of tens of CCDs. It takes 50 seconds to readout entire arrays. We designed a filter-exchange mechanism of the jukebox type that can hold up to ten large filters (205 X 170 X 15 mm^3). The wide-field corrector is basically a three-lens Wynne-type, but has a new type of atmospheric dispersion corrector. The corrector provides a flat focal plane and an un-vignetted field of view of 30' in diameter. The achieved co-planarity of the focal array mosaic is smaller than 30 micron peak-to-peak, which realizes mostly the seeing limited image over the entire field. The median seeing in the Ic-band, measured over one year and a half, is 0.''61. The PSF anisotropy in Suprime-Cam images, estimated by stellar ellipticities, is about 2% under this median seeing condition. At the time of commissioning, Suprime-Cam had the largest survey speed, which is defined as the field of view multiplied by the primary mirror area of the telescope, among those cameras built for sub-arcsecond imaging., Comment: 22 pages, 26 figures, accepted for publication in PASJ, minor corrections, for a higher resolution ps file, see http://anela.mtk.nao.ac.jp/outgoing/suppaper/suprime.ver1.ps.gz (1.6MB)

Published
2002
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4. A Search for Lyman alpha Emitters at Redshift 3.7

Author

Fujita, Shinobu S., Ajiki, Masaru, Shioya, Yasuhiro, Nagao, Tohru, Murayama, Takashi, Taniguchi, Yoshiaki, Okamura, Sadanori, Ouchi, Masami, Shimasaku, Kazuhiro, Doi, Mamoru, Furusawa, Hisanori, Hamabe, Masaru, Kimura, Masahiko, Komiyama, Yutaka, Miyazaki, Masayuki, Miyazaki, Satoshi, Nakata, Fumiaki, Sekiguchi, Maki, Yagi, Masafumi, Yasuda, Naoki, Matsuda, Yuichi, Tamura, Hajime, Hayashino, Tomoki, Kodaira, Keiichi, Karoji, Hiroshi, Yamada, Toru, Ohta, Kouji, and Umemura, Masayuki

Subjects
Astrophysics
Abstract

We present the results of a survey for emission-line objects based on optical intermediate-band ($\lambda_{\rm c}$ = 5736 \AA ~ and $\Delta\lambda$ = 280 \AA) and broad-band ($B$, $V$, $R$, and $i^\prime$) observations of the Subaru/XMM-Newton Deep Field on the 8.2 m Subaru telescope with the Subaru Prime Focus Camera, Suprime-Cam. All the data were obtained during the guaranteed time observations of the Suprime-Cam instrument. The intermediate-band image covered a sky area with 10\minpoint62 $\times 12\minpoint40 \approx 132$ arcmin$^2$ in the Subaru/XMM-Newton Deep Field (Ouchi et al.). Using this image, we have found 23 emission-line sources whose observed emission-line equivalent widths are greater than 250 \AA. Their optical multicolor properties indicate that six emission-line sources are Ly$\alpha$ emitters at $z \approx$ 3.7 ($\Delta z \approx 0.22$). They are either intense starburst galaxies or active galactic nuclei like quasars at $z \approx$ 3.7. Two more emission-line sources may also be Ly$\alpha$ emitters at $z \approx$ 3.7 although their multicolor properties are marginal. Among the remaining 15 emission-line objects, eight objects appear strong emission-line galaxies at lower redshift; e.g., [O {\sc ii}] $\lambda$3727 emitters at $z \approx 0.54$, H$\beta$ at $z \approx 0.18$, or [O {\sc iii}]$\lambda$5007 emitters at $z \approx 0.15$. The remaining seven objects are unclassified because they are too faint to be detected in broad-band images. We discuss observational properties of these strong emission-line sources. In particular, our data allow us to estimate the star formation density at $z \approx 3.7$ for the first time., Comment: Accepted for publication in AJ;14 pages, 26 figures (all figures are JPEG file)

Published
2002
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5. Galaxy Population in a Cluster of Galaxies around the Radio Galaxy 3C 324 at z=1.2

Author

Nakata, Fumiaki, Kajisawa, Masaru, Yamada, Toru, Kodama, Tadayuki, Shimasaku, Kazuhiro, Tanaka, Ichi, Doi, Mamoru, Furusawa, Hisanori, Hamabe, Masaru, Iye, Masanori, Kimura, Masahiko, Komiyama, Yutaka, Miyazaki, Satoshi, Okamura, Sadanori, Ouchi, Masami, Sasaki, Toshiyuki, Sekiguchi, Maki, Yagi, Masafumi, and Yasuda, Naoki

Subjects
Astrophysics
Abstract

We discuss the properties of galaxies around the radio galaxy 3C 324 at z=1.2 based on BVRIK' multi-band imaging data. We have applied a photometric-redshift technique to objects in the 3C 324 field, and identified 35 objects as plausible cluster members. We have found that red and luminous members are concentrated in a small region enclosed by a circle of 40" radius (0.33 Mpc at z=1.2 for \Omega_0=0.3, \lambda_0=0.7, H_0=70km/s/Mpc cosmology) from the 3C 324 galaxy. The 3C 324 cluster is probably much more compact in size compared with the local clusters. We constructed a K'-band luminosity function of the cluster members and fit a Schechter function, and found the characteristic magnitude to be K*_{AB}=20.2+-0.6. This value is consistent with the extrapolation of the pure passive evolution seen for z<1 clusters. We have identified eight bright galaxies which form a red color-magnitude sequence. The slope of the sequence is consistent with the passive evolution model down to K'_{AB}<22; we also found that there is no clear age variation in these bright red galaxies. However, seven out of these eight galaxies exhibit a significant excess in the rest UV light with respect to the passive evolution model. This may suggest that the massive early-type galaxies in this high-redshift cluster are still forming stars to some extent. We have confirmed a truncation of the color-magnitude sequence at K'_{AB}\sim22; faint passively-evolving galaxies may not yet be present in this cluster at z\sim1.2. The overall color distribution of the cluster members, selected by the photometric redshift technique, is found to be very broad. We derived the fraction of blue galaxies in this cluster following a, Comment: 16 pages, 14 figures, PASJ accepted

Published
2001
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6. Discovery of Very Extended Emission-Line Region around the Seyfert 2 Galaxy NGC 4388

Author

Yoshida, Michitoshi, Yagi, Masafumi, Okamura, Sadanori, Aoki, Kentaro, Ohyama, Youichi, Komiyama, Yutaka, Yasuda, Naoki, Iye, Masanori, Kashikawa, Nobunari, Doi, Mamoru, Furusawa, Hisanori, Hamabe, Masaru, Kimura, Masahiko, Miyazaki, Masayuki, Miyazaki, Satoshi, Nakata, Fumiaki, Ouchi, Masami, Sekiguchi, Maki, Shimasaku, Kazuhiro, and Ohtani, Hiroshi

Subjects
Astrophysics
Abstract

We found a very large, 35 kpc, emission-line region around the Seyfert type 2 galaxy NGC 4388, using deep narrow-band imaging with the prime focus camera (Suprime-Cam) of the Subaru telescope. This region consists of many faint gas clouds or filaments, and extends northeastwards from the galaxy. The typical H-alpha luminosity L(H-alpha) of the clouds is 10^37 erg s^-1, and the total L(H-alpha) of the region within 10 kpc from the nucleus is 2 x 10^38 erg s^-1, which corresponds to an ionized gas mass of 10^5 M_solar. The map of the emission-line intensity ratio I([OIII])/I(H-alpha) indicates that the inner (r < 12 kpc) region of the VEELR may be excited by nuclear ionizing radiation. The excitation mechanism of the outer (r > 12 kpc) region is unclear, but it is likely that the nuclear radiation is also a dominant source of its ionization. We discuss the origin of the ionized gas. Two plausible origins of the gas in the VEELR are (i) the tidal debris resulting from a past interaction with a gas-rich dwarf galaxy, i.e., a minor merger, or (ii) the interstellar medium of NGC 4388, stripped by the ram pressure of the hot intracluster medium of the Virgo cluster., Comment: 15 pages, 7 figures, ApJ accepted

Published
2001
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7. Statistical Properties of Lyman Break Galaxies at z~4

Author

Ouchi, Masami, Shimasaku, Kazuhiro, Okamura, Sadanori, Doi, Mamoru, Furusawa, Hisanori, Hamabe, Masaru, Kimura, Masahiko, Komiyama, Yutaka, Miyazaki, Masayuki, Miyazaki, Satoshi, Nakata, Fumiaki, Sekiguchi, Maki, Yagi, Masafumi, and Yasuda, Naoki

