A Matched-Filter Analysis of the Tidal Tails of the Globular Cluster Palomar 5

By C. Rockosi, M. Odenkirchen, E. Grebel, W. Dehnen, K. Cudworth, James E. Gunn, D. York, J. Brinkmann, G. Hennessy, Željko Ivezic´. 2002

188 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/54be9b200b7b7204971b0e8ed56fa4e43331c271

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In Astronomy and Astrophysics

1. Hans-Walter Rix
2. Jo Bovy
3. C. Conroy
4. D. Schneider
5. S. Majewski
6. P. Hopkins
7. A. Helmi
8. Simon D. M. White

In Instrumentation

1. Hans-Walter Rix
2. M. Blanton
3. C. Conroy
4. Jo Bovy
5. David W. Hogg
6. D. Schneider
7. A. Helmi
8. I. Minchev

Citations in the corpus

• A New Milky Way Companion: Unusual Globular Cluster or Extreme Dwarf Satellite? (2004, background): “The density contours do not exhibit obvious evidence of tidal stripping, such as that seen around Pal 5 (Rockosi et al. 2002; Odenkirchen et al. 2003) and numerous other Milky Way GCs (Leon et al. 2000).”
• ASSESSING THE MILKY WAY SATELLITES ASSOCIATED WITH THE SAGITTARIUS DWARF SPHEROIDAL GALAXY (2010, background): “Pal 5 has also been shown to have lengthy (∼ 20◦), well-defined tidal tails of its own (Odenkirchen et al. 2001, 2003; Rockosi et al. 2002; Grillmair & Dionatos 2006) and these provide another indicator of the direction of motion (although see Odenkirchen et al. 2009).”
• A Low-Latitude Halo Stream around the Milky Way (2003, unknown): “…of our Milky Way galaxy have been documented (Odenkirchen et al. 2001; Mateo, Olszewski & Morrison 1998; Majewski et al. 1999; Martinez-Delgado et al. 2001; Vivas et al. 2001; Rockosi et al. 2002; Kundu et al. 2002; Bellazzini, Ferraro, & Ibata 2002) in spatial star-density and kinematic studies.”
• A Two Micron All Sky Survey View of the Sagittarius Dwarf Galaxy. I. Morphology of the Sagittarius Core and Tidal Arms (2003, background): “…is positive toward the Galactic 11 S-shaped structures have been seen in the case of, e.g., the globular cluster Palomar 5 (Odenkirchen et al. 2001a, 2003; Rockosi et al. 2002) and the Ursa Minor dSph (Palma et al. 2003)—both systems for which our perspective is nearly edge-on to the orbital plane.”
• CONSTRAINING THE MILKY WAY POTENTIAL WITH A SIX-DIMENSIONAL PHASE-SPACE MAP OF THE GD-1 STELLAR STREAM (2009, methodology): “The matched filter technique (Odenkirchen et al. 2001; Rockosi et al. 2002) has revealed the beautiful tidal stream of Palomar 5.”
• FOUR NEW STELLAR DEBRIS STREAMS IN THE GALACTIC HALO (2008, methodology): “Once the color-magnitude distribution of the stars of interest has been constructed, an optimal filter requires that this distribution be divided by the corresponding distribution of field stars (e.g. Rockosi et al. (2002)).”
• The Detection of a 45° Tidal Stream Associated with the Globular Cluster NGC 5466 (2006, methodology): “Among the first discoveries in the Sloan Digital Sky Survey (SDSS) data were the remarkably strong tidal tails of Palomar 5 (Odenkirchen et al. 2001; Rockosi et al. 2002; Odenkirchen et al. 2003), spanning over 10 • on the sky.”
• A Comprehensive Maximum Likelihood Analysis of the Structural Properties of Faint Milky Way Satellites (2008, background): “This object is of particular interest as it is known to be tidally disrupting in the gravity field of the Milky Way and shows beautiful stellar tidal tails (Odenkirchen et al. 2001b; Rockosi et al. 2002; Grillmair & Dionatos 2006).”
• Star Cluster Demographics. I. A General Framework and Application to the Antennae Galaxies (2006, methodology): “We are familiar with the process both observationally (e.g., Wielen 1971; Bica et al. 2001; Rockosi et al. 2002) and theoretically (e.g., Fall & Zhang 2001; Vesperini & Zepf 2003; Baumgardt & Makino 2003).”
• Theoretical isochrones in several photometric systems. II. The Sloan Digital Sky Survey ugriz system (2004, background): “Its current mass is only 4.5 to 6· 103 M⊙ (Odenkirchen et al. 2002), and it is undergoing significant tidal disruption as evidenced by its two well-defined, symmetric tidal tails (Odenkirchen et al. 2001a, 2003; Rockosi et al. 2002).”
• Chemical tagging with APOGEE: Discovery of a large population of N-rich stars in the inner Galaxy (2016, background): “Moreover the tidal evaporation of halo GCs through interaction with the Galactic potential has been spotted in real time (e.g., Rockosi et al. 2002; Odenkirchen et al. 2003; Belokurov et al. 2006a), and must be responsible for at least part of the population of N-rich stars detected in the halo by…”
• An Improved Proper-Motion Catalog Combining USNO-B and the Sloan Digital Sky Survey (2004, unknown): “…database of stellar photometry for the study of stellar populations and Galactic structure, and indeed much work as been done in these areas to date (e.g., Harris et al. 2003; Yanny et al. 2003; Hawley et al. 2002; Margon et al. 2002; Newberg et al. 2002; Rockosi et al. 2002; Ivezić et al. 2000).”
• SEGUE: A SPECTROSCOPIC SURVEY OF 240,000 STARS WITH g = 14–20 (2009, unknown): “…serendipitous Galactic structure, Galactic halo, and M31 halo science results; see Ivezic et al. (2000); Yanny et al. (2000); Newberg et al. (2002); Rockosi et al. (2002); Willman et al. (2005); Yanny et al. (2003); Newberg et al. (2003); Zucker et al. (2004a,b); Belokurov et al. (2006a,b);…”
• Comparing the properties of local globular cluster systems: implications for the formation of the Galactic halo (2004, background): “5 (rc = 21.93 pc) has been found to possess massive tidal tails (Odenkirchen et al. 2001; Odenkirchen et al. 2002; Odenkirchen et al. 2003; Rockosi et al. 2002), and is hence inthe process of being tidally disrupted.”
• Detection of a 63° Cold Stellar Stream in the Sloan Digital Sky Survey (2006, unknown): “In addition to the large-scale features attributed to past galaxy accretion events (Yanny et al. 2003; Majewski et al. 2003; Rocha-Pinto et al. 2004), SDSS data were used to detect the remarkably strong tidal tails of Palomar 5 (Odenkirchen et al. 2001; Rockosi et al. 2002; Odenkirchen et al. 2003).”