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188 results on '"Seitz, Stella"'

51. The Wendelstein Calar Alto Pixellensing Project (WeCAPP): The M31 Variable Star Catalogue

Author

Fliri, Juergen, Riffeser, Arno, Seitz, Stella, and Bender, Ralf

Subjects
Astrophysics
Abstract

In this paper we present the WeCAPP variable star catalogue towards the bulge of M31. The observations of the WeCAPP microlensing survey (optical R and I bands) during three years (2000-2003) result in a database with unprecedented time coverage for an extragalactic variable star study. We detect 23781 variable sources in a 16.1' x 16.6' field centered on the nucleus of M31. The catalogue of variable stars contains the positions, the periods and the variations in the R and I bands. We classify the variables according to their position in the R-band period-amplitude plane. Three groups can be distinguished; while the first two groups can be mainly associated with Cepheid-like variables (population I Cepheids in group I, type II Cepheids and RV Tauri stars in group II), the third one consists of Long Period Variables (LPVs). We detect 37 RV Tauri stars and 11 RV Tauri candidates which is one of the largest collections of this class of stars to date. The classification scheme is supported by Fourier decomposition of the light curves. Our data shows a correlation of the low-order Fourier coefficients Phi_21 with Phi_31 for classical Cepheids, as well for type II Cepheids and RV Tauri stars. Correlating our sample of variable stars with the X-ray based catalogues of Kaaret (2002) and Kong et al. (2002) results in 23 and 31 coincidences, 8 of which are M31 globular clusters. The number density of detected variables is clearly not symmetric, which has to be included in the calculations of the expected microlensing event rate towards M31. This asymmetry is due to the enhanced extinction in the spiral arms superimposed on the bulge of M31 which reduces the number of sources to about 60%, if compared to areas of equivalent bulge brightness (without enhanced extinction being present)., Comment: 22 pages, re-submitted to A&A after referee comments have been taken into account

Published
2005
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52. The Wendelstein Calar Alto Pixellensing Project(WeCAPP): First MACHO Candidates

Author

Riffeser, Arno, Fliri, Juergen, Bender, Ralf, Seitz, Stella, and Goessl, Claus A.

Subjects
Astrophysics
Abstract

We report the detection of the first 2 microlensing candidates from the Wendelstein Calar Alto Pixellensing Project (WeCAPP). Both are detected with a high signal-to-noise-ratio and were filtered out from 4.5 mill. pixel light curves using a variety of selection criteria. Here we only consider well-sampled events with timescales of 1 d < t_fwhm < 20 d, high amplitude, and low chi^2 of the microlensing fit. The two-color photometry (R,I) shows that the events are achromatic and that giant stars with colors of (R-I) ~ 1.1 mag in the bulge of M31 have been lensed. The magnification factors are 64 and 10 which are obtained for typical giant luminosities of M_I = -2.5 mag. Both lensing events lasted for only a few days (t_fwhm^GL1 = 1.7 d and t_fwhm^GL2 = 5.4 d). The event GL1 is likely identical with PA-00-S3 reported by the POINT-AGAPE project. Our calculations favor in both cases the possibility that MACHOs in the halo of M31 caused the lensing events. The most probable masses, 0.08 M_sun for GL1 and 0.02 M_sun for GL2, are in the range of the brown dwarf limit of hydrogen burning. Solar mass objects are a factor of two less likely., Comment: Accepted for publication in ApJ Letters (28 Oct 2003), 4 pages, 2 color figures, uses emulateapj style

Published
2003
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53. WeCAPP - The Wendelstein Calar Alto Pixellensing Project I Tracing Dark and Bright Matter in M31

Author

Riffeser, Arno, Fliri, Juergen, Goessl, Claus A., Bender, Ralf, Hopp, Ulrich, Baernbantner, Otto, Ries, Christoph, Barwig, Heinz, Seitz, Stella, and Mitsch, Wolfgang

Subjects
Astrophysics
Abstract

We present WeCAPP, a long term monitoring project searching for microlensing events towards M 31. Since 1997 the bulge of M 31 was monitored in two different wavebands with the Wendelstein 0.8 m telescope. In 1999 we extended our observations to the Calar Alto 1.23 m telescope. Observing simultaneously at these two sites we obtained a time coverage of 53 % during the observability of M 31. To check thousands of frames for variability of unresolved sources, we used the optimal image subtraction method (OIS) by Alard & Lupton (1998) This enabled us to minimize the residuals in the difference image analysis (DIA) and to detect variable sources with amplitudes at the photon noise level. Thus we can detect microlensing events with corresponding amplifications A > 10 of red clump giants with M_I = 0., Comment: 10 pages, 21 figures, published in Astronomy & Astrophysics (2001)

Published
2001
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54. 4MOST Complete Calibration of the Colour-Redshift Relation (4C3R2)

Author

Gruen, Daniel, McCullough, Jamie, Amon, Alexandra, Bernstein, Gary, Van Den Busch, Jan Luca, Canning, Rebecca, Castander, Francisco, DeRose, Joseph, Hartley, William, Hildebrandt, Hendrik, Kuijken, Konrad, Liske, Jochen, Masters, Daniel, Miquel, Ramon, Yuste, Andrea Pocino, Roodman, Aaron, Seitz, Stella, Saglia, Roberto, Stern, Daniel, Tortorelli, Luca, and Wright, Angus H.

