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2 Nov 2017: Follow-up Hubble Space Telescope observations in Adams et al. Existing HST precursor images (top), new 2015 images (middle) and near-infrared images (bottom).

1 Mar 1998: Deep optical surveys combined with the renaissance of interest in large area surveys at all wavelengths are fundamental in searching for rare types of object, discovering new categories of object, and ... Quality control will be assured by a rigorous and

5 Nov 2023: the eccentricity of the new orbit e2.

27 Aug 2022: 4355. 91. R. MacDonald and N. Madhusudhan, HD 209458b in New Light: Detection of Nitrogen Chemistry, Patchy. ... Matsumura, T-S. Pyo, Deep Thermal Infrared Imaging of HR 8799 bcde: New.

7 Feb 2008: Stochastic evolution of small grains and dynamical excitation. Indirect detection of planets and discovery of new phenomena. ... Indirect detection of planets and discovery of new phenomena. Constraining planet properties and comet population.

5 Jul 2018: 1950s. AlpherGamowHermanHayashi. BBN CMB. = New Physics? BBN CMB. = New Physics?

15 Aug 2023: 15/08/2023 2. Astronomy Job Opportunities for New Ph.D. Graduates. Paul Hewett. ... working environment/support compared to academia. Institute of Astronomy “astro-jobs” presentation. Astronomy Job Opportunities for New Ph.D.

18 Jul 2006: The Panel strongly recommends that the PI submits a new proposal which focused on the science that can be achieved by covering the whole southern sky in JK only.

29 Sep 2023: 2.4.3 Tidal Locking. Remember:. Note that at New Moon we only see Earth-shine.

16 Sep 2016: origin. Show that the new orbit of a dust grain with a given β has a semimajor axis ad andeccentricity ed given by.

30 Sep 2015: While you may have many ideas and projects from your PhD to continue in your first postdoc, don’t let this stop you from developing new collaborations with people at your

16 Nov 2017: more tightly constrained via observations?• From the upper end, new studies of supernovae progenitors, as in Star of the Week #2, now making progress• From the lower end, use observations of

30 Oct 2022: new NACRE data basis (Angulo et al.

15 Sep 2019: During your PD phase make sure to work on (some) new ideas with new people. – ... It’s a very good opportunity to widen your scope, learn something new, move to a different subfield, etc.

14 May 2009: Moshut. Woodbury, New York : American Institute of Physics, 1998. (AIP conference proceedings ; 428), p.499. ... S. Young, and D. F. Buscher. A new photon counting spectrometer for the COAST.

5 Oct 2010: def@subeqnnum{{reset@fontrm (thesubequation)}} % % A new label command to refer to subequations.

9 Oct 2015: v22 v21) 4(Mp/M)2ǫ21 v5pv3. Hence show that the new orbit has a semimajor axis with a corresponding ǫ2 thatsatisfies.

15 Oct 2017: The new line-width determination scheme is the key to the project.From Clewley et al., 2002, MNRAS, 337, 87.

5 Oct 2006: If yes, explain why the need for new data. Are the data requested in this proposal on the ESO Archive (http://archive.eso.org)?

7 Oct 2021: This Figure, reproduced from Böhm etal. (2009), shows the radial velocities of the two stars measured with near-continuousobservations during 14 nights at the 1 m Mt John (New Zealand) telescope