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Related papers: Photometry Study of Open Cluster NGC 7788

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Stars appearing in CCD images obtained over 224 nights during the course of 69 observing runs have been calibrated to the Johnson/Kron-Cousins BVRI photometric system defined by the equatorial standards of Landolt (1992, AJ, 104, 340). More…

Astrophysics · Physics 2009-10-31 Peter B. Stetson

In this paper, we present a set of photometric observations in 15 colors of stars in the Landolt covered by the system range from 300 nm to 1000 nm. Visual magnitudes of the stars being studied in the field are from 10th to 20th mag. The…

Three new photometric CCD-based datasets are presented for NGC~6791. They consist of deep UBV photometry (to $V_{lim} =24$, $B_{lim}=24$, $U_{lim} = 23$) of the central parts of the cluster and of selected fields around it, and of…

Astrophysics · Physics 2016-08-30 Janusz Kaluzny , Slavek Rucinski

A photometric, astrometric and spectroscopic investigation of the poorly studied open cluster NGC 6738 has been performed in order to ascertain its real nature. NGC 6738 is definitely not a physical stellar ensemble: photometry does not…

Astrophysics · Physics 2009-11-07 C. Boeche , R. Barbon , A. Henden , U. Munari , P. Agnolin

We present new photometric V-, R- and I-band data for the rich galaxy cluster AC 118 at z=0.31. The new photometry covers an area of 8.6x8.6 arcmin$^2$, corresponding to 2.9$\times$2.9 Mpc$^2$ (H$_0=50$ km s$^{-1}$ Mpc$^{-1}$, q$_0=0.5$ and…

Astrophysics · Physics 2009-11-07 G. Busarello , Merluzzi , F. La Barbera , M. Massarotti , M. Capaccioli

The results of astrometric and photometric investigations of the poorly studied open cluster NGC 1513 are presented. The proper motions of 353 stars with the root-mean-square error of 1.9 mas/yr were obtained by means of the automated…

As part of the Swift/UVOT Stars Survey, we present near-ultraviolet point-source photometry for 103 Galactic open clusters. These data, taken over the span of the mission, provide a unique and unprecedented set of near-ultraviolet…

Solar and Stellar Astrophysics · Physics 2019-07-10 Michael H. Siegel , Samuel J. Laporte , Blair L. Porterfield , Lea M. Z. Hagen , Caryl A. Gronwall

We present the first part of the first large and homogeneous CCD color-magnitude diagram (CMD) data base, comprising 52 nearby Galactic globular clusters (GGC) imaged in the V and I bands using only two telescopes (one for each hemisphere).…

Astrophysics · Physics 2015-06-24 A. Rosenberg , G. Piotto , I. Saviane , A. Aparicio

We present new photometry for 323 of the globular clusters in NGC 5128 (Centaurus A), measured for the first time in the $g'r'i'z'$ filter system. The color indices are calibrated directly to standard stars in the $g'r'i'z'$ system and are…

Astrophysics of Galaxies · Physics 2015-05-20 B. Sinnott , A. Hou , R. Anderson , W. E. Harris , K. A. Woodley

This paper presents 13 color CCD intermediate-band spectrophotometry of a field centered on the open cluster M48 (NGC 2548), from 400nm to nearly 1000nm, taken with Beijing-Arizona-Taiwan-Connecticut (BATC) Multi-Color Survey Photometric…

Astrophysics · Physics 2009-11-10 Zhen-Yu Wu , Xu Zhou , Jun Ma , Zhao-Ji Jiang , Jian-Sheng Chen

We present CCD BV and JHK$_{s}$ 2MASS photometric data for the open cluster NGC 1513. We observed 609 stars in the direction of the cluster up to a limiting magnitude of $V\sim19$ mag. The star count method shows that the centre of the…

Astrophysics of Galaxies · Physics 2014-11-20 S. Bilir , T. Guver , I. Khamitov , T. Ak , S. Ak , K. B. Coskunoglu , E. Paunzen , E. Yaz

We present 13-band CCD intermediate-band spectrophotometry of a field centered on the open cluster NGC 7789 from 400 to nearly 1000 nm, taken with Beijing-Arizona-Taiwan-Connecticut (BATC) Multi-Color Survey photometric system. By comparing…

Astrophysics · Physics 2008-11-26 Zhen-Yu Wu , Xu Zhou , Jun Ma , Zhao-Ji Jiang , Jian-Sheng Chen , Jiang-Hua Wu

A sample of 145 JHK--2MASS observations of NGC open star clusters is studied, of which 132 have never been studied before. Twelve are classified as non-open clusters and 13 are re-estimated self-consistently, after applying the same methods…

Astrophysics of Galaxies · Physics 2019-12-06 A. L. Tadross

In this paper we present the second and final part of a large and photometrically homogeneous CCD color-magnitude diagram (CMD) data base, comprising 52 nearby Galactic globular clusters (GGC) imaged in the V and I bands. The catalog has…

Astrophysics · Physics 2015-06-24 A. Rosenberg , A. Aparicio , I. Saviane , G. Piotto

Here we have obtained the {\it BVRI CCD} photometry down to a limiting magnitude of $V \sim$ 20 for the southern poorly studied open cluster NGC 6631. It is observed from the {\it 1.88 m} Telescope of Kottamia Observatory in Egypt. About…

Astrophysics of Galaxies · Physics 2014-03-04 A. L. Tadross , R. Bendary , H. Priya , A. Essam , A. Osman

We have been doing a photometric and astrometric sample survey programme on Schmidt plates in a few selected directions in the Galaxy with an aim to study galactic stellar populations. In order to calibrate Schmidt plates photometrically,…

CCD photometry on the uvbyCaHbeta system is presented for the open cluster, NGC 3680. Restricting the data to probable cluster members using the CMD and the photometric indices alone defines a sample of 34 stars at the cluster turnoff that…

Astrophysics · Physics 2009-11-10 B. J. Anthony-Twarog , B. A. Twarog

The Hubble Space Telescope has been used to obtain WFPC2 (V,I) photometry for a large sample of stars in the outer halo of the giant elliptical NGC 5128 (d = 4 Mpc). The globular cluster N5128-C44, at the center of the Planetary Camera…

Astrophysics · Physics 2009-10-30 G. L. H. Harris , G. B. Poole , W. E. Harris

We describe a technique to identify Be stars in open clusters using Stromgren b, y, and narrow-band Halpha photometry. We first identify the B-type stars of the cluster using a theoretical isochrone fit to the (b-y, y) color-magnitude…

Astrophysics · Physics 2009-11-10 M. Virginia McSwain , Douglas R. Gies

We present multi-colour broad band CCD photometric observations of a few thousands of stars located region of the galactic globular clusters NGC 1904 and NGC 6341. These observations are used to generate their deep colour magnitude diagrams…

Astrophysics · Physics 2007-05-23 Alok C. Gupta