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
|
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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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