Abstract

Accurate knowledge of the redshift distributions of faint samples of galaxies selected by broad-band photometry is a prerequisite for future weak lensing experiments to deliver precision tests of our cosmological model. The most direct way to measure these redshift distributions is spectroscopic follow-up of representative galaxies. For this to be efficient and accurate, targets have to be selected such that they systematically cover a space defined by apparent colours in which there is little variation in redshift at any point. 4C3R2 will follow this strategy to observe over 100 000 galaxies selected by their KiDS-VIKING ugriZYJHKs photometry over a footprint identical to that of the WAVES survey, to constrain the colour-redshift relation with high multiplicity across two-thirds of the colour space of future Euclid and Rubin samples., Published in The Messenger vol. 190, pp. 28-30, March 2023.

Published
2023
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57. Cepheids in M31: The PAndromeda Cepheid Sample

Author

Kodric, Mihael, primary, Riffeser, Arno, additional, Hopp, Ulrich, additional, Goessl, Claus, additional, Seitz, Stella, additional, Bender, Ralf, additional, Koppenhoefer, Johannes, additional, Obermeier, Christian, additional, Snigula, Jan, additional, Lee, Chien-Hsiu, additional, Burgett, W. S., additional, Draper, P. W., additional, Hodapp, K. W., additional, Kaiser, N., additional, Kudritzki, R.-P., additional, Metcalfe, N., additional, Tonry, J. L., additional, and Wainscoat, R. J., additional

Published
2018
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58. The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters

Author

Umetsu, Keiichi, primary, Sereno, Mauro, additional, Tam, Sut-Ieng, additional, Chiu, I-Non, additional, Fan, Zuhui, additional, Ettori, Stefano, additional, Gruen, Daniel, additional, Okumura, Teppei, additional, Medezinski, Elinor, additional, Donahue, Megan, additional, Meneghetti, Massimo, additional, Frye, Brenda, additional, Koekemoer, Anton, additional, Broadhurst, Tom, additional, Zitrin, Adi, additional, Balestra, Italo, additional, Benítez, Narciso, additional, Higuchi, Yuichi, additional, Melchior, Peter, additional, Mercurio, Amata, additional, Merten, Julian, additional, Molino, Alberto, additional, Nonino, Mario, additional, Postman, Marc, additional, Rosati, Piero, additional, Sayers, Jack, additional, and Seitz, Stella, additional

Published
2018
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59. Entropy-regularized Maximum-Likelihood cluster mass reconstruction

Author

Seitz, Stella, Schneider, Peter, and Bartelmann, Matthias

Subjects
Astrophysics
Abstract

We present a new method for reconstructing two-dimensional mass maps of galaxy clusters from the image distortion of background galaxies. In contrast to most previous approaches, which directly convert locally averaged image ellipticities to mass maps (direct methods), our entropy-regularized maximum-likelihood method is an inverse approach. Albeit somewhat more expensive computationally, our method allows high spatial resolution in those parts of the cluster where the lensing signal is strong enough. Furthermore, it allows to straightforwardly incorporate additional constraints, such as magnification information or strong-lensing features. Using synthetic data, we compare our new approach to direct methods and find indeed a substantial improvement especially in the reconstruction of mass peaks. The main differences to previously published inverse methods are discussed., Comment: 19 pages including 7 postscript figures; submitted to Astronomy and Astrophysics

Published
1998

60. A new finite-field mass reconstruction algorithm

Author

Seitz, Stella and Schneider, Peter

Subjects
Astrophysics
Abstract

A new method for the reconstruction of the projected mass distribution of clusters of galaxies from the image distortion of background galaxies is discussed. This method is essentially equivalent to the one we developed previously, i.e., the noise-filtering method, but has several practical advantages: (1) It is much easier to implement; (2) it can be easily applied to wide-field images, since the constraints on the number of gridpoints are much weaker than for the previous method, and (3) it can be easily generalized to more complicated field geometries, such as that of the Wide Field Planetary Camera 2 (WFPC2) onboard HST. We have tested the performance of our new inversion method (for which a FORTRAN-77 implementation is available from the authors) using simulated data, demonstrating that it fares very favourably., Comment: 13 pages, 6 figures included; Fortran subroutines can be requested after paper will be accepted

Published
1998

61. The Mass Distribution of CL0939+4713 obtained from a `Weak' Lensing Analysis of a WFPC2 image

Author

Seitz, Carolin, Kneib, Jean-Paul, Schneider, Peter, and Seitz, Stella

Subjects
Astrophysics
Abstract

The image distortions of high-redshift galaxies caused by gravitational light deflection of foreground clusters of galaxies can be used to reconstruct the two-dimensional surface mass density of these clusters. We apply an unbiased parameter-free reconstruction technique to the cluster CL0939+4713 (Abell 851), observed with the WFPC2 on board of the HST. We demonstrate that a single deep WFPC2 observation can be used for cluster mass reconstruction despite its small field of view and the irregular shape of the data field (especially for distant clusters). For CL0939, we find a strong correlation between the reconstructed mass distribution and the bright cluster galaxies indicating that mass follows light on average. The detected anti-correlation between the faint galaxies and the reconstructed mass is most likely an effect of the magnification (anti) bias, which was detected previously in the cluster A1689. Because of the high redshift of CL0939 (z_d=0.41), the redshift distribution of the lensed, faint galaxies has to be accounted for in the reconstruction technique. We derive an approximate global transformation for the surface mass density which leaves the mean image ellipticities invariant, resulting in an uncertainty in the normalization of the mass. From the non-negativity of the surface mass density, we derive lower limits on the mass inside the observed field. We can break the invariance transformation for the mass using the magnification effect on the observed number density of the background galaxies. Assuming a mean redshift of 0.8 and a fraction of 15 % (20 %) of cluster galaxies in the observed galaxy sample with 23

