[Starburst classics] [Starburst recent] [High-z star form.] [UV] [ULIRGs] [dwarves] [HI]
Recent articles relevant to
High-redshift star formation
- rest frame UV - optical
- Richards et al. (1999, ApJL accepted(?);
astro-ph/9909251)
I & K HST phot of 1.4 & 8.5 GHz sources; unidentified sources starbursts?
- Hogg et al. (1999, ApJS accepted;
astro-ph/9909360)
Ground based source detection to G=26 in HDF region by Caltech group.
- Cotter et al. (1999, Hy-redshift universe conf.;
astro-ph/9910059
From ground, confusion and incompleteness understimate U-dropout density.
- Waddington et al. (1999, ApJL accepted;
astro-ph/9910069)
z=4.2 microJy radio source imaged with NICMOS.
- Lanzetta et al. (1999, Hy-z Univ. proc.;
astro-ph/9910554)
photometric redshifts: UV density increasing out to z> ~5?
- Liu. (1999, Phot. z's of high-z gals. proc.;
astro-ph/9910571)
photometric redshifts of starbursts
- Crampton & Lilly (1999 conf proc.;
astro-ph/9911227)
Using multislits combined with filters to find em galaxies between atmospheric lines.
- Stockton (1999, Galaxy morph mtg;
astro-ph/9911342)
similr to Crampton & amp;Lilly above.
- Adelberger (1999, "Clustering at High Redshift" proc.;
astro-ph/9912153)
hi-z surveys review. 850 micron SCUBA detections detected in optical?
- Adelberger & Steidel (2000,
astro-ph/0001126):
quantifies accuracy of IRX/beta (0.3 dex), applies to LBGs, Balmer break systems.
- Narrow band imaging
- Steidel et al. (1999, ApJ accepted(?);
astro-ph/9910144)
Narrow band Ly-alpha imaging of galaxies in a z=3.09 overdensity. Two curious 100 kpc blobs
- rest frame FIR
- Harwitt (1999, ApJL, 510, L83)
Cosmic IR (FIR to sub-mm) background.
- Lagache & Puget (1999, A&A accepted;
astro-ph/9910255)
170µm COSMIC FIR backkground fluctions from ISOPHPOT.
- Combes (1999,
astro-ph/9909016)
Gas & dust in protogalaxies.
- Blain et al, (1999, ApJL, 512, L87)
Deep Sub-mm counts: most radiation from z < 2.
- Chapman et al., (1999, MNRAS submitted;
astro-ph/9909092)
Look for submm counterparts to Ly break gals.
- Pontopiddan & Wiklind (1999, Conf proc.;
astro-ph/9909352)
SED distortion of high-z ULIRGs by differential lensing
- Sanders (1999, New millenium galaxy morph. conf.;
astro-ph/9910028)
SCUBA review.
- Blain et al. (1999, MNRAS submitted;
astro-ph/9911108)
expected hi-z FIR-submm line detections with upcoming arrays.
- Peacock et al. (1999, MNRAS submitted;
astro-ph/9911108)
HDF comparison of 850 micron residual map and UV: factor 4-6 of hidden star formation.
- Busswell & Shanks (2000, MNRAS, submitted;
astro-ph/0002081)
FBGs & Calzetti extinction can account for most SCUBA counts except bright end
- Hughes (2000, Evolution of galaxies on cosmological timescales proc.;
astro-ph/0003414)
Review of sub-mm results, future prospects
- Rest frame radio
- Norris et al. (1999, submitted to "Perspectives in Radio Astronomy: ...";
astro-ph/9910437)
Multi-frequency ATCA radio obs of HDF-S.
- Richards (1999, Science with the Atacama Large Array meeting;
astro-ph/9910497)
High resolution radio imaging of SCUBA sources.
- Richards (1999, UVa thesis;
astro-ph/9910526)
Radio properties, distant galxies.
- Garrett et al. (2000, in "The Universe at low radio frequencies";
astro-ph/0001523)
New deep Westerbork 1.4GHz observations, rms noise 8 micro-Jy.
- SED theory
- Jimenez et al. (1999, ApJ submitted;
astro-ph/9910279)
Theoretical UV-mm SEDs of proto-gals
- Rocca-Volmerange & Fioc (2000, "A new millenium in glaxy morphology";
astro-ph/0001398)
SFH as a function of type: reconciling Cowie and Lilly SFR(z)
- Simulations
- Davé et al. (1999, Clustering at high z rencontres;
astro-ph/9910220)
cosmological hydro sims LCDM making z=3 LBGs "need" dust.
- Sommerville et al (1999, 15th IAP meeting proc.;
astro-ph/9910346)
N-body simulations of mergers at z=3 -> simulated HST images.
- Wood & Loeb (1999, ApJ submitted;
astro-ph/9911316)
Escape fraction of ionizing photons in starbursts and mini-QSOs as a fn(z).
[Starburst classics] [Starburst recent] [High-z star form.] [UV] [ULIRGs] [dwarves] [HI]
Page maintained by
Gerhardt Meurer (meurer@pha.jhu.edu)
Timid texture background