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 4U1626-67 248.0601 -67.4675 246.801189 -67.3606 258.324109 -44.911512 321.78071552 -13.09322804 103.0359 53803.0543518518 2006-03-09 01:18:16 53805.818275463 2006-03-11 19:38:19 400015010 102.6392 100 102.654 102.6392 102.6472 102.654 2 2 2 2 1 0 0 93.3932 93.3932 238.7819 3 PROCESSED 57533.2349652778 2016-05-25 05:38:21 54247 2007-05-27 00:00:00 54042.4663657407 2006-11-03 11:11:34 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001081 The X-ray spectrum of the 7 second LMXRB pulsar 4U1626-67 is dominated by low energy line emission with little evedence of iron K line in the pulse phase resolved spectra. It showd also cyclotron line at 37 keV that departs from the correlation of energy cutoff cyclotron energy observed in many other X-ray pulsars. This Suzaku observation allow to characterize the overall continuum, the low energy, the iron K alpha and cyclotron lines as function of the pulse phase, GALACTIC POINT SOURCES 4 A LORELLA ANGELINI JAP 0 SWG 4U1626-67: PHASE RESOLVED SPECTRA AND CYCLOTRON LINE XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400015010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '400015010'

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