Subjects
Astrophysics
Abstract

We study the luminosity function and the correlation function of about 1200 z~4 Lyman break galaxies (LBGs) with i'<26 that are photometrically selected from deep BRi' imaging data of a 618 arcmin^2 area in the Subaru/XMM-Newton Deep Field taken with Subaru Prime Focus Camera. The contamination and completeness of our LBG sample are evaluated, on the basis of the Hubble Deep Field-North (HDF-N) objects, to be 17% and 45%, respectively. We derive the UV (rest 1700A) luminosity functions (LFs) and find a large population of UV-luminous galaxies at z~4. The LFs of the red and blue subsamples imply that the bright LBGs are redder in the UV continuum than the average color of the LBGs. Then we calculate the correlation function over theta = 2''-1000'' and find that it is fitted fairly well by a power law, omega(theta)=A_omega theta^(-0.8), with A_omega=0.71 +/- 0.26. We estimate the correlation length r_0 (in comoving units) of the two-point spatial correlation function xi(r) = (r/r_0)^(-1.8) to be r_0=2.7 +0.5/-0.6 h^(-1) Mpc (Omega_m=0.3 and Omega_Lambda=0.7). The correlation function shows an excess of omega (theta) on small scales (theta < 5''), departing from the power-law fit at > 3 sigma significance level. Interpreting this as being due to galaxy mergers, we evaluate the fraction of galaxies undergoing mergers to be 3.0 +/- 0.9%, which is significantly smaller than those of galaxies at intermediate redshifts., Comment: To appear in the proceedings of the Marseille 2001 conference "Where is the Matter? Tracing Dark and Bright Matter with the New Generation of Large-Scale Surveys", 25-29 June 2001, Marseille (France)

Published
2001

8. Clustering Properties of Galaxies at z~4 in the Subaru/XMM Deep Survey Field

Author

Ouchi, Masami, Shimasaku, Kazuhiro, Okamura, Sadanori, Doi, Mamoru, Furusawa, Hisanori, Hamabe, Masaru, Kimura, Masahiko, Komiyama, Yutaka, Miyazaki, Masayuki, Miyazaki, Satoshi, Nakata, Fumiaki, Sekiguchi, Maki, Yagi, Masafumi, and Yasuda, Naoki

Subjects
Astrophysics
Abstract

We study the clustering properties of about 1200 z~4 Lyman Break Galaxy (LBG) candidates with i'<26 which are selected by color from deep BRi' imaging data of a 618 arcmin^2 area in the Subaru/XMM-Newton Deep Field taken with Subaru Prime Focus Camera. The contamination and completeness of our LBG sample are evaluated, on the basis of the Hubble Deep Field North (HDFN) objects, to be 17% and 45%, respectively. We derive the angular correlation function over theta = 2''-1000'', and find that it is fitted fairly well by a power law, omega(theta)=A_omega theta^{-0.8}, with A_omega = 0.71 +/- 0.26. We then calculate the correlation length r0 (in comoving units) of the two-point spatial correlation function xi(r) = (r/r0)^{-1.8} from A_omega using the redshift distribution of LBGs derived from the HDFN, and find r0=2.7 (+0.5/-0.6) h^{-1} Mpc in a Lambda-dominated universe (Omega_m=0.3 and Omega_Lambda=0.7). This is twice larger than the correlation length of the dark matter at z~4 predicted from an analytic model by Peacock & Dodds but about twice smaller than that of bright galaxies predicted by a semi-analytic model of Baugh et al. We find an excess of omega(theta) on small scales (theta < 5'') departing from the power law fit over 3 sigma significance levels. Interpreting this as due to galaxy mergers, we estimate the fraction of galaxies undergoing mergers in our LBG sample to be 3.0 +/- 0.9%, which is significantly smaller than those of galaxies at intermediate redshifts., Comment: 9 pages, 4 figures, to be published in ApJ Letters

Published
2001
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10. Development of Learning Materials for Experiencing Astronomical Spectral Analysis. In cases of identifying solar absorption lines and measurements of galactic rotational velocitiesd

Author

ITOH, Nobunari, YAMAGATA, Tomohiko, HAMABE, Masaru, and NISHIURA, Shingo

Abstract

Astronomical learning materials in which spectral data are dealt with were developed to provide high school students opportunities to learn astronomy. Two kinds of astronomical topics, elemental identification of solar absorption lines and rotational velocity measurements of spiral galaxies, were selected as material subjects. Each material contains spectral data and spreadsheets and macro commands are built into spreadsheets to reduce analytical work burden. An astronomical image processing software, Makali`i, is adopted as a default image processor. To evaluate the efficiency of the learning materials, the trial practice of the materials were carried out. As a result, the materials got favorable response from over 80% of experimental participants. On the other hand, it is found that considerable fraction of participants felt difficulty to understand the material contents.

Published
2017

13. The Third Data Release of the Sloan Digital Sky Survey

Author

Abazajian, Kevork, Adelman-McCarthy, Jennifer K., Agüeros, Marcel Andre, Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, Bahcall, Neta A., Baldry, Ivan K., Bastian, Steven, Berlind, Andreas, Bernardi, Mariangela, Blanton, Michael R., Bochanski, John J., Boroski, William N., Brewington, Howard J., Briggs, John W., Brinkmann, J., Brunner, Robert J., Budavári, Tamás, Carey, Larry N., Castander, Francisco J., Connolly, A. J., Covey, Kevin R., Csabai, István, Dalcanton, Julianne J., Doi, Mamoru, Dong, Feng, Eisenstein, Daniel J., Evans, Michael L., Fan, Xiaohui, Finkbeiner, Douglas P., Friedman, Scott D., Frieman, Joshua A., Fukugita, Masataka, Gillespie, Bruce, Glazebrook, Karl, Gray, Jim, Grebel, Eva K., Gunn, James E., Gurbani, Vijay K., Hall, Patrick B., Hamabe, Masaru, Harris, Frederick H., Harris, Hugh C., Harvanek, Michael, Heckman, Timothy M., Hendry, John S., Hennessy, Gregory S., Hindsley, Robert B., Hogan, Craig J., Hogg, David W., Holmgren, Donald J., Holtzman, Jon A., Ichikawa, Shin-Ichi, Ichikawa, Takashi, Ivezić, Željko, Jester, Sebastian, Johnston, David E., Jorgensen, Anders M., Jurić, Mario, Kent, Stephen M., Kleinman, S. J., Knapp, G. R., Kniazev, Alexei Yu., Kron, Richard G., Krzesiński, Jurek, Lamb, Donald Q., Lampeitl, Hubert, Lee, Brian C., Lin, Huan, Long, Daniel C., Loveday, Jon, Lupton, Robert H., Mannery, Ed, Margon, Bruce, Martínez-Delgado, David, Matsubara, Takahiko, McGehee, Peregrine M., McKay, Timothy A., Meiksin, Avery, Ménard, Brice, Munn, Jeffrey A., Nash, Thomas, Neilsen, Eric H., Newberg, Heidi Jo, Newman, Peter R., Nichol, Robert C., Nicinski, Tom, Nieto-Santisteban, Maria, Nitta, Atsuko, Okamura, Sadanori, O'Mullane, William, Owen, Russell, Padmanabhan, Nikhil, Pauls, George, Peoples, John, Pier, Jeffrey R., Pope, Adrian C., Pourbaix, Dimitri, Quinn, Thomas R., Raddick, M. Jordan, Richards, Gordon T., Richmond, Michael W., Rix, Hans-Walter, Rockosi, Constance M., Schlegel, David J., Schneider, Donald P., Schroeder, Joshua, Scranton, Ryan, Sekiguchi, Maki, Sheldon, Erin, Shimasaku, Kazu, Silvestri, Nicole M., Smith, J. Allyn, Smolčić, Vernesa, Snedden, Stephanie A., Stebbins, Albert, Stoughton, Chris, Strauss, Michael A., SubbaRao, Mark, Szalay, Alexander S., Szapudi, István, Szkody, Paula, Szokoly, Gyula P., Tegmark, Max, Teodoro, Luis, Thaka, Aniruddha R., Tremonti, Christy, Tucker, Douglas L., Uomoto, Alan, Vanden Berk, Daniel E., Vandenberg, Jan, Vogeley, Michael S., Voges, Wolfgang, Vogt, Nicole P., Walkowicz, Lucianne M., Wang, Shu-I, Weinberg, David H., West, Andrew A., White, Simon D. M., Wilhite, Brian C., Xu, Yongzhong, Yanny, Brian, Yasuda, Naoki, Yip, Ching-Wa, Yocum, D. R., York, Donald G., Zehavi, Idit, Zibetti, Stefano, and Zucker, Daniel B.

Subjects
Imaging systems in astronomy, Stars--Observations, Astronomy, Astrophysics
Abstract

This paper describes the Third Data Release of the Sloan Digital Sky Survey (SDSS). This release, containing data taken up through 2003 June, includes imaging data in five bands over 5282 deg², photometric and astrometric catalogs of the 141 million objects detected in these imaging data, and spectra of 528,640 objects selected over 4188 deg². The pipelines analyzing both images and spectroscopy are unchanged from those used in our Second Data Release.

