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 2005KD 60.8552 71.7156 59.486745 71.577171 76.353108 49.655537 136.84988934 14.24754739 218.8053 54568.8904976852 2008-04-12 21:22:19 54570.0348842593 2008-04-14 00:50:14 703025010 51.6289 50 51.6289 51.6369 0 51.6449 1 1 0 1 1 0 0 63.5726 63.5726 98.8639 1 PROCESSED 57542.2950694444 2016-06-03 07:04:54 54947 2009-04-26 00:00:00 54581.1998842593 2008-04-25 04:47:50 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/ver3.0/703025010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '703025010'

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