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22 Mar 2024: Therefore, tackling a prime objective of exoplanet science and understanding how unique or common planets like our Earth are in our galactic neighborhood will require a new, dedicated approach. ... below). 15. 2.3 Timing for a space-based mid-infrared

6 Nov 2018: In both cases, we find no evidence for. new physics. The Planck results for base CDM are in good agreement with baryon acoustic oscillation data and with the JLA sample of

24 Jan 2003: pointing - a telescope slew to position with new guide star acquisition.

10 Nov 1998: New blocking filters New blocking filters shall be added to CIRSI in Oct 98. ... These new filters have predicted peak throughput of 90% in H compared with 52% for the blocking filters used in May/June 1998.

7 Oct 2011: 2003;Bonsor et al. 2011). Bonsor et al. (2011) estimated the amount ofdestabilised material simply by expanding theµ2/7 zone accordingto the new, lower, stellar mass. ... While this will correctly describethe new chaotic zone at low eccentricity,

8 Jul 2009: Discs were detected with moderate frequencyfor stars a few hundred Myr old, but no new detections were madefor ages comparable to the Sun’s 4.5 Gyr. ... No new discover-ies were made among the 13 stars observed, but the Infrared SpaceObservatory (ISO)

sure that update is also set to yes for dogemini so that the new entries are written to the data when the task is run.

6 Oct 2000: Maximun priority is given to the zone -3º to -9º the same zone observed in San Fernando for the Astrophotographic Catalogue in order to computes proper motions using new measures of ... In 1991 the original declination glass circle was changed for a

18 Jan 2000: This new instrument offers unique opportunities for the UK/NL communities to execute high resolution, deep, wide field optical imaging surveys. ... give an indication of when new data will be available for download.

8 Oct 2018: Bruno was born in 1548,five years after Copernicus died. Between the years 1582 and 1592 he wasthe one who persistently, openly and actively spread the news about the“universe” that

10 Jul 2003: A possible observing strategy might be: JHK, move to new field, JHK etc. ... SJW has this new idea of a Survey Food Taster - a science verifier?

16 Jun 2015: The command will not create a new image if an existing image has the same name. ... Note that new images can be initialised to any value when they are created with the imcreate command.

16 Jun 2015: Package loading. The TCL system contains a mechanism for finding automatically searching and loading new packages to if a command is used which isn't in the currently loaded set. ... The system must be able to issue commands to the telescope to acquire

22 Mar 2024: Science (New York, N.Y.) 233,869–72 (1986). [21] Maurette, M., Brack, A., Kurat, G., Perreau, M. &

19 Mar 2003: Updated after detailed feedback from Steve Warren 23rd January 2003. Updated with new timescales 18th March. ... with some tuning during commissioning and science verification. Further products ---------------- PSF generation methods, oversampled

6 Nov 2018: sources of noise in microwave satel-lite communications at Bell Laboratories in New Jersey.4 Their discoverywas announced alongside the interpretation of the CMB as relic thermalradiation from the Big Bang

New CIRPASS ARGON spectra at all wavlength ranges. IDISPLAY doesn't seem to run in PyRaf.

16 Jun 2015: in_outfi= fibpos_paschenJ.list Name of file to contain the new position informa in_noise= 10 background noise in image in_sigma= 10 sigma above background which indicates a line

16 Jun 2015: Although this model provides a number of important safety features for the new user, you cannot forget to save changes to an image or lose data because of a crash, there ... Instead of loading an image changing it and then saving the result you must copy

8 Mar 2006: GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad band background. ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of 0.1 per cent are needed compared with 1%

19 Apr 2006: A new 850-µmimage shows that there is indeed such a debris disc, extending out to 55 au (15 arcsec)radius.

16 Jun 2015: 3.0 Sept 1996 Richard McMahon (IoA) [rgm@ast.cam.ac.uk] %% Conversion to Latex substyle %% %% 3.1 July 1997 Bill Martin and Vik Dhillon (RGO) %% Released to community for new ... AAO) %% Increased space for Section 14 - Related Applications %% %% 3.5

15 Apr 2006: Infrared OH Sky Observations: Mahaira etal, 1993, PASP. GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of

16 Jun 2015: With the advent of the new 1024. 2. arrays this restriction is removed and it is possible to do the OH suppression in software (digital suppression) by simply capturing the spectra

16 Jun 2015: im_ - Pointer to an image created with new(). h_ - Handle.

12 Oct 2021: Further analysis of the current detections is also leading to new insights, such as a correlation ofplanetesimal belt radius with stellar mass [66]. ... LIDT-DD: A new self-consistent debris disc model that includesradiation pressure and couples

10 Nov 2010: 5. Discussion and conclusions. Using new mid-IR images at 18 and 25µm, we have confirmedthe previously observed brightness asymmetry discovered byTelesco et al. ... 350,Hipparcos, the New Reduction of the Raw Data. Wahhaj, Z., Koerner, D.

