DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

No.
object_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
observation_id
exposure
awarded_exposure
xis0_exposure
xis1_exposure
xis2_exposure
xis3_exposure
xis0_observation_mode
xis1_observation_mode
xis2_observation_mode
xis3_observation_mode
hxd_observation_mode
hxd_coarse_clock_rate_exposure
hxd_first_clock_rate_exposure
hxd_normal_clock_rate_exposure
hxd_all_clock_rate_exposure
hxd_wam_exposure
quantity_of_hxd_burst
processing_status
processing_date_mjd
processing_date
public_date_mjd
public_date
distribution_date_mjd
distribution_date
processing_version
processing_count
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
observation_type
proposal_title
main_instrument
has_xis_injection
data_access_url
ql_access_url
ql_image_url
1 SN 1987A 83.9013 -69.2655 83.9928 -69.294887 307.391677 -86.458548 279.69660922 -31.92548266 330.0004 53894.6930555556 2006-06-08 16:38:00 53895.6683449074 2006-06-09 16:02:25 801090010 39.6464 40 39.6464 39.6464 39.6464 39.6464 2 2 2 2 1 0 0 39.2519 39.2519 84.2399 0 PROCESSED 57534.6267592593 2016-05-26 15:02:32 54400 2007-10-27 00:00:00 53928.1346527778 2006-07-12 03:13:54 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 012006 In an early Suzaku observation during the SWG time in November 2005 we have already obtained an excellent XIS spectrum. The flux of SN 1987A continues to rise exponentially with an e-folding time of ~800 days. The abundances in the ejecta could be measured with unprecedented accuracy. We confirm that Oxygen and Iron are significantly underabundant with respect to other elements, indicating the formation of dust, maybe even black rust grains (Fe3O4). We propose to monitor the chemical evolution of SN 1987A with Suzaku for 40 ksec in AO-1, where we expect about twice the previous flux. The exponential brightening and the chemical abundance is expected to change, when the full inner ring is engulfed. Simultaneously we can search for a periodic hard signal from the putative pulsar. EXTRAGALACTIC DIFFUSE SOURCES 8 B G NTHER HASINGER EUR 1 AO1 SN 1987A - A RUSTY REMNANT? XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801090010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '801090010'

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