Published
1996

62. Maximum-Likelihood Cluster Recontruction

Author

Bartelmann, Matthias, Narayan, Ramesh, Seitz, Stella, and Schneider, Peter

Subjects
Astrophysics
Abstract

We present a novel method to recontruct the mass distribution of galaxy clusters from their gravitational lens effect on background galaxies. The method is based on a least-chisquare fit of the two-dimensional gravitational cluster potential. The method combines information from shear and magnification by the cluster lens and is designed to easily incorporate possible additional information. We describe the technique and demonstrate its feasibility with simulated data. Both the cluster morphology and the total cluster mass are well reproduced., Comment: 9 pages including 2 figures, submitted to ApJ Letters

Published
1996
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63. Cluster lens reconstruction using only observed local data -- an improved finite-field inversion technique

Author

Seitz, Stella and Schneider, Peter

Subjects
Astrophysics
Abstract

Gravitational light deflection can distort the images of distant sources by its tidal effects. The population of faint blue galaxies is at sufficiently high redshift so that their images are distorted near foreground clusters, with giant luminous arcs being the most spectacular evidence for this effect. Much weaker distortions, however, can observationally be detected by a statistical analysis of the numerous faint galaxy images, as first demonstrated by Tyson, Valdes \& Wenk. This distortion effect can be used as a {\it quantitativetool} for the reconstruction of the surface mass density of galaxy clusters with appropriate redshifts, as was demonstrated by Kaiser \&Squires. They have derived an explicit equation for this surface mass density in terms of its tidal field. The reconstruction formula by Kaiser \& Squires must be modified because of two effects: in its original form it applies only to weak lenses, and hence must be generalized to account for stronger lensing effects. Second, due to the nature of the inversion formula, it produces boundary artefacts (or biases) if applied to real data which are confined to a finite field on the sky. We discuss several possibilities to obtain inversion formulae which are exact for ideal data on a finite data field (CCD). We demonstrate that there exists an infinite number of such finite-field inversion formulae, which differ in their sensitivity to observational effects (such as noise, intrinsic ellipticities of the sources, etc.). We show that, using two simple conditions, one can uniquely specify a finite-field formula which in a well-defined sense minimizes the sensitivity to observational effects. We then use synthetic data to compare the quality of our new reconstruction method with that of previous, Comment: uuenc.ps-file, Fig.1,4,10 are in a second file (uuenc.ps) The new inversion kernel is easy to program but can also be obtained from the Authors (stella@mpa-garching.mpg.de)

Published
1995

64. The Density of 1-Jansky Sources Around Zwicky Clusters

Author

Seitz, Stella and Schneider, Peter

Subjects
Astrophysics
Abstract

In a recent paper by Rodrigues-Williams \& Hogan (RH94), a correlation between high-redshift, optically-selected QSOs and Zwicky clusters was reported at a very high significance level. Due to the fairly bright flux threshold of the cluster sample, these correlations cannot be interpreted as being due to an environmental effect of the clusters on the quasar activity. The most likely interpretation employed in RH94 was the effect of gravitational lensing by the foreground clusters, though the required magnification to explain the observed correlations has to be considerably higher than obtained from simple mass models for the clusters. We have repeated the analysis of RH94 using a different QSO sample, namely radio quasars and radio galaxies from the 1-Jy sample. In accordance with RH, we detect a statistically significant correlation between Zwicky clusters and 1-Jy sources with intermediate redshift ($z\approx 1$), but fail to detect significant effects for higher-redshift sources. In addition, we detect a highly significant underdensity of low-redshift radio sources around Zwicky clusters, for which an environmental interpretation seems to be most reasonable. Our result for the overdensity of $z\sim 1$ sources is in good agreement with previous results and can possibly be interpreted as a lensing effect, though we have not tried to quantitatively investigate a lensing model. Other interpretations, such as patchy dust obscuration, can not explain the observed effect and its tendency with redshift., Comment: 21 pages, uudecoded postscriptfile, figures included, MPA preprint number 828

Published
1994

65. Light Propagation in Arbitrary Spacetimes and the Gravitational Lens Approximation

Author

Seitz, Stella, Schneider, Peter, and Ehlers, Juergen

Subjects
Astrophysics
Abstract

We reformulate the transport equation which determines the size, shape and orientation of infinitesimal light beams in arbitrary spacetimes. The behaviour of such light beams near vertices and conjugate points is investigated, with special attention to the singular behaviour of the optical scalars. We then specialize the general transport equation to the case of an approximate metric of an inhomogeneous universe, which is a Friedmann metric `on average' with superposed isolated weak matter inhomogeneities. In a series of well-defined approximations, the equations of gravitational lens theory are derived. Finally, we derive a relative optical focusing equation which describes the focusing of light beams relative to the case that the beam is unaffected by matter inhomogeneities in the universe, from which it follows immediately that no beam can be focused less than one which is unaffected by matter clumps, before it propagates through its first conjugate point., Comment: 31 pages, uuencoded compressed postscript; preprint MPA 787