Published
2005
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14. The Second Data Release of the Sloan Digital Sky Survey

Author

Abazajian, Kevork, Adelman-McCarthy, Jennifer K., Agüeros, Marcel Andre, Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, Bahcall, Neta A., Baldry, Ivan K., Bastian, Steven, Berlind, Andreas, Bernardi, Mariangela, Blanton, Michael R., Bochanski, John J., Boroski, William N., Briggs, John W., Brinkmann, J., Brunner, Robert J., Budavári, Tamás, Carey, Larry N., Carliles, Samuel, Castander, Francisco J., Connolly, A. J., Csabai, István, Doi, Mamoru, Dong, Feng, Eisenstein, Daniel J., Evans, Michael L., Fan, Xiaohui, Finkbeiner, Douglas P., Friedman, Scott D., Frieman, Joshua A., Fukugita, Masataka, Gal, Roy R., Gillespie, Bruce, Glazebrook, Karl, Gray, Jim, Grebel, Eva K., Gunn, James E., Gurbani, Vijay K., Hall, Patrick B., Hamabe, Masaru, Harris, Frederick H., Harris, Hugh C., Harvanek, Michael, Heckman, Timothy M., Hendry, John S., Hennessy, Gregory S., Hindsley, Robert B., Hogan, Craig J., Hogg, David W., Holmgren, Donald J., Ichikawa, Shin-Ichi, Ichikawa, Takashi, Ivezić, Željko, Jester, Sebastian, Johnston, David E., Jorgensen, Anders M., Kent, Stephen M., Kleinman, S. J., Knapp, G. R., Kniazev, Alexei Yu., Kron, Richard G., Krzesiński, Jurek, Kunszt, Peter Z., Kuropatkin, Nickolai, Lamb, Donald Q., Lampeitl, Hubert, Lee, Brian C., Leger, R. French, Li, Nolan, Lin, Huan, Loh, Yeong-Shang, Long, Daniel C., Loveday, Jon, Lupton, Robert H., Malik, Tanu, Margon, Bruce, Matsubara, Takahiko, McGehee, Peregrine M., McKay, Timothy A., Meiksin, Avery, Munn, Jeffrey A., Nakajima, Reiko, Nash, Thomas, Neilsen, Eric H., Newberg, Heidi Jo, Newman, Peter R., Nichol, Robert C., Nicinski, Tom, Nieto-Santisteban, Maria, Nitta, Atsuko, Okamura, Sadanori, O'Mullane, William, Ostriker, Jeremiah P., Owen, Russell, Padmanabhan, Nikhil, Peoples, John, Pier, Jeffrey R., Pope, Adrian C., Quinn, Thomas R., Richards, Gordon T., Richmond, Michael W., Rix, Hans-Walter, Rockosi, Constance M., Schlegel, David J., Schneider, Donald P., Scranton, Ryan, Sekiguchi, Maki, Seljak, Uroš, Sergey, Gary, Sesar, Branimir, Sheldon, Erin, Shimasaku, Kazu, Siegmund, Walter A., Silvestri, Nicole M., Sirko, Edwin, Smith, J. Allyn, Smolčić, Vernesa, Snedden, Stephanie A., Stebbins, Albert, Stoughton, Chris, Strauss, Michael A., SubbaRao, Mark, Szalay, Alexander S., Szapudi, István, Szkody, Paula, Szokoly, Gyula P., Tegmark, Max, Teodoro, Luis, Thaka, Aniruddha R., Tremonti, Christy, Tucker, Douglas L., Uomoto, Alan, Vanden Berk, Daniel E., Vandenberg, Jan, Vogeley, Michael S., Voges, Wolfgang, Vogt, Nicole P., Walkowicz, Lucianne M., Wang, Shu-I, Weinberg, David H., West, Andrew A., White, Simon D. M., Wilhite, Brian C., Xu, Yongzhong, Yanny, Brian, Yasuda, Naoki, Yip, Ching-Wa, Yocum, D. R., York, Donald G., Zehavi, Idit, Zibetti, Stefano, and Zucker, Daniel B.

Subjects
Imaging systems in astronomy, Stars--Observations, Astronomy, Astrophysics
Abstract

The Sloan Digital Sky Survey (SDSS) has validated and made publicly available its Second Data Release. This data release consists of 3324 deg² of five-band (ugriz) imaging data with photometry for over 88 million unique objects, 367,360 spectra of galaxies, quasars, stars, and calibrating blank sky patches selected over 2627 deg² of this area, and tables of measured parameters from these data. The imaging data reach a depth of r ≈ 22.2 (95% completeness limit for point sources) and are photometrically and astrometrically calibrated to 2% rms and 100 mas rms per coordinate, respectively. The imaging data have all been processed through a new version of the SDSS imaging pipeline, in which the most important improvement since the last data release is fixing an error in the model fits to each object. The result is that model magnitudes are now a good proxy for point-spread function magnitudes for point sources, and Petrosian magnitudes for extended sources. The spectroscopy extends from 3800 to 9200 Å at a resolution of 2000. The spectroscopic software now repairs a systematic error in the radial velocities of certain types of stars and has substantially improved spectrophotometry. All data included in the SDSS Early Data Release and First Data Release are reprocessed with the improved pipelines and included in the Second Data Release. Further characteristics of the data are described, as are the data products themselves and the tools for accessing them.

Published
2004
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15. Wide-Field Survey around Local Group Dwarf Spheroidal Galaxy Leo II: Spatial Distribution of Stellar Content

Author

Komiyama, Yutaka, primary, Doi, Mamoru, additional, Furusawa, Hisanori, additional, Hamabe, Masaru, additional, Imi, Katsumi, additional, Kimura, Masahiko, additional, Miyazaki, Satoshi, additional, Nakata, Fumiaki, additional, Okada, Norio, additional, Okamura, Sadanori, additional, Ouchi, Masami, additional, Sekiguchi, Maki, additional, Shimasaku, Kazuhiro, additional, Yagi, Masafumi, additional, and Yasuda, Naoki, additional

Published
2007
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17. The Third Data Release of the Sloan Digital Sky Survey

Author

Abazajian, Kevork, primary, Adelman-McCarthy, Jennifer K., additional, Agüeros, Marcel A., additional, Allam, Sahar S., additional, Anderson, Kurt S. J., additional, Anderson, Scott F., additional, Annis, James, additional, Bahcall, Neta A., additional, Baldry, Ivan K., additional, Bastian, Steven, additional, Berlind, Andreas, additional, Bernardi, Mariangela, additional, Blanton, Michael R., additional, Bochanski, Jr., John J., additional, Boroski, William N., additional, Brewington, Howard J., additional, Briggs, John W., additional, Brinkmann, J., additional, Brunner, Robert J., additional, Budavári, Tamás, additional, Carey, Larry N., additional, Castander, Francisco J., additional, Connolly, A. J., additional, Covey, Kevin R., additional, Csabai, István, additional, Dalcanton, Julianne J., additional, Doi, Mamoru, additional, Dong, Feng, additional, Eisenstein, Daniel J., additional, Evans, Michael L., additional, Fan, Xiaohui, additional, Finkbeiner, Douglas P., additional, Friedman, Scott D., additional, Frieman, Joshua A., additional, Fukugita, Masataka, additional, Gillespie, Bruce, additional, Glazebrook, Karl, additional, Gray, Jim, additional, Grebel, Eva K., additional, Gunn, James E., additional, Gurbani, Vijay K., additional, Hall, Patrick B., additional, Hamabe, Masaru, additional, Harbeck, Daniel, additional, Harris, Frederick H., additional, Harris, Hugh C., additional, Harvanek, Michael, additional, Hawley, Suzanne L., additional, Hayes, Jeffrey, additional, Heckman, Timothy M., additional, Hendry, John S., additional, Hennessy, Gregory S., additional, Hindsley, Robert B., additional, Hogan, Craig J., additional, Hogg, David W., additional, Holmgren, Donald J., additional, Holtzman, Jon A., additional, Ichikawa, Shin-ichi, additional, Ichikawa, Takashi, additional, Ivezić, Željko, additional, Jester, Sebastian, additional, Johnston, David E., additional, Jorgensen, Anders M., additional, Jurić, Mario, additional, Kent, Stephen M., additional, Kleinman, S. J., additional, Knapp, G. R., additional, Kniazev, Alexei Yu., additional, Kron, Richard G., additional, Krzesinski, Jurek, additional, Lamb, Donald Q., additional, Lampeitl, Hubert, additional, Lee, Brian C., additional, Lin, Huan, additional, Long, Daniel C., additional, Loveday, Jon, additional, Lupton, Robert H., additional, Mannery, Ed, additional, Margon, Bruce, additional, Martínez-Delgado, David, additional, Matsubara, Takahiko, additional, McGehee, Peregrine M., additional, McKay, Timothy A., additional, Meiksin, Avery, additional, Ménard, Brice, additional, Munn, Jeffrey A., additional, Nash, Thomas, additional, Neilsen, Jr., Eric H., additional, Newberg, Heidi Jo, additional, Newman, Peter R., additional, Nichol, Robert C., additional, Nicinski, Tom, additional, Nieto-Santisteban, Maria, additional, Nitta, Atsuko, additional, Okamura, Sadanori, additional, O'Mullane, William, additional, Owen, Russell, additional, Padmanabhan, Nikhil, additional, Pauls, George, additional, Peoples, John, additional, Pier, Jeffrey R., additional, Pope, Adrian C., additional, Pourbaix, Dimitri, additional, Quinn, Thomas R., additional, Raddick, M. Jordan, additional, Richards, Gordon T., additional, Richmond, Michael W., additional, Rix, Hans-Walter, additional, Rockosi, Constance M., additional, Schlegel, David J., additional, Schneider, Donald P., additional, Schroeder, Joshua, additional, Scranton, Ryan, additional, Sekiguchi, Maki, additional, Sheldon, Erin, additional, Shimasaku, Kazu, additional, Silvestri, Nicole M., additional, Smith, J. Allyn, additional, Smolčić, Vernesa, additional, Snedden, Stephanie A., additional, Stebbins, Albert, additional, Stoughton, Chris, additional, Strauss, Michael A., additional, SubbaRao, Mark, additional, Szalay, Alexander S., additional, Szapudi, István, additional, Szkody, Paula, additional, Szokoly, Gyula P., additional, Tegmark, Max, additional, Teodoro, Luis, additional, Thakar, Aniruddha R., additional, Tremonti, Christy, additional, Tucker, Douglas L., additional, Uomoto, Alan, additional, Vanden Berk, Daniel E., additional, Vandenberg, Jan, additional, Vogeley, Michael S., additional, Voges, Wolfgang, additional, Vogt, Nicole P., additional, Walkowicz, Lucianne M., additional, Wang, Shu-i, additional, Weinberg, David H., additional, West, Andrew A., additional, White, Simon D. M., additional, Wilhite, Brian C., additional, Xu, Yongzhong, additional, Yanny, Brian, additional, Yasuda, Naoki, additional, Yip, Ching-Wa, additional, Yocum, D. R., additional, York, Donald G., additional, Zehavi, Idit, additional, Zibetti, Stefano, additional, and Zucker, Daniel B., additional

