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Replication Data for: YSOVAR: Mid-infrared Variability in the Star-forming Region Lynds 1688
May 15, 2015
Guenther, Hans Moritz, 2015, "Replication Data for: YSOVAR: Mid-infrared Variability in the Star-forming Region Lynds 1688", https://doi.org/10.7910/DVN/LNRC6A, Harvard Dataverse, V1
This dataset contains all YSOVAR lightcurves of L1688 as published in YSOVAR: Mid-infrared Variability in the Star-forming Region Lynds 1688. The data has been processed and cleaned as described in that article. Please note that additional electronic data (e.g. a table of source properties) is included in the article and is available from CDS.
Replication data for: The disk-bearing young star IM Lupi. X-ray properties and limits on accretion
May 15, 2013
Günther, H. M; Matt, S. P.; Schmitt, J. H. M. M.; Güdel, M.; Li, Z.-Y.; Burton, D. M., 2013, "Replication data for: The disk-bearing young star IM Lupi. X-ray properties and limits on accretion", https://doi.org/10.7910/DVN/TO6U8U, Harvard Dataverse, V1
This archive contains the AAO data used in the referenced publication. The Chandra and ESO/HARPS data can be downloaded from the respective institutional archives. Some information on the data format is below, see the original publication for details. The reduced spectra have not been spliced together and the continuum fitting is not perfect in the...
UBVRI photometry of star forming regions
May 15, 2013
Günther, Hans Moritz, 2013, "UBVRI photometry of star forming regions", https://doi.org/10.7910/DVN/GOIM4Y, Harvard Dataverse, V1
This dataset contains UBVRI catalogs for the following star forming regions: alpha Per, IRAS 20050+2720, Lk Ha 101, NGC 281, Orion (not the ONC, but the less dense "hokey stick" region). The catalogs are merged form observations that were carried out over 4 nights from 2009-11-18 to 2009-11-21 at the Fred Lawrence Whipple Observatory. Optical photo...
Replication data for: Simulating the X-ray emission from accretion shocks on T Tauri stars
Feb 12, 2013
Günther, Hans Moritz, 2012, "Replication data for: Simulating the X-ray emission from accretion shocks on T Tauri stars", https://doi.org/10.7910/DVN/CAQG1T, Harvard Dataverse, V2
Classical T Tauri stars (CTTS) are surrounded by actively accreting disks. According to current models material falls along the magnetic field lines from the disk with more or less free-fall velocity onto the star, where the plasma heats up and generates X-rays. We want to quantitatively explain the observed high energy emission and measure the inf...
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