Published
1994
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66. Unveiling the Dynamical State of Massive Clusters through the ICL Fraction

Author

Jiménez-Teja, Yolanda, primary, Dupke, Renato, additional, Benítez, Narciso, additional, Koekemoer, Anton M., additional, Zitrin, Adi, additional, Umetsu, Keiichi, additional, Ziegler, Bodo L., additional, Frye, Brenda L., additional, Ford, Holland, additional, Bouwens, Rychard J., additional, Bradley, Larry D., additional, Broadhurst, Thomas, additional, Coe, Dan, additional, Donahue, Megan, additional, Graves, Genevieve J., additional, Grillo, Claudio, additional, Infante, Leopoldo, additional, Jouvel, Stephanie, additional, Kelson, Daniel D., additional, Lahav, Ofer, additional, Lazkoz, Ruth, additional, Lemze, Dorom, additional, Maoz, Dan, additional, Medezinski, Elinor, additional, Melchior, Peter, additional, Meneghetti, Massimo, additional, Mercurio, Amata, additional, Merten, Julian, additional, Molino, Alberto, additional, Moustakas, Leonidas A., additional, Nonino, Mario, additional, Ogaz, Sara, additional, Riess, Adam G., additional, Rosati, Piero, additional, Sayers, Jack, additional, Seitz, Stella, additional, and Zheng, Wei, additional

Published
2018
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69. Falling Outer Rotation Curves of Star-forming Galaxies at 0.6 ≲z≲ 2.6 Probed with KMOS3Dand SINS/zC-SINF

Author

Lang, Philipp, primary, Förster Schreiber, Natascha M., additional, Genzel, Reinhard, additional, Wuyts, Stijn, additional, Wisnioski, Emily, additional, Beifiori, Alessandra, additional, Belli, Sirio, additional, Bender, Ralf, additional, Brammer, Gabe, additional, Burkert, Andreas, additional, Chan, Jeffrey, additional, Davies, Ric, additional, Fossati, Matteo, additional, Galametz, Audrey, additional, Kulkarni, Sandesh K., additional, Lutz, Dieter, additional, Mendel, J. Trevor, additional, Momcheva, Ivelina G., additional, Naab, Thorsten, additional, Nelson, Erica J., additional, Saglia, Roberto P., additional, Seitz, Stella, additional, Tacchella, Sandro, additional, Tacconi, Linda J., additional, Tadaki, Ken-ichi, additional, Übler, Hannah, additional, van Dokkum, Pieter G., additional, and Wilman, David J., additional

Published
2017
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72. KMOS3D: DYNAMICAL CONSTRAINTS ON THE MASS BUDGET IN EARLY STAR-FORMING DISKS

Author

Wuyts, Stijn, primary, Schreiber, Natascha M. Förster, additional, Wisnioski, Emily, additional, Genzel, Reinhard, additional, Burkert, Andreas, additional, Bandara, Kaushala, additional, Beifiori, Alessandra, additional, Belli, Sirio, additional, Bender, Ralf, additional, Brammer, Gabriel B., additional, Chan, Jeffrey, additional, Davies, Ric, additional, Fossati, Matteo, additional, Galametz, Audrey, additional, Kulkarni, Sandesh K., additional, Lang, Philipp, additional, Lutz, Dieter, additional, Mendel, J. Trevor, additional, Momcheva, Ivelina G., additional, Naab, Thorsten, additional, Nelson, Erica J., additional, Saglia, Roberto P., additional, Seitz, Stella, additional, Tacconi, Linda J., additional, Tadaki, Ken-ichi, additional, Übler, Hannah, additional, Dokkum, Pieter G. van, additional, Wilman, David J., additional, and Wuyts, Eva, additional

Published
2016
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73. THE EVOLUTION OF METALLICITY AND METALLICITY GRADIENTS FROMz= 2.7 TO 0.6 WITH KMOS3D

Author

Wuyts, Eva, primary, Wisnioski, Emily, additional, Fossati, Matteo, additional, Schreiber, Natascha M. Förster, additional, Genzel, Reinhard, additional, Davies, Ric, additional, Mendel, J. Trevor, additional, Naab, Thorsten, additional, Röttgers, Bernhard, additional, Wilman, David J., additional, Wuyts, Stijn, additional, Bandara, Kaushala, additional, Beifiori, Alessandra, additional, Belli, Sirio, additional, Bender, Ralf, additional, Brammer, Gabriel B., additional, Burkert, Andreas, additional, Chan, Jeffrey, additional, Galametz, Audrey, additional, Kulkarni, Sandesh K., additional, Lang, Philipp, additional, Lutz, Dieter, additional, Momcheva, Ivelina G., additional, Nelson, Erica J., additional, Rosario, David, additional, Saglia, Roberto P., additional, Seitz, Stella, additional, Tacconi, Linda J., additional, Tadaki, Ken-ichi, additional, Übler, Hannah, additional, and Dokkum, Pieter van, additional