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2005
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18. Subaru Deep Survey. V. A Census of Lyman Break Galaxies atz ≃ 4 and 5 in the Subaru Deep Fields: Photometric Properties

Author

Ouchi, Masami, primary, Shimasaku, Kazuhiro, additional, Okamura, Sadanori, additional, Furusawa, Hisanori, additional, Kashikawa, Nobunari, additional, Ota, Kazuaki, additional, Doi, Mamoru, additional, Hamabe, Masaru, additional, Kimura, Masahiko, additional, Komiyama, Yutaka, additional, Miyazaki, Masayuki, additional, Miyazaki, Satoshi, additional, Nakata, Fumiaki, additional, Sekiguchi, Maki, additional, Yagi, Masafumi, additional, and Yasuda, Naoki, additional

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2004
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19. Subaru Deep Survey. VI. A Census of Lyman Break Galaxies atz ≃ 4 and 5 in the Subaru Deep Fields: Clustering Properties

Author

Ouchi, Masami, primary, Shimasaku, Kazuhiro, additional, Okamura, Sadanori, additional, Furusawa, Hisanori, additional, Kashikawa, Nobunari, additional, Ota, Kazuaki, additional, Doi, Mamoru, additional, Hamabe, Masaru, additional, Kimura, Masahiko, additional, Komiyama, Yutaka, additional, Miyazaki, Masayuki, additional, Miyazaki, Satoshi, additional, Nakata, Fumiaki, additional, Sekiguchi, Maki, additional, Yagi, Masafumi, additional, and Yasuda, Naoki, additional

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2004
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20. The Second Data Release of the Sloan Digital Sky Survey

Author

Abazajian, Kevork, primary, Adelman-McCarthy, Jennifer K., additional, Agüeros, Marcel A., additional, Allam, Sahar S., additional, Anderson, Kurt, S. J., additional, Anderson, Scott F., additional, Annis, James, additional, Bahcall, Neta A., additional, Baldry, Ivan K., additional, Bastian, Steven, additional, Berlind, Andreas, additional, Bernardi, Mariangela, additional, Blanton, Michael R., additional, Bochanski, Jr., John J., additional, Boroski, William N., additional, Briggs, John W., additional, Brinkmann, J., additional, Brunner, Robert J., additional, Budavári, Tamás, additional, Carey, Larry N., additional, Carliles, Samuel, additional, Castander, Francisco J., additional, Connolly, A. J., additional, Csabai, István, additional, Doi, Mamoru, additional, Dong, Feng, additional, Eisenstein, Daniel J., additional, Evans, Michael L., additional, Fan, Xiaohui, additional, Finkbeiner, Douglas P., additional, Friedman, Scott D., additional, Frieman, Joshua A., additional, Fukugita, Masataka, additional, Gal, Roy R., additional, Gillespie, Bruce, additional, Glazebrook, Karl, additional, Gray, Jim, additional, Grebel, Eva K., additional, Gunn, James E., additional, Gurbani, Vijay K., additional, Hall, Patrick B., additional, Hamabe, Masaru, additional, Harris, Frederick H., additional, Harris, Hugh C., additional, Harvanek, Michael, additional, Heckman, Timothy M., additional, Hendry, John S., additional, Hennessy, Gregory S., additional, Hindsley, Robert B., additional, Hogan, Craig J., additional, Hogg, David W., additional, Holmgren, Donald J., additional, Ichikawa, Shin-ichi, additional, Ichikawa, Takashi, additional, Ivezić, Željko, additional, Jester, Sebastian, additional, Johnston, David E., additional, Jorgensen, Anders M., additional, Kent, Stephen M., additional, Kleinman, S. J., additional, Knapp, G. R., additional, Kniazev, Alexei Yu., additional, Kron, Richard G., additional, Krzesinski, Jurek, additional, Kunszt, Peter Z., additional, Kuropatkin, Nickolai, additional, Lamb, Donald Q., additional, Lampeitl, Hubert, additional, Lee, Brian C., additional, Leger, R. French, additional, Li, Nolan, additional, Lin, Huan, additional, Loh, Yeong-Shang, additional, Long, Daniel C., additional, Loveday, Jon, additional, Lupton, Robert H., additional, Malik, Tanu, additional, Margon, Bruce, additional, Matsubara, Takahiko, additional, McGehee, Peregrine M., additional, McKay, Timothy A., additional, Meiksin, Avery, additional, Munn, Jeffrey A., additional, Nakajima, Reiko, additional, Nash, Thomas, additional, Neilsen, Jr., Eric H., additional, Newberg, Heidi Jo, additional, Newman, Peter R., additional, Nichol, Robert C., additional, Nicinski, Tom, additional, Nieto-Santisteban, Maria, additional, Nitta, Atsuko, additional, Okamura, Sadanori, additional, O'Mullane, William, additional, Ostriker, Jeremiah P., additional, Owen, Russell, additional, Padmanabhan, Nikhil, additional, Peoples, John, additional, Pier, Jeffrey R., additional, Pope, Adrian C., additional, Quinn, Thomas R., additional, Richards, Gordon T., additional, Richmond, Michael W., additional, Rix, Hans-Walter, additional, Rockosi, Constance M., additional, Schlegel, David J., additional, Schneider, Donald P., additional, Scranton, Ryan, additional, Sekiguchi, Maki, additional, Seljak, Uros, additional, Sergey, Gary, additional, Sesar, Branimir, additional, Sheldon, Erin, additional, Shimasaku, Kazu, additional, Siegmund, Walter A., additional, Silvestri, Nicole M., additional, Smith, J. Allyn, additional, Smolčić, Vernesa, additional, Snedden, Stephanie A., additional, Stebbins, Albert, additional, Stoughton, Chris, additional, Strauss, Michael A., additional, SubbaRao, Mark, additional, Szalay, Alexander S., additional, Szapudi, István, additional, Szkody, Paula, additional, Szokoly, Gyula P., additional, Tegmark, Max, additional, Teodoro, Luis, additional, Thakar, Aniruddha R., additional, Tremonti, Christy, additional, Tucker, Douglas L., additional, Uomoto, Alan, additional, Vanden Berk, Daniel E., additional, Vandenberg, Jan, additional, Vogeley, Michael S., additional, Voges, Wolfgang, additional, Vogt, Nicole P., additional, Walkowicz, Lucianne M., additional, Wang, Shu-i, additional, Weinberg, David H., additional, West, Andrew A., additional, White, Simon D. M., additional, Wilhite, Brian C., additional, Xu, Yongzhong, additional, Yanny, Brian, additional, Yasuda, Naoki, additional, Yip, Ching-Wa, additional, Yocum, D. R., additional, York, Donald G., additional, Zehavi, Idit, additional, Zibetti, Stefano, additional, and Zucker, Daniel B., additional

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2004
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21. Erratum: "Subaru Deep Spectroscopy of the Very Extended Emission-Line Region of NGC 4388: Ram Pressure Stripped Gas Ionized by Nuclear Radiation" [[URL ADDRESS="/cgi-bin/resolve?2004AJ....127...90Y" STATUS="OKAY"]Astron. J.127, 90 (2004)[/URL]]

Author

Yoshida, Michitoshi, primary, Ohyama, Youichi, additional, Iye, Masanori, additional, Aoki, Kentaro, additional, Kashikawa, Nobunari, additional, Sasaki, Toshiyuki, additional, Shimasaku, Kazuhiro, additional, Yagi, Masafumi, additional, Okamura, Sadanori, additional, Doi, Mamoru, additional, Furusawa, Hisanori, additional, Hamabe, Masaru, additional, Kimura, Masahiko, additional, Komiyama, Yutaka, additional, Miyazaki, Masayuki, additional, Miyazaki, Satoshi, additional, Nakata, Fumiaki, additional, Ouchi, Masami, additional, Sekiguchi, Maki, additional, and Yasuda, Naoki, additional

