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. |
observation_id
|
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
|
exposure
|
awarded_exposure
|
resolve_exposure
|
xtend_exposure
|
resolve_data_mode
|
resolve_with_filter_be
|
resolve_with_filter_fe55
|
resolve_with_filter_nd
|
resolve_with_filter_poly
|
resolve_with_filter_open
|
resolve_with_filter_undef
|
is_resolve_gatevalve_closed
|
is_resolve_mxs1
|
is_resolve_mxs2
|
is_resolve_mxs3
|
is_resolve_mxs4
|
xtend_number_modes
|
xtend_dataclass_file1
|
xtend_dataclass_file2
|
xtend_window1_exposure
|
xtend_window2_exposure
|
xtend_window1_burst_exposure
|
xtend_window2_burst_exposure
|
xtend_code
|
resolve_code
|
gen_code
|
processing_status
|
processing_date
|
public_date
|
distribution_date
|
processing_version
|
caldb_version
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
proposal_type
|
proposal_title
|
observation_status
|
data_access_url
|
xtend_data_mode1
|
xtend_data_mode2
|
processing_count
|
remarks
|
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | 201068010 | GRS1915+105 | 288.79871 | 10.94557 | 288.2088 | 10.85721 | 292.14994 | 32.95063 | 45.36583 | -0.2197 | 259.88992 | 60600.03963 | 2024-10-17 00:57:04 | 60600.90074 | 2024-10-17 21:37:04 | 37.517 | 30.000 | 37.517 | 3.966 | PX_NORMAL | N | Y | N | N | Y | N | Y | OFF | OFF | OFF | OFF | 2 | 31300010 | 320000A0 | 31.661 | 0.000 | 0.000 | 3.966 | 11110 | 313430 | 11310 | PROCESSED | 2024-10-26 06:25:46 | 2025-10-31 00:00:00 | 2024-10-27 06:25:46 | 03.00.013.009 | gen20240315_xtd20240815_rsl20240815 | Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 | 000013007 | After a long period wherein it was the archetype micro-quasar, GRS 1915+105 has spent the last several years in a highly obscured state that evokes Compton- thick AGN like NGC 1068. However, even in its most obscured phases it is an order of magitude brighter than NGC 1068, and it can deliver even deeper insights into accretion and outflows in this universally important mode. We request a 30 ks observation with XRISM to perform line diagnostics that will reveal the relative radial positioning of cold and hot gas components components, whether or not they are bound to the system or escaping, how much mechanical power is being channeled into the flows, and how the flows relate to the large obscuring column density. | BH AND NS BINARIES | 2 | A | JON MILLER | SHOGO KOBAYASHI | USJ | 1 | NOR | GRS 1915+105: FROM MICRO-QUASAR TO MICRO-COMPTON-THICK AGN? | archived | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201068010/ | WINDOW2BURST | WINDOW1 | 1 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '201068010'
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