Published
2016
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75. The FORS Deep Field: The Photometric Catalog

Author

The FDF-Team, Heidt, Jochen, Appenzeller, Immo, Gabasch, Armin, Seitz, Stella, Jäger, Klaus, Hensler, Gerhard, editor, Stasińska, Grażyna, editor, Harfst, Stefan, editor, Kroupa, Pavel, editor, and Theis, Christian, editor

Published
2003
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77. THE DETECTION AND STATISTICS OF GIANT ARCS BEHIND CLASH CLUSTERS

Author

Xu, Bingxiao, primary, Postman, Marc, additional, Meneghetti, Massimo, additional, Seitz, Stella, additional, Zitrin, Adi, additional, Merten, Julian, additional, Maoz, Dani, additional, Frye, Brenda, additional, Umetsu, Keiichi, additional, Zheng, Wei, additional, Bradley, Larry, additional, Vega, Jesus, additional, and Koekemoer, Anton, additional

Published
2016
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82. CLASH: EXTREME EMISSION-LINE GALAXIES AND THEIR IMPLICATION ON SELECTION OF HIGH-REDSHIFT GALAXIES

Author

Huang, Xingxing, primary, Zheng, Wei, additional, Wang, Junxian, additional, Ford, Holland, additional, Lemze, Doron, additional, Moustakas, John, additional, Shu, Xinwen, additional, Van der Wel, Arjen, additional, Zitrin, Adi, additional, Frye, Brenda L., additional, Postman, Marc, additional, Bartelmann, Matthias, additional, Benítez, Narciso, additional, Bradley, Larry, additional, Broadhurst, Tom, additional, Coe, Dan, additional, Donahue, Megan, additional, Infante, Leopoldo, additional, Kelson, Daniel, additional, Koekemoer, Anton, additional, Lahav, Ofer, additional, Medezinski, Elinor, additional, Moustakas, Leonidas, additional, Rosati, Piero, additional, Seitz, Stella, additional, and Umetsu, Keiichi, additional

Published
2015
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84. CLASH: WEAK-LENSING SHEAR-AND-MAGNIFICATION ANALYSIS OF 20 GALAXY CLUSTERS

Author

Umetsu, Keiichi, primary, Medezinski, Elinor, additional, Nonino, Mario, additional, Merten, Julian, additional, Postman, Marc, additional, Meneghetti, Massimo, additional, Donahue, Megan, additional, Czakon, Nicole, additional, Molino, Alberto, additional, Seitz, Stella, additional, Gruen, Daniel, additional, Lemze, Doron, additional, Balestra, Italo, additional, Benítez, Narciso, additional, Biviano, Andrea, additional, Broadhurst, Tom, additional, Ford, Holland, additional, Grillo, Claudio, additional, Koekemoer, Anton, additional, Melchior, Peter, additional, Mercurio, Amata, additional, Moustakas, John, additional, Rosati, Piero, additional, and Zitrin, Adi, additional

Published
2014
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85. CLASH-X: A COMPARISON OF LENSING AND X-RAY TECHNIQUES FOR MEASURING THE MASS PROFILES OF GALAXY CLUSTERS

Author

Donahue, Megan, primary, Voit, G. Mark, additional, Mahdavi, Andisheh, additional, Umetsu, Keiichi, additional, Ettori, Stefano, additional, Merten, Julian, additional, Postman, Marc, additional, Hoffer, Aaron, additional, Baldi, Alessandro, additional, Coe, Dan, additional, Czakon, Nicole, additional, Bartelmann, Mattias, additional, Benitez, Narciso, additional, Bouwens, Rychard, additional, Bradley, Larry, additional, Broadhurst, Tom, additional, Ford, Holland, additional, Gastaldello, Fabio, additional, Grillo, Claudio, additional, Infante, Leopoldo, additional, Jouvel, Stephanie, additional, Koekemoer, Anton, additional, Kelson, Daniel, additional, Lahav, Ofer, additional, Lemze, Doron, additional, Medezinski, Elinor, additional, Melchior, Peter, additional, Meneghetti, Massimo, additional, Molino, Alberto, additional, Moustakas, John, additional, Moustakas, Leonidas A., additional, Nonino, Mario, additional, Rosati, Piero, additional, Sayers, Jack, additional, Seitz, Stella, additional, Van der Wel, Arjen, additional, Zheng, Wei, additional, and Zitrin, Adi, additional

Published
2014
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87. A CONSISTENT STUDY OF METALLICITY EVOLUTION AT 0.8 < z < 2.6

Author

Wuyts, Eva, primary, Kurk, Jaron, additional, Förster Schreiber, Natascha M., additional, Genzel, Reinhard, additional, Wisnioski, Emily, additional, Bandara, Kaushala, additional, Wuyts, Stijn, additional, Beifiori, Alessandra, additional, Bender, Ralf, additional, Brammer, Gabriel B., additional, Burkert, Andreas, additional, Buschkamp, Peter, additional, Carollo, C. Marcella, additional, Chan, Jeffrey, additional, Davies, Ric, additional, Eisenhauer, Frank, additional, Fossati, Matteo, additional, Kulkarni, Sandesh K., additional, Lang, Philipp, additional, Lilly, Simon J., additional, Lutz, Dieter, additional, Mancini, Chiara, additional, Mendel, J. Trevor, additional, Momcheva, Ivelina G., additional, Naab, Thorsten, additional, Nelson, Erica J., additional, Renzini, Alvio, additional, Rosario, David, additional, Saglia, Roberto P., additional, Seitz, Stella, additional, Sharples, Ray M., additional, Sternberg, Amiel, additional, Tacchella, Sandro, additional, Tacconi, Linda J., additional, van Dokkum, Pieter, additional, and Wilman, David J., additional