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2004
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22. Subaru Deep Spectroscopy of the Very Extended Emission-Line Region of NGC 4388: Ram Pressure Stripped Gas Ionized by Nuclear Radiation

Author

Yoshida, Michitoshi, primary, Ohyama, Youichi, additional, Iye, Masanori, additional, Aoki, Kentaro, additional, Kashikawa, Nobunari, additional, Sasaki, Toshiyuki, additional, Shimasaku, Kazuhiro, additional, Yagi, Masafumi, additional, Okamura, Sadanori, additional, Doi, Mamoru, additional, Furusawa, Hisanori, additional, Hamabe, Masaru, additional, Kimura, Masahiko, additional, Komiyama, Yutaka, additional, Miyazaki, Masayuki, additional, Miyazaki, Satoshi, additional, Nakata, Fumiaki, additional, Ouchi, Masami, additional, Sekiguchi, Maki, additional, and Yasuda, Naoki, additional

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2004
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23. Evolution of Elliptical Galaxies at $z \gtrsim 1$ Revealed from a Large, Multicolor Sample of Extremely Red Objects

Author

Miyazaki, Masayuki, primary, Shimasaku, Kazuhiro, additional, Kodama, Tadayuki, additional, Okamura, Sadanori, additional, Furusawa, Hisanori, additional, Ouchi, Masami, additional, Nakata, Fumiaki, additional, Doi, Mamoru, additional, Hamabe, Masaru, additional, Kimura, Masahiko, additional, Komiyama, Yutaka, additional, Miyazaki, Satoshi, additional, Nagashima, Chie, additional, Nagata, Tetsuya, additional, Nagayama, Takahiro, additional, Nakajima, Yasushi, additional, Nakaya, Hidehiko, additional, Pickles, Andrew J., additional, Sato, Shuji, additional, Sekiguchi, Kazuhiro, additional, Sekiguchi, Maki, additional, Sugitani, Koji, additional, Takata, Tadafumi, additional, Tamura, Motohide, additional, Yagi, Masafumi, additional, and Yasuda, Naoki, additional

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2003
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24. Cosmic Shear Statistics in the Suprime‐Cam 2.1 Square Degree Field: Constraints on Ωmand σ8

Author

Hamana, Takashi, primary, Miyazaki, Satoshi, additional, Shimasaku, Kazuhiro, additional, Furusawa, Hisanori, additional, Doi, Mamoru, additional, Hamabe, Masaru, additional, Imi, Katsumi, additional, Kimura, Masahiko, additional, Komiyama, Yutaka, additional, Nakata, Fumiaki, additional, Okada, Norio, additional, Okamura, Sadanori, additional, Ouchi, Masami, additional, Sekiguchi, Maki, additional, Yagi, Masafumi, additional, and Yasuda, Naoki, additional

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2003
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25. Discovery of Latent Star Formation in the Extended H i Gas around the Local Group Dwarf Irregular Galaxy NGC 6822

Author

Komiyama, Yutaka, primary, Okamura, Sadanori, additional, Yagi, Masafumi, additional, Furusawa, Hisanori, additional, Doi, Mamoru, additional, Hamabe, Masaru, additional, Imi, Katsumi, additional, Kimura, Masahiko, additional, Miyazaki, Satoshi, additional, Nakata, Fumiaki, additional, Okada, Norio, additional, Ouchi, Masami, additional, Sekiguchi, Maki, additional, Shimasaku, Kazuhiro, additional, Yasuda, Naoki, additional, Arimoto, Nobuo, additional, and Ikuta, Chisato, additional

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2003
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26. Suprime-Cam: Subaru prime focus camera

Author

Komiyama, Yutaka, primary, Miyazaki, Satoshi, additional, Yagi, Masafumi, additional, Yasuda, Naoki, additional, Okamura, Sadanori, additional, Sekiguchi, Masaki, additional, Doi, Mamoru, additional, Shimasaku, Kazuhiro, additional, Nakata, Fumiaki, additional, Furusawa, Hisanori, additional, Kimura, Masahiko, additional, Ouchi, Masami, additional, Hamabe, Masaru, additional, and Nakaya, Hidehiko, additional

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2003
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27. A Search for [CLC]Ly[/CLC]α Emitters at Redshift 3.7

Author

Fujita, Shinobu S., primary, Ajiki, Masaru, additional, Shioya, Yasuhiro, additional, Nagao, Tohru, additional, Murayama, Takashi, additional, Taniguchi, Yoshiaki, additional, Okamura, Sadanori, additional, Ouchi, Masami, additional, Shimasaku, Kazuhiro, additional, Doi, Mamoru, additional, Furusawa, Hisanori, additional, Hamabe, Masaru, additional, Kimura, Masahiko, additional, Komiyama, Yutaka, additional, Miyazaki, Masayuki, additional, Miyazaki, Satoshi, additional, Nakata, Fumiaki, additional, Sekiguchi, Maki, additional, Yagi, Masafumi, additional, Yasuda, Naoki, additional, Matsuda, Yuichi, additional, Tamura, Hajime, additional, Hayashino, Tomoki, additional, Kodaira, Keiichi, additional, Karoji, Hiroshi, additional, Yamada, Toru, additional, Ohta, Kouji, additional, and Umemura, Masayuki, additional

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2003
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28. Subaru Deep Survey. II. Luminosity Functions and Clustering Properties of Lyα Emitters atz = 4.86 in the Subaru Deep Field

Author

Ouchi, Masami, primary, Shimasaku, Kazuhiro, additional, Furusawa, Hisanori, additional, Miyazaki, Masayuki, additional, Doi, Mamoru, additional, Hamabe, Masaru, additional, Hayashino, Tomoki, additional, Kimura, Masahiko, additional, Kodaira, Keiichi, additional, Komiyama, Yutaka, additional, Matsuda, Yuichi, additional, Miyazaki, Satoshi, additional, Nakata, Fumiaki, additional, Okamura, Sadanori, additional, Sekiguchi, Maki, additional, Shioya, Yasuhiro, additional, Tamura, Hajime, additional, Taniguchi, Yoshiaki, additional, Yagi, Masafumi, additional, and Yasuda, Naoki, additional

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2003
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29. Subaru Prime Focus Camera — Suprime-Cam

Author

Miyazaki, Satoshi, primary, Komiyama, Yutaka, additional, Sekiguchi, Maki, additional, Okamura, Sadanori, additional, Doi, Mamoru, additional, Furusawa, Hisanori, additional, Hamabe, Masaru, additional, Imi, Katsumi, additional, Kimura, Masahiko, additional, Nakata, Fumiaki, additional, Okada, Norio, additional, Ouchi, Masami, additional, Shimasaku, Kazuhiro, additional, Yagi, Masafumi, additional, and Yasuda, Naoki, additional

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2002
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30. Candidates for Intracluster Planetary Nebulae in the Virgo Cluster Based on the Suprime-Cam Narrow-Band Imaging in [O III] and $\mathrm{H}\alpha$

Author

Okamura, Sadanori, primary, Yasuda, Naoki, additional, Arnaboldi, Magda, additional, Freeman, Kenneth C., additional, Ando, Hiroyasu, additional, Doi, Mamoru, additional, Furusawa, Hisanori, additional, Gerhard, Ortwin, additional, Hamabe, Masaru, additional, Kimura, Masahiko, additional, Kajino, Toshitaka, additional, Komiyama, Yutaka, additional, Miyazaki, Satoshi, additional, Nakata, Fumiaki, additional, Napolitano, Nicola R., additional, Ouchi, Masami, additional, Pannella, Maurilio, additional, Sekiguchi, Maki, additional, Shimasaku, Kazuhiro, additional, and Yagi, Masafumi, additional

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2002
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31. Searching for Dark Matter Halos in the Suprime-Cam 2 Square Degree Field

Author

Miyazaki, Satoshi, primary, Hamana, Takashi, additional, Shimasaku, Kazuhiro, additional, Furusawa, Hisanori, additional, Doi, Mamoru, additional, Hamabe, Masaru, additional, Imi, Katsumi, additional, Kimura, Masahiko, additional, Komiyama, Yutaka, additional, Nakata, Fumiaki, additional, Okada, Norio, additional, Okamura, Sadanori, additional, Ouchi, Masami, additional, Sekiguchi, Maki, additional, Yagi, Masafumi, additional, and Yasuda, Naoki, additional

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2002
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32. The [CLC][ITAL]u[/ITAL][/CLC][arcmin]′[CLC][ITAL]g[/ITAL][/CLC][arcmin]′[CLC][ITAL]r[/ITAL][/CLC][arcmin]′[CLC][ITAL]i[/ITAL][/CLC][arcmin]′[CLC][ITAL]z[/ITAL][/CLC][arcmin]′ Standard-Star System

Author

Smith, J. Allyn, primary, Tucker, Douglas L., additional, Kent, Stephen, additional, Richmond, Michael W., additional, Fukugita, Masataka, additional, Ichikawa, Takashi, additional, Ichikawa, Shin-ichi, additional, Jorgensen, Anders M., additional, Uomoto, Alan, additional, Gunn, James E., additional, Hamabe, Masaru, additional, Watanabe, Masaru, additional, Tolea, Alin, additional, Henden, Arne, additional, Annis, James, additional, Pier, Jeffrey R., additional, McKay, Timothy A., additional, Brinkmann, Jon, additional, Chen, Bing, additional, Holtzman, Jon, additional, Shimasaku, Kazuhiro, additional, and York, Donald G., additional

