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 | SN 2006JD | 120.5331 | 0.8102 | 119.888824 | 0.950282 | 122.553341 | -19.245849 | 220.45612728 | 16.05834455 | 284.354 | 54578.4377777778 | 2008-04-22 10:30:24 | 54579.6807175926 | 2008-04-23 16:20:14 | 703026010 | 54.1968 | 50 | 54.2048 | 54.1968 | 0 | 54.2048 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 52.0488 | 52.0488 | 107.3398 | 1 | PROCESSED | 57542.379837963 | 2016-06-03 09:06:58 | 54957 | 2009-05-06 00:00:00 | 54588.1523611111 | 2008-05-02 03:39:24 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 031241 | Supernovae (SNe) 2005kd and 2006jd are some of the brightest SNe ever detected in X-rays. The high X-ray luminosities (>E41 erg/s) are the results of the SN shock interacting with dense material in the environment of the SNe. We propose one Suzaku observation of each SN to obtain high-quality spectra that will be used to measure the temperature of the forward and reverse shock and to establish the rate of decline in comparison with existing Swift, Chandra and XMM-Newton data. The data will further be used to measure the circumstellar matter density and mass-loss rate of the progenitors to probe the nature of the SN progenitors. Our science objectives rely on Suzaku's uniqueness, i.e. the large collecting area, good spectral resolution, and the high sensitivity in the hard X-ray band. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | STEFAN IMMLER | USA | 3 | AO3 | SUZAKU OBSERVATIONS OF X-RAY BRIGHT SUPERNOVAE | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703026010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '703026010'
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