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 | GRB060105 | 297.6095 | 46.3384 | 297.227077 | 46.210211 | 319.460988 | 65.110067 | 80.2506255 | 9.98748628 | 191.1906 | 53740.5089351852 | 2006-01-05 12:12:52 | 53741.5002083333 | 2006-01-06 12:00:18 | 900001010 | 42.2208 | 40 | 42.2208 | 42.2208 | 42.2208 | 42.2208 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 37.718 | 37.718 | 85.6419 | 2 | PROCESSED | 57532.6415856482 | 2016-05-24 15:23:53 | 54247 | 2007-05-27 00:00:00 | 54039.776712963 | 2006-10-31 18:38:28 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001008 | (i) Early break in lightcurve of X-ray afterglows using HXD. Recent Swift/XRT observations reveal that early X-ray afterglows of GRB has flat portion with very shallow decay. It may suggest continuous energy input from the central engine. The transition from its phase to general afterglow may display hard-to-soft evolution reflecting the cooling frequency. Thus multi wavelength observation will provide a key to the physics of central engine activity. (ii) Emission lines in the afterglows. The confirmation of line existence should be a matter of great importance because there remains unanswered questions. Some data may indicate a prominent iron line but others seem to suggest significant lower energy lines instead without iron lines. | EXTRAGALACTIC COMPACT SOURCES | 9 | A | TOSHIO MURAKAMI | JAP | 0 | SWG-TOO | TOO OBSERVATIONS OF GAMMA-RAY BURSTS | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/900001010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '900001010'
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