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2002
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33. Discovery of a Very Extended Emission‐Line Region around the Seyfert 2 Galaxy NGC 4388

Author

Yoshida, Michitoshi, primary, Yagi, Masafumi, additional, Okamura, Sadanori, additional, Aoki, Kentaro, additional, Ohyama, Youichi, additional, Komiyama, Yutaka, additional, Yasuda, Naoki, additional, Iye, Masanori, additional, Kashikawa, Nobunari, additional, Doi, Mamoru, additional, Furusawa, Hisanori, additional, Hamabe, Masaru, additional, Kimura, Masahiko, additional, Miyazaki, Masayuki, additional, Miyazaki, Satoshi, additional, Nakata, Fumiaki, additional, Ouchi, Masami, additional, Sekiguchi, Maki, additional, Shimasaku, Kazuhiro, additional, and Ohtani, Hiroshi, additional

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2002
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34. Sloan Digital Sky Survey: Early Data Release

Author

Stoughton, Chris, primary, Lupton, Robert H., additional, Bernardi, Mariangela, additional, Blanton, Michael R., additional, Burles, Scott, additional, Castander, Francisco J., additional, Connolly, A. J., additional, Eisenstein, Daniel J., additional, Frieman, Joshua A., additional, Hennessy, G. S., additional, Hindsley, Robert B., additional, Ivezić, Željko, additional, Kent, Stephen, additional, Kunszt, Peter Z., additional, Lee, Brian C., additional, Meiksin, Avery, additional, Munn, Jeffrey A., additional, Newberg, Heidi Jo, additional, Nichol, R. C., additional, Nicinski, Tom, additional, Pier, Jeffrey R., additional, Richards, Gordon T., additional, Richmond, Michael W., additional, Schlegel, David J., additional, Smith, J. Allyn, additional, Strauss, Michael A., additional, SubbaRao, Mark, additional, Szalay, Alexander S., additional, Thakar, Aniruddha R., additional, Tucker, Douglas L., additional, Vanden Berk, Daniel E., additional, Yanny, Brian, additional, Adelman, Jennifer K., additional, Anderson, Jr., John E., additional, Anderson, Scott F., additional, Annis, James, additional, Bahcall, Neta A., additional, Bakken, J. A., additional, Bartelmann, Matthias, additional, Bastian, Steven, additional, Bauer, Amanda, additional, Berman, Eileen, additional, Böhringer, Hans, additional, Boroski, William N., additional, Bracker, Steve, additional, Briegel, Charlie, additional, Briggs, John W., additional, Brinkmann, J., additional, Brunner, Robert, additional, Carey, Larry, additional, Carr, Michael A., additional, Chen, Bing, additional, Christian, Damian, additional, Colestock, Patrick L., additional, Crocker, J. H., additional, Csabai, István, additional, Czarapata, Paul C., additional, Dalcanton, Julianne, additional, Davidsen, Arthur F., additional, Davis, John Eric, additional, Dehnen, Walter, additional, Dodelson, Scott, additional, Doi, Mamoru, additional, Dombeck, Tom, additional, Donahue, Megan, additional, Ellman, Nancy, additional, Elms, Brian R., additional, Evans, Michael L., additional, Eyer, Laurent, additional, Fan, Xiaohui, additional, Federwitz, Glenn R., additional, Friedman, Scott, additional, Fukugita, Masataka, additional, Gal, Roy, additional, Gillespie, Bruce, additional, Glazebrook, Karl, additional, Gray, Jim, additional, Grebel, Eva K., additional, Greenawalt, Bruce, additional, Greene, Gretchen, additional, Gunn, James E., additional, de Haas, Ernst, additional, Haiman, Zoltán, additional, Haldeman, Merle, additional, Hall, Patrick B., additional, Hamabe, Masaru, additional, Hansen, Brad, additional, Harris, Frederick H., additional, Harris, Hugh, additional, Harvanek, Michael, additional, Hawley, Suzanne L., additional, Hayes, J. J. E., additional, Heckman, Timothy M., additional, Helmi, Amina, additional, Henden, Arne, additional, Hogan, Craig J., additional, Hogg, David W., additional, Holmgren, Donald J., additional, Holtzman, Jon, additional, Huang, Chih-Hao, additional, Hull, Charles, additional, Ichikawa, Shin-Ichi, additional, Ichikawa, Takashi, additional, Johnston, David E., additional, Kauffmann, Guinevere, additional, Kim, Rita S. J., additional, Kimball, Tim, additional, Kinney, E., additional, Klaene, Mark, additional, Kleinman, S. J., additional, Klypin, Anatoly, additional, Knapp, G. R., additional, Korienek, John, additional, Krolik, Julian, additional, Kron, Richard G., additional, Krzesiński, Jurek, additional, Lamb, D. Q., additional, Leger, R. French, additional, Limmongkol, Siriluk, additional, Lindenmeyer, Carl, additional, Long, Daniel C., additional, Loomis, Craig, additional, Loveday, Jon, additional, MacKinnon, Bryan, additional, Mannery, Edward J., additional, Mantsch, P. M., additional, Margon, Bruce, additional, McGehee, Peregrine, additional, McKay, Timothy A., additional, McLean, Brian, additional, Menou, Kristen, additional, Merelli, Aronne, additional, Mo, H. J., additional, Monet, David G., additional, Nakamura, Osamu, additional, Narayanan, Vijay K., additional, Nash, Thomas, additional, Neilsen, Jr., Eric H., additional, Newman, Peter R., additional, Nitta, Atsuko, additional, Odenkirchen, Michael, additional, Okada, Norio, additional, Okamura, Sadanori, additional, Ostriker, Jeremiah P., additional, Owen, Russell, additional, Pauls, A. George, additional, Peoples, John, additional, Peterson, R. S., additional, Petravick, Donald, additional, Pope, Adrian, additional, Pordes, Ruth, additional, Postman, Marc, additional, Prosapio, Angela, additional, Quinn, Thomas R., additional, Rechenmacher, Ron, additional, Rivetta, Claudio H., additional, Rix, Hans-Walter, additional, Rockosi, Constance M., additional, Rosner, Robert, additional, Ruthmansdorfer, Kurt, additional, Sandford, Dale, additional, Schneider, Donald P., additional, Scranton, Ryan, additional, Sekiguchi, Maki, additional, Sergey, Gary, additional, Sheth, Ravi, additional, Shimasaku, Kazuhiro, additional, Smee, Stephen, additional, Snedden, Stephanie A., additional, Stebbins, Albert, additional, Stubbs, Christopher, additional, Szapudi, István, additional, Szkody, Paula, additional, Szokoly, Gyula P., additional, Tabachnik, Serge, additional, Tsvetanov, Zlatan, additional, Uomoto, Alan, additional, Vogeley, Michael S., additional, Voges, Wolfgang, additional, Waddell, Patrick, additional, Walterbos, René, additional, Wang, Shu-i, additional, Watanabe, Masaru, additional, Weinberg, David H., additional, White, Richard L., additional, White, Simon D. M., additional, Wilhite, Brian, additional, Wolfe, David, additional, Yasuda, Naoki, additional, York, Donald G., additional, Zehavi, Idit, additional, and Zheng, Wei, additional

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2002
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35. Suprime-Cam: Subaru prime focus camera.

Author

Komiyama, Yutaka, Miyazaki, Satoshi, Yagi, Masafumi, Yasuda, Naoki, Okamura, Sadanori, Sekiguchi, Masaki, Doi, Mamoru, Shimasaku, Kazuhiro, Nakata, Fumiaki, Furusawa, Hisanori, Kimura, Masahiko, Ouchi, Masami, Hamabe, Masaru, and Nakaya, Hidehiko

Published
2003
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36. Galaxy Population in a Cluster of Galaxies around the Radio Galaxy 3C 324 at $z=1.2$

Author

Nakata, Fumiaki, primary, Kajisawa, Masaru, additional, Yamada, Toru, additional, Kodama, Tadayuki, additional, Shimasaku, Kazuhiro, additional, Tanaka, Ichi, additional, Doi, Mamoru, additional, Furusawa, Hisanori, additional, Hamabe, Masaru, additional, Iye, Masanori, additional, Kimura, Masahiko, additional, Komiyama, Yutaka, additional, Miyazaki, Satoshi, additional, Okamura, Sadanori, additional, Ouchi, Masami, additional, Sasaki, Toshiyuki, additional, Sekiguchi, Maki, additional, Yagi, Masafumi, additional, and Yasuda, Naoki, additional

Published
2001
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37. Color Separation of Galaxy Types in the Sloan Digital Sky Survey Imaging Data