Published
2014
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89. THREE GRAVITATIONALLY LENSED SUPERNOVAE BEHIND CLASH GALAXY CLUSTERS

Author

Patel, Brandon, primary, McCully, Curtis, additional, Jha, Saurabh W., additional, Rodney, Steven A., additional, Jones, David O., additional, Graur, Or, additional, Merten, Julian, additional, Zitrin, Adi, additional, Riess, Adam G., additional, Matheson, Thomas, additional, Sako, Masao, additional, Holoien, Thomas W.-S., additional, Postman, Marc, additional, Coe, Dan, additional, Bartelmann, Matthias, additional, Balestra, Italo, additional, Benítez, Narciso, additional, Bouwens, Rychard, additional, Bradley, Larry, additional, Broadhurst, Tom, additional, Cenko, S. Bradley, additional, Donahue, Megan, additional, Filippenko, Alexei V., additional, Ford, Holland, additional, Garnavich, Peter, additional, Grillo, Claudio, additional, Infante, Leopoldo, additional, Jouvel, Stéphanie, additional, Kelson, Daniel, additional, Koekemoer, Anton, additional, Lahav, Ofer, additional, Lemze, Doron, additional, Maoz, Dan, additional, Medezinski, Elinor, additional, Melchior, Peter, additional, Meneghetti, Massimo, additional, Molino, Alberto, additional, Moustakas, John, additional, Moustakas, Leonidas A., additional, Nonino, Mario, additional, Rosati, Piero, additional, Seitz, Stella, additional, Strolger, Louis G., additional, Umetsu, Keiichi, additional, and Zheng, Wei, additional

Published
2014
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90. CLASH-VLT: CONSTRAINTS ON THE DARK MATTER EQUATION OF STATE FROM ACCURATE MEASUREMENTS OF GALAXY CLUSTER MASS PROFILES

Author

Sartoris, Barbara, primary, Biviano, Andrea, additional, Rosati, Piero, additional, Borgani, Stefano, additional, Umetsu, Keiichi, additional, Bartelmann, Matthias, additional, Girardi, Marisa, additional, Grillo, Claudio, additional, Lemze, Doron, additional, Zitrin, Adi, additional, Balestra, Italo, additional, Mercurio, Amata, additional, Nonino, Mario, additional, Postman, Marc, additional, Czakon, Nicole, additional, Bradley, Larry, additional, Broadhurst, Tom, additional, Coe, Dan, additional, Medezinski, Elinor, additional, Melchior, Peter, additional, Meneghetti, Massimo, additional, Merten, Julian, additional, Annunziatella, Marianna, additional, Benitez, Narciso, additional, Czoske, Oliver, additional, Donahue, Megan, additional, Ettori, Stefano, additional, Ford, Holland, additional, Fritz, Alexander, additional, Kelson, Dan, additional, Koekemoer, Anton, additional, Kuchner, Ulrike, additional, Lombardi, Marco, additional, Maier, Christian, additional, Moustakas, Leonidas A., additional, Munari, Emiliano, additional, Presotto, Valentina, additional, Scodeggio, Marco, additional, Seitz, Stella, additional, Tozzi, Paolo, additional, Zheng, Wei, additional, and Ziegler, Bodo, additional

Published
2014
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91. CLASH: COMPLETE LENSING ANALYSIS OF THE LARGEST COSMIC LENS MACS J0717.5+3745 AND SURROUNDING STRUCTURES

Author

Medezinski, Elinor, primary, Umetsu, Keiichi, additional, Nonino, Mario, additional, Merten, Julian, additional, Zitrin, Adi, additional, Broadhurst, Tom, additional, Donahue, Megan, additional, Sayers, Jack, additional, Waizmann, Jean-Claude, additional, Koekemoer, Anton, additional, Coe, Dan, additional, Molino, Alberto, additional, Melchior, Peter, additional, Mroczkowski, Tony, additional, Czakon, Nicole, additional, Postman, Marc, additional, Meneghetti, Massimo, additional, Lemze, Doron, additional, Ford, Holland, additional, Grillo, Claudio, additional, Kelson, Daniel, additional, Bradley, Larry, additional, Moustakas, John, additional, Bartelmann, Matthias, additional, Benítez, Narciso, additional, Biviano, Andrea, additional, Bouwens, Rychard, additional, Golwala, Sunil, additional, Graves, Genevieve, additional, Infante, Leopoldo, additional, Jiménez-Teja, Yolanda, additional, Jouvel, Stephanie, additional, Lahav, Ofer, additional, Moustakas, Leonidas, additional, Ogaz, Sara, additional, Rosati, Piero, additional, Seitz, Stella, additional, and Zheng, Wei, additional