28 Jan 2020: Here we present new anddeep ALMA observations of TRAPPIST-1 to look for an exo-Kuiper belt which canprovide clues about the formation and architecture of this system. ... This is due to its high sensitivity andthe longer wavelength, being more sensitive

22 Mar 2024: We describethe new mid-IR observations of Beta Pic in Section 2 and the datareduction procedures in Section 3. ... 5 DISCUSSION. In the following sections, we discuss new constraints that can beobtained in light of the newobservations under theories

4 Jun 1999: Further improvements of this are planned. Note that most extant image display programs do not recognise the RA--ZPX and DEC--ZPX keywords even though it is the new WCS standard

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.

22 Oct 2003: 0.2. 2003-Feb-10. all. Tables include comment records; new headers including "TSCAN"s. ... New section on contents of HDS container. New astrometric (WCS) headers: CDi_j and PV1_n.

23 Jan 2003: with some tuning during commissioning and science verification. Further products ---------------- PSF generation methods, oversampled spatially varying PSFs good news, how to form them cf.

16 Jun 2015: The essential tasks required at the telescope are:. display a reconstructed broad-band image (with the option to save this image into a new FITS file).

16 Nov 2021: a new solution for a star of a different totalmass M ′ simply by multiplying the other physical variables by appropriatescaling factors.

11 Jun 2004: APM building news 8. AOB Minutes ------- 1. Actions from last meeting STH has made no progress regarding the spatial systematics in the UFTI standards data and new test data. ... Continuing Actions ------------------ STH finish looking at the spatial

24 Aug 2007: VISTA news - pipeline progress - cold camera test data from Paranal - VISTA QC and operations 7. ... 5. WFCAM news All of the available WFCAM raw data for 06B has arrived.

22 Mar 2024: In order to do so, we de-velop a new extension of Frankenstein (Jennings et al. ... The new version of frank includes now an option to consider opticallythin or thick emission.

22 Mar 2024: any detections of circumstellar dust emission. These data provide new limits on dust belt fractional luminosities and. ... 2007a). Najita et al. (2022) used new coagulation models to assess the possibility that the observed population of cold debris.

15 Aug 2003: He is in touch with Bertin to further this. JRL asked about the parameter order in the new catalogue software. ... There has been no further news about the new job contracts.

18 Jul 2006: 6. WFCAM news (Non)linearity saga - this one could run for a long time. ... 7. VDFS news PSB reported that he had a productive visit to RAL and that he has returned with 270 files - all with full headers.

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

18 May 2004: ESO PDR news 5. Update quarterly plan 04Q2 6. Status WFCAM test data 7. ... carry out further checks on the new WFCAM test data MJI ask for more news on WFCAM status at tonight's JAC telecon.

21 Oct 2006: Progress is being made - ongoing EGS has made the new ING archive interface the default one. ... He also noted that various UKIRT new project Letters of Intent were being circulated to those likely to interested.

1 Sep 2005: Review of UKIDSS meeting 5. Upcoming VDUC meeting 6. WFCAM news and JAC telecons 7. ... 10. AOB monthly reports, hardware MJI said that two new disc servers (8 TBytes each) have been ordered.

12 Sep 2003: Preparation for camera design review meeting 7. AOB: (in)visibility of CASU web pages on new IoA web site Minutes ------- 1. ... Comments on WFAU minutes No new minutes were available since the previous CASU meeting, so there were no comments.

6 Apr 2004: STH said that he would do this. STH has made no progress regarding the spatial systematics in the UFTI standards data and new test data - ongoing JRL has reached agreement with ... for the refurbishment works, including a new roof and some new windows,

14 Feb 2008: PSB also requested that we consider purchasing a new colour printer to replace the current one. ... updated SMPs for VISTA public surveys MJI PSB investigate new colour printer options and report back at next meeting.

In order to implement the new tasks the CIRPASS package should be reinstalled. ... For _ms.fits files the new task MEFARITH2 handles the alternate file format.

6 Nov 2006: Tests are underway on the new baffling tube which should cut out remaining Moon glint problems. ... New acquisition hardware has been installed and still has a few teething troubles.