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NICMOS Observations of Extragalactic Cepheids. I. Photometry Database and a Test of the Standard Extinction Law

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arxiv astro-ph/0102125 v1 pith:LLFAYXUR submitted 2001-02-07 astro-ph

classification astro-ph
keywords distanceextragalacticwerecepheidsmoduliobservationsobtainedphotometry
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We present the results of near-infrared observations of extragalactic Cepheids made with the Near Infrared Camera and Multi-Object Spectrometer on board the Hubble Space Telescope. The variables are located in the galaxies IC 1613, IC 4182, M 31, M 81, M 101, NGC 925, NGC 1365, NGC 2090, NGC 3198, NGC 3621, NGC 4496A and NGC 4536. All fields were observed in the F160W bandpass; additional images were obtained in the F110W and F205W filters. Photometry was performed using the DAOPHOT II/ALLSTAR package. Self-consistent distance moduli and color excesses were obtained by fitting Period-Luminosity relations in the H, I and V bands. Our results support the assumption of a standard reddening law adopted by the HST Key Project on the Extragalactic Distance Scale. A companion paper will determine true distance moduli and explore the effects of metallicity on the Cepheid distance scale.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. The potential broader complex linked to the key Cepheid SV Vul

    astro-ph.SR 2026-07 conditional novelty 5.0 of 10

    SV Vul and its host cluster Alicante 13 lie at 2.30 ± 0.13 kpc and may share a common origin with the nearby cluster Liu-Pang 1738.

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