Published
2013
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92. THE CONTRIBUTION OF HALOS WITH DIFFERENT MASS RATIOS TO THE OVERALL GROWTH OF CLUSTER-SIZED HALOS

Author

Lemze, Doron, primary, Postman, Marc, additional, Genel, Shy, additional, Ford, Holland C., additional, Balestra, Italo, additional, Donahue, Megan, additional, Kelson, Daniel, additional, Nonino, Mario, additional, Mercurio, Amata, additional, Biviano, Andrea, additional, Rosati, Piero, additional, Umetsu, Keiichi, additional, Sand, David, additional, Koekemoer, Anton, additional, Meneghetti, Massimo, additional, Melchior, Peter, additional, Newman, Andrew B., additional, Bhatti, Waqas A., additional, Voit, G. Mark, additional, Medezinski, Elinor, additional, Zitrin, Adi, additional, Zheng, Wei, additional, Broadhurst, Tom, additional, Bartelmann, Matthias, additional, Benitez, Narciso, additional, Bouwens, Rychard, additional, Bradley, Larry, additional, Coe, Dan, additional, Graves, Genevieve, additional, Grillo, Claudio, additional, Infante, Leopoldo, additional, Jimenez-Teja, Yolanda, additional, Jouvel, Stephanie, additional, Lahav, Ofer, additional, Maoz, Dan, additional, Merten, Julian, additional, Molino, Alberto, additional, Moustakas, John, additional, Moustakas, Leonidas, additional, Ogaz, Sara, additional, Scodeggio, Marco, additional, and Seitz, Stella, additional

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2013
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93. GALAXY HALO TRUNCATION AND GIANT ARC SURFACE BRIGHTNESS RECONSTRUCTION IN THE CLUSTER MACSJ1206.2-0847

Author

Eichner, Thomas, primary, Seitz, Stella, additional, Suyu, Sherry H., additional, Halkola, Aleksi, additional, Umetsu, Keiichi, additional, Zitrin, Adi, additional, Coe, Dan, additional, Monna, Anna, additional, Rosati, Piero, additional, Grillo, Claudio, additional, Balestra, Italo, additional, Postman, Marc, additional, Koekemoer, Anton, additional, Zheng, Wei, additional, Høst, Ole, additional, Lemze, Doron, additional, Broadhurst, Tom, additional, Moustakas, Leonidas, additional, Bradley, Larry, additional, Molino, Alberto, additional, Nonino, Mario, additional, Mercurio, Amata, additional, Scodeggio, Marco, additional, Bartelmann, Matthias, additional, Benitez, Narciso, additional, Bouwens, Rychard, additional, Donahue, Megan, additional, Infante, Leopoldo, additional, Jouvel, Stephanie, additional, Kelson, Daniel, additional, Lahav, Ofer, additional, Medezinski, Elinor, additional, Melchior, Peter, additional, Merten, Julian, additional, and Riess, Adam, additional

Published
2013
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94. PROPERTIES OF M31. II. A CEPHEID DISK SAMPLE DERIVED FROM THE FIRST YEAR OF PS1 PANDROMEDA DATA

Author

Kodric, Mihael, primary, Riffeser, Arno, additional, Hopp, Ulrich, additional, Seitz, Stella, additional, Koppenhoefer, Johannes, additional, Bender, Ralf, additional, Goessl, Claus, additional, Snigula, Jan, additional, Lee, Chien-Hsiu, additional, Ngeow, Chow-Choong, additional, Chambers, K. C., additional, Magnier, E. A., additional, Price, P. A., additional, Burgett, W. S., additional, Hodapp, K. W., additional, Kaiser, N., additional, and Kudritzki, R.-P., additional

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2013
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95. CLASH: THREE STRONGLY LENSED IMAGES OF A CANDIDATEz≈ 11 GALAXY

Author

Coe, Dan, primary, Zitrin, Adi, additional, Carrasco, Mauricio, additional, Shu, Xinwen, additional, Zheng, Wei, additional, Postman, Marc, additional, Bradley, Larry, additional, Koekemoer, Anton, additional, Bouwens, Rychard, additional, Broadhurst, Tom, additional, Monna, Anna, additional, Host, Ole, additional, Moustakas, Leonidas A., additional, Ford, Holland, additional, Moustakas, John, additional, van der Wel, Arjen, additional, Donahue, Megan, additional, Rodney, Steven A., additional, Benítez, Narciso, additional, Jouvel, Stephanie, additional, Seitz, Stella, additional, Kelson, Daniel D., additional, and Rosati, Piero, additional

Published
2012
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96. Bright radio emission from an ultraluminous stellar-mass microquasar in M 31

Author

Middleton, Matthew J., primary, Miller-Jones, James C. A., additional, Markoff, Sera, additional, Fender, Rob, additional, Henze, Martin, additional, Hurley-Walker, Natasha, additional, Scaife, Anna M. M., additional, Roberts, Timothy P., additional, Walton, Dominic, additional, Carpenter, John, additional, Macquart, Jean-Pierre, additional, Bower, Geoffrey C., additional, Gurwell, Mark, additional, Pietsch, Wolfgang, additional, Haberl, Frank, additional, Harris, Jonathan, additional, Daniel, Michael, additional, Miah, Junayd, additional, Done, Chris, additional, Morgan, John S., additional, Dickinson, Hugh, additional, Charles, Phil, additional, Burwitz, Vadim, additional, Valle, Massimo Della, additional, Freyberg, Michael, additional, Greiner, Jochen, additional, Hernanz, Margarita, additional, Hartmann, Dieter H., additional, Hatzidimitriou, Despina, additional, Riffeser, Arno, additional, Sala, Gloria, additional, Seitz, Stella, additional, Reig, Pablo, additional, Rau, Arne, additional, Orio, Marina, additional, Titterington, David, additional, and Grainge, Keith, additional

