Publications based on observation at Calar Alto


Footnote to be included in your articles

The bibliographic data of any publications based on observations at Calar Alto are to be communicated to CAHA as described on our web page:

http://www.caha.es/CAHA/Applications/index.html

Publications must contain a footnote as follows: 

Based on observations collected at Centro Astronómico Hispano en Andalucía (CAHA) at Calar Alto, operated jointly by Instituto de Astrofísica de Andalucía (CSIC) and Junta de Andalucía

Publications based on data collected before January 1st 2019 must contain a footnote as follows: 

Data here reported were acquired at Centro Astronómico Hispano Alemán (CAHA) at Calar Alto operated jointly by Instituto de Astrofísica de Andalucía (CSIC) and Max Planck Institut für Astronomie (MPG). Centro Astronómico Hispano en Andalucía is now operated by Instituto de Astrofísica de Andalucía and Junta de Andalucía.

Search by author/co-author, year of publication or part of the publication title:
1st Author Publication Title Year
J.A. Combi Multi-wavelength properties of the high-energy bright Seyfert 1 galaxy IGR J18027-1455 2006

Multi-wavelength properties of the high-energy bright Seyfert 1 galaxy
IGR J18027-1455

J. A. Combi, M. Ribó, J. Martí, S. Chaty

A&A 458,761

C. Trachternach An optical search for low surface brightness galaxies in the Arecibo HI Strip Survey 2006

An optical search for low surface brightness galaxies in the Arecibo
HI Strip Survey

C. Trachternach - D. J. Bomans - L. Haberzettl - R.-J. Dettmar

A&A 458,341

A. Just An evolutionary disc model of the edge-on galaxy NGC 5907 2006

An evolutionary disc model of the edge-on galaxy NGC 5907

A. Just, C. Möllenhoff, A. Borch

A&A 459,703

E. Mazzotta The dust coma of the active Centaur P/2004 A1 (LONEOS): a CO-driven environment? 2006

The dust coma of the active Centaur P/2004 A1 (LONEOS): a CO-driven
environment?

E. Mazzotta Epifani, P. Palumbo, M. T. Capria, G. Cremonese, M. Fulle, L. Colangeli

A&A 460,935

Racine The Strehl Efficiency of Adaptive Optics Systems 2006

The Strehl Efficiency of Adaptive Optics Systems

René Racine PASP

118,1066

Buyle The v_c-sigma_c relation in low-mass and low surface brightness galaxies 2006

The vcc relation in low-mass and low surface brightness galaxies

P. Buyle, L. Ferrarese, G. Gentile, H. Dejonghe, M. Baes, U. Klein

MNRAS 373,700

R.E.M.Griffin Composite spectra Paper 14: HR 1129, a long-period binary showing evidence of circumbinary materia 2006

Composite spectra Paper 14: HR 1129, a long-period binary showing
evidence of circumbinary material

R. E. M. Griffin, R. F. Griffin, D. J. Stickland

MNRAS 373,1351

W.J.Frith New H-band galaxy number counts: a large local hole in the galaxy distribution 2006

New H-band galaxy number counts: a large local hole in the galaxy
distribution

W. J. Frith, N. Metcalfe, T. Shanks

MNRAS 371,1601

S. Taubenberger SN 2004aw: confirming diversity of Type Ic supernovae 2006

SN 2004aw: confirming diversity of Type Ic supernovae

S. Taubenberger, A. Pastorello, P. A. Mazzali, S. Valenti, G. Pignata,D. N. Sauer, A. Arbey, O. Bärnbantne, S. Benetti, A. Della Valle,J. Deng, N. Elias-Rosa, A. V. Filippenko, R. J. Foley, A. Gooba, R. Kotak,
W. Li, P. Meikle, J. Mendez, F. Patat, E. Pian, C. Ries, P. Ruiz-Lapuente,
M. Salvo, V. Stanishev, M. Turatto, W. Hillebrandt
MNRAS 371,1459

M. Kun Low-mass star formation in Lynds 1333 2006

Low-mass star formation in Lynds 1333

M. Kun, S. Nikolic, L. E. B. Johansson, Z. Balog, A. Gáspár

MNRAS 371,732

N. Metcalfe Galaxy number counts - VI. An H-band survey of the Herschel Deep Field 2006

Galaxy number counts - VI. An H-band survey of the Herschel Deep Field

N. Metcalfe, T. Shanks, P. M. Weilbacher, H. J. McCracken, R. Fong,D. Thompson

 MNRAS 370, 1257

J.R. MAund Faint supernovae and supernova impostors: case studies of SN 2002kg/NGC 2403-V37 and SN 2003gm 2006

Faint supernovae and supernova impostors: case studies of SN 2002kg/NGC 2403-V37 and SN 2003gm

J. R. Maund, S. J. Smartt, R.-P. Kudritzki, A. Pastorello, G. Nelemans, F. Bresolin, F. Patat, G. F. Gilmore, C. R. Benn

MNRAS 369,390

R.F. Griffin Comment on 'The case and fate of HD 75767 – neutronstar or supernova?' by Fuhrmann et al. 2006

Comment on 'The case and fate of HD 75767 – neutron
star or supernova?' by Fuhrmann et al.

R. F. Griffin

MNRAS 368,1359

B. Rockenfeller Multiband photometric detection of a huge flare on the M9 dwarf 2MASSW J1707183+643933 2006

Multiband photometric detection of a huge flare on the M9 dwarf
2MASSW J1707183+643933

B. Rockenfeller, C. A. L. Bailer-Jones, R. Mundt, M. A.Ibrahimov

MNRAS 367,407

 

A.D. Barnes On the origin of the absorption features in SS 433 2006

On the origin of the absorption features in SS 433

A. D. Barnes, J. Casares, P. A. Charles, J. S. Clark, R. Cornelisse, C. Knigge,D. Steeghs

MNRAS 365, 296

C. Hoyos The impact of the visibility of the [OIII]l4363 line on the general properties of HII galaxies in 2006

The impact of the visibility of the [OIII]λ4363 line on the general properties of HII galaxies in the Local Universe

C. Hoyos, A.I.Diaz

MNRAS 365,454

J.B. Haislip A photometric redshift of z=6.39 +-0.12 for GRB050904 2006

A photometric redshift of z=6.39 +-0.12 for GRB050904

J.B. Haislip et al.

Nature 440,181

M. Ammler Characterisation of young nearby stars -- The Ursa Major group 2006

Characterisation of young nearby stars -- The Ursa Major group

M. Ammler

PhD thesis  

S. F. Sánchez A new technique for decoupling the host and nuclear spectra of type I AGNs using integral field sp 2006

A new technique for decoupling the host and nuclear spectra of
type I AGNs using integral field spectroscopy

S. F. Sánchez, B. García-Lorenzo, K. Jahnke, E. Mediavilla, J. I. González-Serrano, L. Christensen, L. Wisotzki

AN 327,167

M. Villar-Martín The giant Lyalpha nebula associated with a z = 2.5 radio galaxy 2006

The giant Lyalpha nebula associated with a z = 2.5 radio galaxy

M. Villar-Martín, S. F. Sánchez, R. Peletier, J. Vernet, C. de Breuck, A. Humphrey, S. di Serego Alighieri, R. Fosbury, D. Stern

AN 327,187