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 GRO J1655-40 253.5027 -39.8455 252.639975 -39.764411 256.800671 -17.156383 344.98315976 2.45489032 268.0237 53635.3140625 2005-09-22 07:32:15 53636.2968055556 2005-09-23 07:07:24 100029010 35.2228 40 0 35.2336 35.2228 35.2308 0 1 2 2 1 0 0 28.7315 28.7315 84.9019 1 PROCESSED 57527.3997337963 2016-05-19 09:35:37 54247 2007-05-27 00:00:00 54035.4940625 2006-10-27 11:51:27 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000029 We propose to observe GRO J1655-40, a transient galactic black hole candidate. With M=~7 Msolar and distinct radio lobes, GRO J1655-40 has been classified as a microquasar. It was highly variable during the first few years after its discovery while showing irregular flaring and a wide range of continuum states. Discrete Fe K absorption structure was observed with ASCA. In the summer of 1997 it entered an extended quiescence that lasted for ~8 years. In March 2005 it became active again and XMM & Chandra have observed it since. Only Suzaku can provide the broadband sensitivity required to map the Fe K structure and the continuum as they change. GRO J1655-40 is rapidly declining and must be observed soon before it reenters quiescence. CALIBRATION 1 A SWG JAP 0 SWG GRO J1655-40 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100029010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '100029010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