Published
2012
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98. A magnified young galaxy from about 500 million years after the Big Bang

Author

Zheng, Wei, primary, Postman, Marc, additional, Zitrin, Adi, additional, Moustakas, John, additional, Shu, Xinwen, additional, Jouvel, Stephanie, additional, Høst, Ole, additional, Molino, Alberto, additional, Bradley, Larry, additional, Coe, Dan, additional, Moustakas, Leonidas A., additional, Carrasco, Mauricio, additional, Ford, Holland, additional, Benítez, Narciso, additional, Lauer, Tod R., additional, Seitz, Stella, additional, Bouwens, Rychard, additional, Koekemoer, Anton, additional, Medezinski, Elinor, additional, Bartelmann, Matthias, additional, Broadhurst, Tom, additional, Donahue, Megan, additional, Grillo, Claudio, additional, Infante, Leopoldo, additional, Jha, Saurabh W., additional, Kelson, Daniel D., additional, Lahav, Ofer, additional, Lemze, Doron, additional, Melchior, Peter, additional, Meneghetti, Massimo, additional, Merten, Julian, additional, Nonino, Mario, additional, Ogaz, Sara, additional, Rosati, Piero, additional, Umetsu, Keiichi, additional, and van der Wel, Arjen, additional

Published
2012
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99. CLASH: PRECISE NEW CONSTRAINTS ON THE MASS PROFILE OF THE GALAXY CLUSTER A2261

Author

Coe, Dan, primary, Umetsu, Keiichi, additional, Zitrin, Adi, additional, Donahue, Megan, additional, Medezinski, Elinor, additional, Postman, Marc, additional, Carrasco, Mauricio, additional, Anguita, Timo, additional, Geller, Margaret J., additional, Rines, Kenneth J., additional, Diaferio, Antonaldo, additional, Kurtz, Michael J., additional, Bradley, Larry, additional, Koekemoer, Anton, additional, Zheng, Wei, additional, Nonino, Mario, additional, Molino, Alberto, additional, Mahdavi, Andisheh, additional, Lemze, Doron, additional, Infante, Leopoldo, additional, Ogaz, Sara, additional, Melchior, Peter, additional, Host, Ole, additional, Ford, Holland, additional, Grillo, Claudio, additional, Rosati, Piero, additional, Jiménez-Teja, Yolanda, additional, Moustakas, John, additional, Broadhurst, Tom, additional, Ascaso, Begoña, additional, Lahav, Ofer, additional, Bartelmann, Matthias, additional, Benítez, Narciso, additional, Bouwens, Rychard, additional, Graur, Or, additional, Graves, Genevieve, additional, Jha, Saurabh, additional, Jouvel, Stephanie, additional, Kelson, Daniel, additional, Moustakas, Leonidas, additional, Maoz, Dan, additional, Meneghetti, Massimo, additional, Merten, Julian, additional, Riess, Adam, additional, Rodney, Steve, additional, and Seitz, Stella, additional

Published
2012
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100. CLASH: MASS DISTRIBUTION IN AND AROUND MACS J1206.2-0847 FROM A FULL CLUSTER LENSING ANALYSIS

Author

Umetsu, Keiichi, primary, Medezinski, Elinor, additional, Nonino, Mario, additional, Merten, Julian, additional, Zitrin, Adi, additional, Molino, Alberto, additional, Grillo, Claudio, additional, Carrasco, Mauricio, additional, Donahue, Megan, additional, Mahdavi, Andisheh, additional, Coe, Dan, additional, Postman, Marc, additional, Koekemoer, Anton, additional, Czakon, Nicole, additional, Sayers, Jack, additional, Mroczkowski, Tony, additional, Golwala, Sunil, additional, Koch, Patrick M., additional, Lin, Kai-Yang, additional, Molnar, Sandor M., additional, Rosati, Piero, additional, Balestra, Italo, additional, Mercurio, Amata, additional, Scodeggio, Marco, additional, Biviano, Andrea, additional, Anguita, Timo, additional, Infante, Leopoldo, additional, Seidel, Gregor, additional, Sendra, Irene, additional, Jouvel, Stephanie, additional, Host, Ole, additional, Lemze, Doron, additional, Broadhurst, Tom, additional, Meneghetti, Massimo, additional, Moustakas, Leonidas, additional, Bartelmann, Matthias, additional, Benítez, Narciso, additional, Bouwens, Rychard, additional, Bradley, Larry, additional, Ford, Holland, additional, Jiménez-Teja, Yolanda, additional, Kelson, Daniel, additional, Lahav, Ofer, additional, Melchior, Peter, additional, Moustakas, John, additional, Ogaz, Sara, additional, Seitz, Stella, additional, and Zheng, Wei, additional

Published
2012
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