Author

Strateva, Iskra, primary, Ivezić, Željko, additional, Knapp, Gillian R., additional, Narayanan, Vijay K., additional, Strauss, Michael A., additional, Gunn, James E., additional, Lupton, Robert H., additional, Schlegel, David, additional, Bahcall, Neta A., additional, Brinkmann, Jon, additional, Brunner, Robert J., additional, Budavári, Tamás, additional, Csabai, István, additional, Castander, Francisco Javier, additional, Doi, Mamoru, additional, Fukugita, Masataka, additional, Győry, Zsuzsanna, additional, Hamabe, Masaru, additional, Hennessy, Greg, additional, Ichikawa, Takashi, additional, Kunszt, Peter Z., additional, Lamb, Don Q., additional, McKay, Timothy A., additional, Okamura, Sadanori, additional, Racusin, Judith, additional, Sekiguchi, Maki, additional, Schneider, Donald P., additional, Shimasaku, Kazuhiro, additional, and York, Donald, additional

Published
2001
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38. Clustering Properties of Galaxies at [CLC][ITAL]z[/ITAL][/CLC] ∼ 4 in the Subaru/[ITAL]XMM[/ITAL] Deep Survey Field

Author

Ouchi, Masami, primary, Shimasaku, Kazuhiro, additional, Okamura, Sadanori, additional, Doi, Mamoru, additional, Furusawa, Hisanori, additional, Hamabe, Masaru, additional, Kimura, Masahiko, additional, Komiyama, Yutaka, additional, Miyazaki, Masayuki, additional, Miyazaki, Satoshi, additional, Nakata, Fumiaki, additional, Sekiguchi, Maki, additional, Yagi, Masafumi, additional, and Yasuda, Naoki, additional

Published
2001
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39. Statistical Properties of Bright Galaxies in the Sloan Digital Sky Survey Photometric System

Author

Shimasaku, Kazuhiro, primary, Fukugita, Masataka, additional, Doi, Mamoru, additional, Hamabe, Masaru, additional, Ichikawa, Takashi, additional, Okamura, Sadanori, additional, Sekiguchi, Maki, additional, Yasuda, Naoki, additional, Brinkmann, Jon, additional, Csabai, István, additional, Ichikawa, Shin-Ichi, additional, Ivezić, Zeljko, additional, Kunszt, Peter Z., additional, Schneider, Donald P., additional, Szokoly, Gyula P., additional, Watanabe, Masaru, additional, and York, Donald G., additional

Published
2001
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40. Galaxy Number Counts from the Sloan Digital Sky Survey Commissioning Data

Author

Yasuda, Naoki, primary, Fukugita, Masataka, additional, Narayanan, Vijay K., additional, Lupton, Robert H., additional, Strateva, Iskra, additional, Strauss, Michael A., additional, Ivezić, Željko, additional, Kim, Rita S. J., additional, Hogg, David W., additional, Weinberg, David H., additional, Shimasaku, Kazuhiro, additional, Loveday, Jon, additional, Annis, James, additional, Bahcall, Neta A., additional, Blanton, Michael, additional, Brinkmann, Jon, additional, Brunner, Robert J., additional, Connolly, Andrew J., additional, Csabai, István, additional, Doi, Mamoru, additional, Hamabe, Masaru, additional, Ichikawa, Shin-Ichi, additional, Ichikawa, Takashi, additional, Johnston, David E., additional, Knapp, G. R., additional, Kunszt, Peter Z., additional, Lamb, D. Q., additional, McKay, Timothy A., additional, Munn, Jeffrey A., additional, Nichol, Robert C., additional, Okamura, Sadanori, additional, Schneider, Donald P., additional, Szokoly, Gyula P., additional, Vogeley, Michael S., additional, Watanabe, Masaru, additional, and York, Donald G., additional

Published
2001
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41. Narrowband filter system at the Subaru prime focus.

Author

Hayashino, Tomoki, Taniguchi, Yoshiaki, Yamada, Tohru, Shioya, Yasuhiro, Nagao, Tohru, Yoshida, Toshimitsu, Doi, Mamoru, Shimasaku, Kazuhiro, Komiyama, Yutaka, Nakata, Fumiaki, Furusawa, Hisanori, Kimura, Hitohiko, Ouchi, Masami, Aoki, Tsutomu, Hamabe, Masaru, Kodaira, Keiichi, Miyazaki, Satoshi, Takato, Naruhisa, Yagi, Masafumi, and Yasuda, Naoki

Published
2000
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43. Narrowband filter system at the Subaru prime focus

Author

Hayashino, Tomoki, primary, Taniguchi, Yoshiaki, additional, Yamada, Tohru, additional, Shioya, Yasuhiro, additional, Nagao, Tohru, additional, Yoshida, Toshimitsu, additional, Doi, Mamoru, additional, Shimasaku, Kazuhiro, additional, Komiyama, Yutaka, additional, Nakata, Fumiaki, additional, Furusawa, Hisanori, additional, Kimura, Hitohiko, additional, Ouchi, Masami, additional, Aoki, Tsutomu, additional, Hamabe, Masaru, additional, Kodaira, Keiichi, additional, Miyazaki, Satoshi, additional, Takato, Naruhisa, additional, Yagi, Masafumi, additional, Yasuda, Naoki, additional, Sekiguchi, Masaki, additional, and Okamura, Sadanori, additional

Published
2000
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44. Deep-Imaging Observations of a Candidate of an Absorbed QSO atz= 0.653, AX J131831+3341

Author

Akiyama, Masayuki, primary, Ohta, Kouji, additional, Tamura, Naoyuki, additional, Doi, Mamoru, additional, Kimura, Masahiko, additional, Komiyama, Yutaka, additional, Miyazaki, Satoshi, additional, Nakata, Fumiaki, additional, Okamura, Sadanori, additional, Sekiguchi, Maki, additional, Shimasaku, Kazuhiro, additional, Yagi, Masafumi, additional, Hamabe, Masaru, additional, Yoshida, Michitoshi, additional, and Takata, Tadahumi, additional

Published
2000
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45. STARS (Subaru Telescope archive system) for the effective return from Subaru Telescope

Author

Takata, Tadafumi, primary, Ogasawara, Ryusuke, additional, Kosugi, George, additional, Mizumoto, Yoshihiko, additional, Ichikawa, Shinichi, additional, Yasuda, Naoki, additional, Taga, Masatoshi, additional, Yagi, Masafumi, additional, Horaguchi, Toshihiro, additional, Baba, Hajime, additional, Watanabe, Masaru, additional, Ozawa, Tomohiko, additional, Hamabe, Masaru, additional, Yamamoto, Tadahiro, additional, and Kawarai, Kenji, additional

Published
2000
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46. Infrared Imaging of the Gravitational Lens PG 1115+080 with the Subaru Telescope

Author

Iwamuro, Fumihide, primary, Motohara, Kentaro, additional, Maihara, Toshinori, additional, Iwai, Jun'ichi, additional, Tanabe, Hirohisa, additional, Taguchi, Tomoyuki, additional, Hata, Ryuji, additional, Terada, Hiroshi, additional, Goto, Miwa, additional, Oya, Shin, additional, Akiyama, Masayuki, additional, Ando, Hiroyasu, additional, Aoki, Tetsuo, additional, Chikada, Yoshihiro, additional, Doi, Mamoru, additional, Fukuda, Takeo, additional, Hamabe, Masaru, additional, Hayashi, Masahiko, additional, Hayashi, Saeko S., additional, Horaguchi, Toshihiro, additional, Ichikawa, Shinichi, additional, Ichikawa, Takashi, additional, Imanishi, Masatoshi, additional, Imi, Katsumi, additional, Inata, Motoko, additional, Isobe, Shuzo, additional, Itoh, Yoichi, additional, Iye, Masanori, additional, Kaifu, Norio, additional, Kamata, Yukiko, additional, Kanzawa, Tomio, additional, Karoji, Hiroshi, additional, Kashikawa, Nobunari, additional, Kato, Taichi, additional, Kobayashi, Naoto, additional, Kobayashi, Yukiyasu, additional, Kodaira, Keiichi, additional, Kosugi, George, additional, Kurakami, Tomio, additional, Mikami, Yoshitaka, additional, Miyashita, Akihiko, additional, Miyata, Takashi, additional, Miyazaki, Satoshi, additional, Mizumoto, Yoshihiko, additional, Nakagiri, Masao, additional, Nakajima, Koich, additional, Nakamura, Kyoko, additional, Nariai, Kyoji, additional, Nishihara, Eiji, additional, Nishikawa, Jun, additional, Nishimura, Shiro, additional, Nishimura, Tetsuo, additional, Nishino, Tetsuo, additional, Noguchi, Kunio, additional, Noguchi, Takeshi, additional, Noumaru, Jun'ichi, additional, Ogasawara, Ryusuke, additional, Okada, Norio, additional, Okita, Kiichi, additional, Omata, Koji, additional, Oshima, Norio, additional, Otsubo, Masashi, additional, Sasaki, Goro, additional, Sasaki, Toshiyuki, additional, Sekiguchi, Maki, additional, Sekiguchi, Kazuhiro, additional, Shelton, Ian, additional, Simpson, Chris, additional, Suto, Hiroshi, additional, Takami, Hideki, additional, Takata, Tadafumi, additional, Takato, Naruhisa, additional, Tamura, Motohide, additional, Tanaka, Kyoko, additional, Tanaka, Wataru, additional, Tomono, Daigo, additional, Torii, Yasuo, additional, Usuda, Tomonori, additional, Waseda, Koichi, additional, Watanabe, Juni'chi, additional, Watanabe, Masaru, additional, Yagi, Masafumi, additional, Yamashita, Takuya, additional, Yamashita, Yasumasa, additional, Yasuda, Naoki, additional, Yoshida, Michitoshi, additional, Yoshida, Shigeomi, additional, and Yutani, Masami, additional

