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 SNR 1987A 83.833 -69.2775 83.924877 -69.307216 307.543742 -86.433259 279.71430694 -31.94790633 135.9732 56233.5143981482 2012-11-02 12:20:44 56234.854375 2012-11-03 20:30:18 707020010 81.2764 80 81.2764 81.2844 0 81.2924 2 2 0 2 1 0 0 78.5842 78.5842 115.7599 0 PROCESSED 57607.9555439815 2016-08-07 22:55:59 56611 2013-11-15 00:00:00 56245.4956365741 2012-11-14 11:53:43 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 071331 Despite extensive observations of supernova remnant (SNR) 1987A with Chandra and XMM-Newton, the origin of the hard band (3-10 keV) X-ray emission is elusive (thermal vs nonthermal). A straightforward way to discriminate the thermal and nonthermal origins of the hard X-rays is to detect Fe K lines. The Suzaku XIS provides a uniquely efficient opportunity for a sensitive search for the Fe K lines, which is an excellent complement to the existing Chandra and XMM-Newton studies of SNR 1987A. Thus, we propose an 80 ks Suzaku observation of SNR 1987A. EXTRAGALACTIC COMPACT SOURCES 7 C SANGWOOK PARK USA 7 AO7 X-RAY EMISSION FROM SUPERNOVA REMNANT 1987A XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/707020010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '707020010'

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