Published
2000
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47. High-Resolution Images of the Ring Nebula Taken with the Subaru Telescope

Author

Komiyama, Yutaka, primary, Yagi, Masafumi, additional, Miyazaki, Satoshi, additional, Okamura, Sadanori, additional, Tamura, Shin'ichi, additional, Fukushima, Hideo, additional, Doi, Mamoru, additional, Furusawa, Hisanori, additional, Fuse, Tetsuharu, additional, Hamabe, Masaru, additional, Hayashi, Masahiko, additional, Hayashino, Tomoki, additional, Imi, Katsumi, additional, Iye, Masanori, additional, Kaifu, Norio, additional, Karoji, Hiroshi, additional, Kawasaki, Wataru, additional, Kimura, Masahiko, additional, Kosugi, George, additional, Nakata, Fumiaki, additional, Noumaru, Junichi, additional, Okada, Norio, additional, Sasaki, Toshiyuki, additional, Sawada, Yasuhiro, additional, Sekiguchi, Maki, additional, Shelton, Ian, additional, Shimasaku, Kazuhiro, additional, Suzuki, Katsuyuki, additional, Takata, Tadafumi, additional, Taniguchi, Yoshiaki, additional, Usuda, Tomonori, additional, Yamashita, Takuya, additional, and Yasuda, Naoki, additional

Published
2000
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48. Subaru First-Light Deep Photometry of Galaxies in A 851 Field

Author

Iye, Masanori, primary, Iwamuro, Fumihide, additional, Maihara, Toshinori, additional, Miyazaki, Satoshi, additional, Okamura, Sadanori, additional, Shimasaku, Kazuhiro, additional, Simpson, Chris, additional, Akiyama, Masayuki, additional, Ando, Hiroyasu, additional, Aoki, Tetsuo, additional, Aoki, Tsutomu, additional, Chikada, Yoshihiro, additional, Doi, Mamoru, additional, Ebizuka, Noboru, additional, Fukuda, Takeo, additional, Furusawa, Hisanori, additional, Goto, Miwa, additional, Hamabe, Masaru, additional, Hata, Ryuji, additional, Hayashi, Masahiko, additional, Hayashi, Saeko S., additional, Horaguchi, Toshihiro, additional, Ichikawa, Shinichi, additional, Ichikawa, Takashi, additional, Imanishi, Masatoshi, additional, Imi, Katsumi, additional, Inata, Motoko, additional, Isobe, Shuzo, additional, Itoh, Yoichi, additional, Iwai, Junichi, additional, Kaifu, Norio, additional, Kamata, Yukiko, additional, Kanzawa, Tomio, additional, Karoji, Hiroshi, additional, Kashikawa, Nobunari, additional, Kato, Taichi, additional, Kawasaki, Wataru, additional, Kimura, Masahiko, additional, Kobayashi, Naoto, additional, Kobayashi, Yukiyasu, additional, Kodaira, Keiichi, additional, Komiyama, Yutaka, additional, Kosugi, George, additional, Kurakami, Tomio, additional, Mikami, Yoshitaka, additional, Miyashita, Akihiko, additional, Miyata, Takashi, additional, Mizumoto, Yoshihiko, additional, Motohara, Kentaro, additional, Nakagiri, Masao, additional, Nakajima, Koich, additional, Nakamura, Kyoko, additional, Nakata, Fumiaki, additional, Nariai, Kyoji, additional, Nishihara, Eiji, additional, Nishikawa, Jun, additional, Nishimura, Shiro, additional, Nishimura, Tetsuo, additional, Nishino, Tetsuo, additional, Noguchi, Kunio, additional, Noguchi, Takeshi, additional, Noumaru, Junichi, additional, Ogasawara, Ryusuke, additional, Okada, Norio, additional, Okita, Kiichi, additional, Omata, Koji, additional, Oshima, Norio, additional, Otsubo, Masashi, additional, Oya, Shin, additional, Sasaki, Goro, additional, Sasaki, Toshiyuki, additional, Sawada, Yasuhiro, additional, Sekiguchi, Kazuhiro, additional, Sekiguchi, Maki, additional, Shelton, Ian, additional, Suto, Hiroshi, additional, Suzuki, Katsuyuki, additional, Taguchi, Tomoyuki, additional, Takami, Hideki, additional, Takata, Tadafumi, additional, Takato, Naruhisa, additional, Tamura, Motohide, additional, Tanabe, Hirohisa, additional, Tanaka, Kyoko, additional, Tanaka, Wataru, additional, Terada, Hiroshi, additional, Tomono, Daigo, additional, Torii, Yasuo, additional, Tsukamoto, Hiroyuki, additional, Usuda, Tomonori, additional, Watanabe, Junichi, additional, Watanabe, Masaru, additional, Yagi, Masafumi, additional, Yamashita, Takuya, additional, Yamashita, Yasumasa, additional, Yasuda, Naoki, additional, Yoshida, Michitoshi, additional, Yoshida, Shigeomi, additional, and Yutani, Masami, additional

Published
2000
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49. The First Light of the Subaru Telescope: A New Infrared Image of the Orion Nebula

Author

Kaifu, Norio, primary, Usuda, Tomonori, additional, Hayashi, Saeko S., additional, Itoh, Yoichi, additional, Akiyama, Masayuki, additional, Yamashita, Takuya, additional, Nakajima, Yasushi, additional, Tamura, Motohide, additional, Inutsuka, Shuichiro, additional, Hayashi, Masahiko, additional, Maihara, Toshinori, additional, Iwamuro, Fumihide, additional, Motohara, Kentaro, additional, Iwai, Jun'ich, additional, Tanabe, Hirohisa, additional, Taguchi, Tomoyuki, additional, Hata, Ryuji, additional, Terada, Hiroshi, additional, Goto, Miwa, additional, Ando, Hiroyasu, additional, Aoki, Tetsuo, additional, Chikada, Yoshihiro, additional, Doi, Mamoru, additional, Ebizuka, Noboru, additional, Fukuda, Takeo, additional, Hamabe, Masaru, additional, Hasegawa, Tetsuo, additional, Horaguchi, Toshihiro, additional, Ichikawa, Shinichi, additional, Ichikawa, Takashi, additional, Imanishi, Masatoshi, additional, Imi, Katsumi, additional, Inata, Motoko, additional, Isobe, Shuzo, additional, Iye, Masanori, additional, Kamata, Yukiko, additional, Kanzawa, Tomio, additional, Karoji, Hiroshi, additional, Kashikawa, Nobunari, additional, Kataza, Hirokazu, additional, Kato, Taichi, additional, Kobayashi, Naoto, additional, Kobayashi, Yukiyasu, additional, Kodaira, Keiichi, additional, Kosugi, George, additional, Kurakami, Tomio, additional, Mikami, Yoshitaka, additional, Miyama, Shoken M., additional, Miyashita, Akihiko, additional, Miyata, Takashi, additional, Miyazaki, Satoshi, additional, Mizumoto, Yoshihiko, additional, Nakagiri, Masao, additional, Nakajima, Koich, additional, Nakamura, Kyoko, additional, Nariai, Kyoji, additional, Nishihara, Eiji, additional, Nishikawa, Jun, additional, Nishimura, Shiro, additional, Nishimura, Tetsuo, additional, Nishino, Tetsuo, additional, Noguchi, Kunio, additional, Noguchi, Takeshi, additional, Noumaru, Junichi, additional, Ogasawara, Ryusuke, additional, Okada, Norio, additional, Okita, Kiichi, additional, Omata, Koji, additional, Oshima, Norio, additional, Otsubo, Masashi, additional, Sasaki, Goro, additional, Sasaki, Toshiyuki, additional, Sekiguchi, Maki, additional, Sekiguchi, Kazuhiro, additional, Shelton, Ian, additional, Simpson, Chris, additional, Suto, Hiroshi, additional, Takami, Hideki, additional, Takata, Tadafumi, additional, Takato, Naruhisa, additional, Tanaka, Kyoko, additional, Tanaka, Wataru, additional, Tomono, Daigo, additional, Torii, Yasuo, additional, Waseda, Koichi, additional, Watanabe, Junichi, additional, Watanabe, Masaru, additional, Yagi, Masafumi, additional, Yamashita, Yasumasa, additional, Yasuda, Naoki, additional, Yoshida, Michitoshi, additional, Yoshida, Shigeomi, additional, and Yutani, Masami, additional

Published
2000
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50. An Astronomical Data Archive System with a Java-Based User Interface

Author

Horaguchi, Toshihiro, primary, Nishihara, Eiji, additional, Yoshida, Michitoshi, additional, Aoki, Kentaro, additional, Ito, Takashi, additional, Watanabe, Masaru, additional, Ichikawa, Shin'ichi, additional, Takata, Tadafumi, additional, Yoshida, Shigeomi, additional, and Hamabe, Masaru, additional

Published
1999
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